BEGIN:VCALENDAR
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PRODID:researchseminars.org
CALSCALE:GREGORIAN
X-WR-CALNAME:researchseminars.org
BEGIN:VEVENT
SUMMARY:Javier Fuentes-Martin
DTSTART:20200903T130000Z
DTEND:20200903T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/1
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 /">Third-family quark-lepton unification with a fundamental composite Higg
 s</a>\nby Javier Fuentes-Martin as part of CERN BSM Forums\n\n\nAbstract\n
 Zoom coordinates below:\n\nhttps://cern.zoom.us/j/99113688676\n\nMeeting I
 D: 991 1368 8676\nOne tap mobile\n+41432107108\,\,99113688676# Switzerland
 \n+41315280988\,\,99113688676# Switzerland\n\nDial by your location\n     
    +41 43 210 71 08 Switzerland\n        +41 31 528 09 88 Switzerland\n   
      +41 43 210 70 42 Switzerland\n        +33 7 5678 4048 France\n       
  +33 1 7037 2246 France\n        +33 1 7037 9729 France\nMeeting ID: 991 1
 368 8676\nFind your local number: https://cern.zoom.us/u/awBF3LWct\n\nJoin
  by SIP\n99113688676@zoomcrc.com\n\nJoin by H.323\n162.255.37.11 (US West)
 \n162.255.36.11 (US East)\n221.122.88.195 (China)\n115.114.131.7 (India Mu
 mbai)\n115.114.115.7 (India Hyderabad)\n213.19.144.110 (EMEA)\n103.122.166
 .55 (Australia)\n209.9.211.110 (Hong Kong\n China)\n64.211.144.160 (Brazil
 )\n69.174.57.160 (Canada)\n207.226.132.110 (Japan)\nMeeting ID: 991 1368 8
 676\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/1/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Joe Davighi
DTSTART:20200917T130000Z
DTEND:20200917T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/2
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 /">Global anomalies in the Standard Model(s) and Beyond</a>\nby Joe Davigh
 i as part of CERN BSM Forums\n\n\nAbstract\nGlobal anomalies in gauge theo
 ries are detected by the exponentiated eta-invariant\, which becomes a cob
 ordism invariant when perturbative anomalies vanish. After giving a gentle
  introduction to these concepts\, I will analyse global anomalies in four 
 distinct (but equally valid) versions of the Standard Model by computing a
 ppropriate bordism groups. In two cases we find no global anomalies beyond
  the famous Witten anomaly associated with electroweak SU(2) symmetry\, wh
 ile in the other two cases there can be no global anomalies at all. This i
 s due to an interplay between local and global anomalies in "closely relat
 ed" gauge theories. If there is time\, I will discuss a more subtle versio
 n of this anomaly interplay occurring in a U(2) gauge theory defined witho
 ut a spin structure\, and/or global anomalies in BSM theories.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/2/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Steven Adam Abel (University of Durham (GB))
DTSTART:20200924T130000Z
DTEND:20200924T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/3
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 /">Quantum Annealers as a Laboratory for Quantum Physics</a>\nby Steven Ad
 am Abel (University of Durham (GB)) as part of CERN BSM Forums\n\n\nAbstra
 ct\nI discuss recent work done with Michael Spannowsky at Durham in which 
 we propose quantum annealers as a \nlaboratory for studying non-perturbati
 ve aspects of quantum mechanics and quantum field theories.  Our approach 
 encodes the field theory as an Ising model\, which is then solved by the a
 nnealer. As a proof-of-concept\, we encode a scalar field theory and measu
 re the probability for it to tunnel from the false to the true vacuum for 
 various tunnelling times\, vacuum displacements and potential profiles. Th
 is is the first time it has been possible to experimentally measure instan
 ton processes in a freely chosen quantum field theory. This novel and flex
 ible probe of quantum systems can in principle be applied to study any fie
 ld theory of interest using genuine quantum experimentation. Measurements 
 of the dynamical behaviour of field theories are independent of theoretica
 l calculations and could be used to infer their properties without being l
 imited by the availability of suitable perturbative or nonperturbative com
 putational methods.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/3/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Majid Ekhterachian
DTSTART:20201001T130000Z
DTEND:20201001T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/4
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 /">Holography of the cosmological phase transition of composite Higgs conf
 inement</a>\nby Majid Ekhterachian as part of CERN BSM Forums\n\n\nAbstrac
 t\nI will discuss the cosmological (de)confinement phase transition (PT) o
 f nearly conformal\, strongly coupled large N field theories\, applicable 
 to composite Higgs models\, using their holographic dual 5D formulation.  
 In this description\, the PT is from the high temperature phase in which t
 he IR of the warped extra dimension is covered by a black-brane horizon to
  the low temperature Randall-Sundrum-1 phase. The PT proceeds by percolati
 on of IR-brane bubbles nucleating from the horizon\, and the bubble dynami
 cs during the PT sources a stochastic gravitational wave background that c
 an be detected by future experiments. I will show how to construct a smoot
 h “bounce” configuration that interpolates between the two phases\, al
 lowing for a controlled description of bubble nucleation within 5D EFT. We
  will see that the cosmological PT in the minimal models can complete only
  after a large period of supercooling\, potentially resulting in excessive
  dilution of primordial matter abundances. I will then show how generic mo
 difications of the minimal models can result in a much faster completion o
 f the PT. Finally\, I will discuss the gravitational wave signal produced 
 by the PT and the implications of the PT for baryogenesis.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/4/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Alexander Monin
DTSTART:20201008T130000Z
DTEND:20201008T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/5
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 /">Multiparticle processes\, large charge and semiclassics</a>\nby Alexand
 er Monin as part of CERN BSM Forums\n\n\nAbstract\nUnderstanding the behav
 ior of a cross section at high enough energies\, when the number of partic
 les in the final state is large\, is an important and yet unsolved subject
 . The difficulty in addressing the question is inapplicability of the stan
 dard perturbation theory for describing processes with many quanta even in
  weakly coupled theories. However\, a certain reorganization (similar to R
 G improvement) of the perturbative expansion indicates a possibility of a 
 semiclassical description: in other words perturbation theory around a non
 -trivial saddle. First\, I’ll present the current state of affairs with 
 regards to a scalar 𝜆𝜙4 theory. And later I’ll show an explicit an
 d consistent construction allowing to compute observables like anomalous d
 imension etc. for operators with arbitrary large charge in 𝑈(1) symmetr
 ic scalar field theory at Wilson-Fisher fixed point.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/5/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Iftah Galon
DTSTART:20201015T130000Z
DTEND:20201015T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/6
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 /">Synchrotron-Like Radiation Beyond The Standard Model I: Hunting for new
  physics with the Sokolov-Ternov effect</a>\nby Iftah Galon as part of CER
 N BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/6/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Jordy de Vries
DTSTART:20201022T130000Z
DTEND:20201022T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/7
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 /">Lepton number violation in effective field theory</a>\nby Jordy de Vrie
 s as part of CERN BSM Forums\n\n\nAbstract\nNext-generation neutrinoless d
 ouble-beta decay (0vbb) experiments\naim to discover lepton number violati
 on in order to shed light on the\nnature of neutrino masses. A non-zero si
 gnal would have profound\nimplications by demonstrating the existence of e
 lementary Majorana\nparticles and possibly pointing towards a solution of 
 matter-antimatter\nasymmetry in the universe. However\, the interpretation
  of the\nexperimental signal (or lack thereof) requires care as complicate
 d\nhadronic and nuclear input is required to connect the experimental data
 \nto a fundamental description of lepton-number violation. In this talk\, 
 I\nuse effective field theories to connect low-energy measurements to the\
 nfundamental lepton-number-violating source. In particular\, I will argue\
 nthat interpretation of neutrinoless double beta decay in terms of light M
 ajorana\nneutrinos is more complicated than normally considered.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/7/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Patrick Foldenauer
DTSTART:20201029T140000Z
DTEND:20201029T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/8
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 /">Light Dark Matter Annihilation and Scattering in LHC Detectors</a>\nby 
 Patrick Foldenauer as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/8/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Ofri Telem
DTSTART:20201119T160000Z
DTEND:20201119T170000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/9
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/9
 /">Scattering Amplitudes for Monopoles: Pairwise Little Group and Pairwise
  Helicity</a>\nby Ofri Telem as part of CERN BSM Forums\n\n\nAbstract\nOn-
 shell methods are particularly suited for exploring the scattering of elec
 trically and magnetically charged objects\, for which there is no local an
 d Lorentz invariant Lagrangian description. In this paper we show how to c
 onstruct a Lorentz-invariant S-matrix for the scattering of electrically a
 nd magnetically charged particles\, without ever having to refer to a Dira
 c string. A key ingredient is a revision of our fundamental understanding 
 of multi-particle representations of the Poincaré group. Surprisingly\, t
 he asymptotic states for electric-magnetic scattering transform with an ad
 ditional little group phase\, associated with pairs of electrically and ma
 gnetically charged particles. The corresponding “pairwise helicity” is
  identified with the quantized “cross product” of charges\, e1g2 − e
 2g1\, for every charge-monopole pair\, and represents the extra angular mo
 mentum stored in the asymptotic electromagnetic field. We define a new kin
 d of pairwise spinor-helicity variable\, which serves as an additional bui
 lding block for electric-magnetic scattering amplitudes. We then construct
  the most general 3-point S-matrix elements\, as well as the full partial 
 wave decomposition for the 2 → 2 fermion-monopole S-matrix. In particula
 r\, we derive the famous helicity flip in the lowest partial wave as a sim
 ple consequence of a generalized spin-helicity selection rule\, as well as
  the full angular dependence for the higher partial waves. Our constructio
 n provides a significant new achievement for the on-shell program\, succee
 ding where the Lagrangian description has so far failed.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/9/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Fotis Farakos
DTSTART:20201126T140000Z
DTEND:20201126T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/10
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 0/">de Sitter decay through goldstino evaporation</a>\nby Fotis Farakos as
  part of CERN BSM Forums\n\n\nAbstract\nWe study the restoration of supers
 ymmetry within systems\nwhere it is intrinsically non-linearly realized an
 d we discuss\nphysical applications of such a procedure related to de Sitt
 er vacua.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/10/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Francesco Riva
DTSTART:20201203T140000Z
DTEND:20201203T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/11
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 1/">Positive Moments for Scattering Amplitudes</a>\nby Francesco Riva as p
 art of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/11/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Juan Carlos Criado Álamo
DTSTART:20210114T140000Z
DTEND:20210114T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/12
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 2/">Electroweak Skyrmions</a>\nby Juan Carlos Criado Álamo as part of CER
 N BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/12/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Gabriele Rigo
DTSTART:20210121T140000Z
DTEND:20210121T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/13
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 3/">Anomaly inflow and holography</a>\nby Gabriele Rigo as part of CERN BS
 M Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/13/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Tzu-Chen Huang
DTSTART:20210128T140000Z
DTEND:20210128T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/14
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 4/">The EFTHedron</a>\nby Tzu-Chen Huang as part of CERN BSM Forums\n\nAbs
 tract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/14/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Diego Redigolo
DTSTART:20210204T140000Z
DTEND:20210204T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/15
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 5/">Ripples in Spacetime from Broken Supersymmetry</a>\nby Diego Redigolo 
 as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/15/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Ferruccio Feruglio
DTSTART:20210211T140000Z
DTEND:20210211T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/16
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 6/">Gauge Anomaly Cancellation in Effective Field Theories</a>\nby Ferrucc
 io Feruglio as part of CERN BSM Forums\n\n\nAbstract\nIn Effective Field T
 heories\, gauge anomalies are expected to be determined by the charge assi
 gnment of the fermion sector\, as in renormalizable theories. Nevertheless
 \, the mechanism of gauge anomaly cancellation is nontrivial and has direc
 t consequences on the computation of physical quantities. By considering a
  simple explicit model that mimics the SMEFT properties and includes a com
 plete set of dimension six operators\, the (candidate) anomaly is evaluate
 d in the regularized theory. The contribution to the anomaly from the non-
 renormalizable sector can be removed by a local counterterm\, having a dir
 ect impact on the computation of scattering amplitudes in perturbation the
 ory.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/16/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Isabel Garcia Garcia
DTSTART:20210218T160000Z
DTEND:20210218T170000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/17
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 7/">P not PQ</a>\nby Isabel Garcia Garcia as part of CERN BSM Forums\n\n\n
 Abstract\nParity solutions to the strong CP problem are a compelling alter
 native to approaches based on Peccei-Quinn symmetry\, particularly given t
 he expected violation of global symmetries in a theory of quantum gravity.
  The most natural of these solutions break parity at a low scale\, giving 
 rise to a host of experimentally accessible signals. We assess the status 
 of the simplest parity-based solution in light of LHC data and flavor cons
 traints\, highlighting the prospects for near-future tests at colliders\, 
 tabletop experiments\, and gravitational wave observatories. The origin of
  parity breaking and associated gravitational effects play crucial roles\,
  providing new avenues for discovery through EDMs and gravity waves. These
  experimental opportunities underline the promise of generalized parity\, 
 rather than Peccei-Quinn symmetry\, as a robust and testable solution to t
 he strong CP problem.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/17/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Rick S. Gupta
DTSTART:20210225T140000Z
DTEND:20210225T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/18
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 8/">A heavy axion/'massless up' from partial compositeness</a>\nby Rick S.
  Gupta as part of CERN BSM Forums\n\n\nAbstract\nWe show that QCD instanto
 ns can generate large effects at small length scales in the ultraviolet in
  standard composite Higgs models that utilise partial compositeness. This 
 has important implications for possible solutions of the strong CP problem
  in these models. First\, we show that in the simplest known UV completion
 s of composite Higgs models\, if an axion is also present\, it can have a 
 mass much larger than the usual QCD axion. Even more remarkable is the cas
 e where there are no axions\, but the strong CP problem can be solved by g
 enerating the up-quark mass entirely from the contribution of instantons t
 hus reviving the massless up-quark solution for these models. In both case
 s no additional field content is required apart from what is required to r
 ealise partial compositeness.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/18/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Nima Arkani-Hamed (IAS)
DTSTART:20210304T140000Z
DTEND:20210304T160000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/19
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/1
 9/">UV/IR\, Celestial Amplitudes\, and the Anti-Wilsonian Paradigm</a>\nby
  Nima Arkani-Hamed (IAS) as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/19/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Raffaele Tito D'agnolo
DTSTART:20210311T140000Z
DTEND:20210311T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/20
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 0/">The Weak Scale as a Trigger</a>\nby Raffaele Tito D'agnolo as part of 
 CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/20/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Yu-Dai Tsai
DTSTART:20210318T140000Z
DTEND:20210318T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/21
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 1/">The High Energy-Intensity Frontier - Resonant Dark Mesons & FORMOSA</a
 >\nby Yu-Dai Tsai as part of CERN BSM Forums\n\n\nAbstract\nI will introdu
 ce a new dark matter model\, resonant self-interacting dark meson (RSIDM)\
 , and talk about its implications on small-scale structure observations an
 d the experimental signatures.\n \nI will then give a general overview of 
 experimental facilities with high energies and high intensities\, focusing
  on proton fixed-target (at Fermilab) and hadron collider experiments (at 
 the LHC). I will classify the searches as "decay" searches and "scattering
 " searches\, and detail the new physics models of interest. These experime
 nts can help close the gap between the low-mass/high-mass gap for the dark
  sector searches\, and the low-energy/high-energy gap for the neutrino stu
 dy.\n\nI will present two new experimental proposals\, LongQuest and FORMO
 SA. LongQuest is a multi-purpose proton fixed-target experiment\, studying
  the decay particles\, including dark photons and axion-like particles. FO
 RMOSA is a specialized LHC forward experiment that is the world-most sensi
 tive proposal to study millicharged particles\, and also has the potential
  ability to study heavy neutrino and tau neutrino dipole moments.\n\nFinal
 ly\, I will discuss the possibility of constructing liquid Argon neutrino 
 detectors at the LHC forward physics region to study high-energy neutrino 
 cross-sections\, named nu-FLArE. This talk is based on arXiv:2008.08608\, 
 arXiv:1908.07525\, arXiv:2010.07941\, arXiv:1812.03998\, and ongoing works
 .\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/21/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Akshay Ghalsasi
DTSTART:20210325T140000Z
DTEND:20210325T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/22
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 2/">Axions\, Domain Walls\, and Cosmic Strings</a>\nby Akshay Ghalsasi as 
 part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/22/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Azadeh Maleknejad
DTSTART:20210401T130000Z
DTEND:20210401T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/23
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 3/">Is Our Universe the Remnant of Chiral Anomaly in Inflation?</a>\nby Az
 adeh Maleknejad as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/23/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Aritra Gupta
DTSTART:20210408T130000Z
DTEND:20210408T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/24
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 4/">Dark matter capture in Celestial objects: Effect of multi-scattering a
 nd light mediator</a>\nby Aritra Gupta as part of CERN BSM Forums\n\n\nAbs
 tract\nWe revisit dark matter (DM) capture in celestial objects\, includin
 g the impact of multiple scattering\, and obtain updated constraints on th
 e DM-proton cross-section using observations of white dwarfs. Considering 
 a general form for the energy loss distribution in each scattering\, we de
 rive an exact formula for the capture probability through multiple scatter
 ings. We employ these results to compute a “dark” luminosity (LDM)\, a
 rising solely from the thermalized annihilation products of the captured d
 ark matter. Demanding that LDM does not exceed the luminosity of the white
  dwarfs in the M4 globular cluster\, we set a bound on the DM-proton cross
 -section\, almost independent of the dark matter mass between 100 GeV and 
 1 PeV and mildly weakening beyond. This is a stronger constraint than thos
 e obtained by direct detection experiments in both large masses (M>5 TeV) 
 and small mass (M<10 GeV) regimes. For dark matter lighter than 350 MeV\, 
 which is beyond the sensitivity of the present direct detection experiment
 s\, this is the strongest available constraint. Moving further\, we also g
 eneralize the formalism for DM capture in celestial bodies to account for 
 arbitrary mediator mass\, and update the existing and projected astrophysi
 cal constraints on DM-nucleon scattering cross-section from observations o
 f neutron stars. We show that the astrophysical constraints on the DM-nucl
 eon interaction strength\, which were thought to be the most stringent\, d
 rastically weaken for light mediators and can be completely voided.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/24/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Nick Rodd
DTSTART:20210415T150000Z
DTEND:20210415T160000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/25
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 5/">New ideas for the axion dark matter program</a>\nby Nick Rodd as part 
 of CERN BSM Forums\n\n\nAbstract\nThe coming decade will bring dramatic im
 provement in the axion dark matter program as new experimental designs mov
 e beyond the proof of principle stage. In this talk I will outline two new
  ideas that exploit this experimental progress. The first is to combine th
 e results from two or more instruments in order to perform interferometry 
 directly on the dark-matter wave. This technique reveals aspects of the ax
 ion signal that can be invisible to a single detector\, such as the incide
 nt direction of the dark-matter wave. The second is to search for relativi
 stic axions in these experiments\, in particular future instruments like d
 ark-matter radio will be sensitive to axions produced in the early univers
 e that constitute a residual Cosmic axion Background (CaB). Existing searc
 hes at\, for instance ADMX\, are not yet sensitive to a cosmic relic\, alt
 hough if relativistic axions are produce in the late universe\, by for ins
 tance dark-matter decaying to axions\, then this is a signal the experimen
 ts are already sensitive to\, but would miss with existing analyses.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/25/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Ilja Dorsner
DTSTART:20210429T130000Z
DTEND:20210429T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/26
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 6/">Novel Leptoquark Pair Production at LHC</a>\nby Ilja Dorsner as part o
 f CERN BSM Forums\n\n\nAbstract\nI will introduce two novel mechanisms to 
 produce pairs of leptoquarks at Large Hadron Collider and present several 
 case studies to discuss the associated phenomenological implications.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/26/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Sophie Renner
DTSTART:20210506T130000Z
DTEND:20210506T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/27
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 7/">The flavour phenomenology of ALP EFTs</a>\nby Sophie Renner as part of
  CERN BSM Forums\n\n\nAbstract\nAxion-like particles (ALPs) are a generic 
 and well-motivated class of BSM particles\, which have a rich phenomenolog
 y. I will discuss the effective field theory of a general axion-like parti
 cle in the MeV to GeV mass range\, focussing on its flavour changing effec
 ts. Starting from the UV scale\, I’ll describe its running and matching 
 through the electroweak scale and down to the scale of flavour measurement
 s. I’ll focus on a calculation of ALP effects in kaon decays within the 
 framework of chiral perturbation theory\, and discuss other flavour constr
 aints in this mass range\, expressed in terms of the fundamental ALP coupl
 ings at the UV scale.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/27/
END:VEVENT
BEGIN:VEVENT
SUMMARY:David B. Kaplan
DTSTART:20210527T150000Z
DTEND:20210527T160000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/28
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 8/">Gravitational contributions to the electron g-factor</a>\nby David B. 
 Kaplan as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/28/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Benjamin Allanach
DTSTART:20210520T140000Z
DTEND:20210520T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/29
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/2
 9/">Solving the u(1)xSM anomaly equations</a>\nby Benjamin Allanach as par
 t of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/29/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Zohar Komargodski
DTSTART:20210603T130000Z
DTEND:20210603T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/30
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 0/">The very high temperature limit of QFT</a>\nby Zohar Komargodski as pa
 rt of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/30/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Slava Mukhanov
DTSTART:20210610T130000Z
DTEND:20210610T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/31
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 1/">Quantum fluctuations and new instantons</a>\nby Slava Mukhanov as part
  of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/31/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Admir Greljo
DTSTART:20210617T130000Z
DTEND:20210617T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/32
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 2/">A Model of Muon Anomalies</a>\nby Admir Greljo as part of CERN BSM For
 ums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/32/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Jack Shergold
DTSTART:20210701T130000Z
DTEND:20210701T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/33
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 3/">talk by Jack Shergold</a>\nby Jack Shergold as part of CERN BSM Forums
 \n\n\nAbstract\nWe present a new technique for observing low energy\nneutr
 inos with the aim of detecting the cosmic neutrino background\nusing ion s
 torage rings. Utilising high energy targets exploits the\nquadratic increa
 se in the neutrino capture cross section with beam\nenergy\, and with suff
 icient beam energy\, enables neutrino capture\nthrough inverse-beta decay 
 processes from a stable initial state. We\nalso show that there exist ion 
 systems admitting resonant neutrino\ncapture\, capable of achieving larger
  capture cross sections at lower\nbeam energies than their non-resonant co
 unterparts. We calculate the\nneutrino capture rate and the optimal experi
 mental runtime for a range\nof different resonant processes and target ion
 s and we demonstrate that\nthe resonant capture experiment can be performe
 d with beam energies as\nlow as O(10TeV) per target nucleon. Unfortunately
 \, none of the ion\nsystems discussed here can provide sufficient statisti
 cs to discover\nthe cosmic neutrino background with current technology. We
  address the\nchallenges associated with realising this experiment in the 
 future\,\ntaking into account the uncertainty in the beam and neutrino mom
 entum\ndistributions\, synchrotron radiation\, as well as the beam stabili
 ty.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/33/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Ken Van Tilburg
DTSTART:20210708T130000Z
DTEND:20210708T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/34
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 4/">Results and simulations for solar basins of light bosonic particles</a
 >\nby Ken Van Tilburg as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/34/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Tobias Binder
DTSTART:20210715T130000Z
DTEND:20210715T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/35
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 5/">Non-equilibrium theory of non-relativistic pairs inside an environment
 </a>\nby Tobias Binder as part of CERN BSM Forums\n\n\nAbstract\nWe derive
  differential equations from path-integral-based non-equilibrium quantum f
 ield theory that cover the dynamics and spectrum of non-relativistic two-b
 ody fields for any environment. For concreteness of the two-body fields\, 
 we choose the full potential non-relativistic quantum electrodynamics Lagr
 angian in this work. After closing the correlation function hierarchy of t
 hese equations and performing consistency checks with previous literature 
 under certain limits\, we demonstrate the range of physics applications. T
 his includes cosmology such as dark matter in the primordial plasma\, quar
 konia inside a quark-gluon plasma\, and other phenomena in condensed or st
 rongly correlated matter physics.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/35/
END:VEVENT
BEGIN:VEVENT
SUMMARY:ANUPAM RAY
DTSTART:20210729T130000Z
DTEND:20210729T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/36
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 6/">Mergers as a Probe of Particle Dark Matter</a>\nby ANUPAM RAY as part 
 of CERN BSM Forums\n\n\nAbstract\nUnusual masses of the black holes being 
 discovered by gravitational wave experiments pose fundamental questions ab
 out the origin of these black holes. More interestingly\, black holes with
  masses smaller than the Chandrasekhar limit (~1.4 solar mass)? are essent
 ially impossible to produce through any standard stellar evolution. Black 
 holes of primordial origin\, with fine-tuned parameters and with no well-e
 stablished formation mechanisms\, are the most discussed explanation of th
 ese objects. In this talk\, I will discuss a simple and elegant production
  channel of sub-Chandrasekhar mass non-primordial black holes. Particle da
 rk matter with no antiparticle counterpart\, owing to their interaction wi
 th stellar nuclei\, can catastrophically accumulate inside compact stars a
 nd eventually transmute them to sub-Chandrasekhar mass black holes. Our re
 cent work points out several avenues to test the transmuted origin of low 
 mass black holes\, and demonstrates that binary merger rates at high redsh
 ift are distinctively different for primordial and transmuted black holes.
  Measurement of these binary merger rates by the imminent gravitational wa
 ve detectors can conclusively determine the origin of low mass black holes
 .\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/36/
END:VEVENT
BEGIN:VEVENT
SUMMARY:James Mangan
DTSTART:20210930T110000Z
DTEND:20210930T120000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/37
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 7/">Covariant Color-Kinematics Duality</a>\nby James Mangan as part of CER
 N BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/37/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Volodymyr Takhistov
DTSTART:20211007T113000Z
DTEND:20211007T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/38
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 8/">Exploring Depths of the Dark: Neutrinos\, Axion Explosions and Multive
 rse Black Holes</a>\nby Volodymyr Takhistov as part of CERN BSM Forums\n\n
 \nAbstract\nWhat is dark matter\, the mysterious predominant constituent o
 f all matter in the Universe? While particle dark matter has eluded detect
 ion thus far\, as I will demonstrate\, large dark matter experiments thems
 elves form impressive neutrino telescopes. This opens a new window into as
 tronomy as well as major problems such as the origin of supermassive black
  holes. Drawing on lessons from neutrino astronomy\, I will also show how 
 signatures from transient sources could lead to new insights into the fund
 amental properties of axions. I will then demonstrate how intimate connect
 ions with astronomical puzzles as well as ongoing boom in gravitational wa
 ve and multi-messenger astronomy are particularly pronounced for primordia
 l black holes from the early Universe that make an attractive non-particle
  dark matter candidate. In fact\, primordial black holes from the general 
 formation scenario of bubble multiverse might have already been seen by Su
 baru Hyper Suprime-Cam.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/38/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Disha Bhatia
DTSTART:20211014T113000Z
DTEND:20211014T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/39
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/3
 9/">Frugal 𝑈(1)𝑋 models with non-minimal flavor violation for 𝑏
 →𝑠ℓℓ anomalies and neutrino mixings</a>\nby Disha Bhatia as part 
 of CERN BSM Forums\n\n\nAbstract\nWe present a class of 𝑈(1)𝑋 models
  which are can simultaneously explain the neutrino mixings and flavor anom
 alies in neutral B decays. The frugal set up apart from additional 𝑍′
 \, requires additional singlet scalar for neutrino mixings and an addition
 al scalar doublet for quark mixings. Our set up identifies a class of symm
 etries wherein all generations of quarks are necessarily charged\, renderi
 ng collider constraints to be stringent. We show all our models with the a
 ssumption of CKM-like mixings are ruled out from the current data. Introdu
 ction of a single source parameter for non-minimal mixings allows for a wi
 der class of models consistent with the data. We show the viable symmetry 
 patterns are of the form 𝐿𝑒−3𝐿𝜇−𝐿𝜏\, 𝐿𝑒−3
 𝐿𝜇+𝐿𝜏\, and 𝐿𝑒+3𝐿𝜇−𝐿𝜏.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/39/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Joshua Foster
DTSTART:20211021T113000Z
DTEND:20211021T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/40
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 0/">Adaptive Mesh Refinement Simulations of Post-Inflationary Axion Misali
 gnment</a>\nby Joshua Foster as part of CERN BSM Forums\n\n\nAbstract\nAxi
 ons are hypothetical particles that may explain the observed dark matter (
 DM) density and the non-observation of a neutron electric dipole moment. A
 n increasing number of axion laboratory searches are underway worldwide\, 
 but these efforts are made difficult by the fact that the axion mass is la
 rgely unconstrained. If the axion is generated after inflation\, a unique 
 mass gives rise to the observed DM abundance\; due to nonlinearities and t
 opological defects known as strings\, computing this mass accurately has b
 een a challenge for four decades. Recent works using large static lattice 
 simulations have led to largely disparate predictions for the axion mass\,
  spanning the range from 25 microelectronvolts to over 500 microelectronvo
 lts. However\, static lattices are intrinsically limited for studies of ax
 ion cosmology\, which requires both large simulation volumes and good spat
 ial resolution of strings to accurately capture the relevant physics. As I
  will show\, simulations using adaptive mesh refinement\, a technique for 
 solving systems of partial differential equations on a dynamic non-uniform
  lattice\, are better suited for this context since only the string cores 
 require high spatial resolution. Using dedicated AMR simulations\, we achi
 eve an over three-order-of-magnitude leap in dynamic range and provide evi
 dence that axion strings radiate their energy with a scale-invariant spect
 rum\, leading to a mass prediction in the range (40\,180) microelectronvol
 ts.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/40/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Felix Kling
DTSTART:20211028T113000Z
DTEND:20211028T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/41
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 1/">Forward Physics Facility: Sites\, Experiments\, and Physics Potential<
 /a>\nby Felix Kling as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/41/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Marat Freytsis
DTSTART:20211111T123000Z
DTEND:20211111T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/42
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 2/">Particle Physics with Quantum Computers</a>\nby Marat Freytsis as part
  of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/42/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Brian Shuve
DTSTART:20211118T150000Z
DTEND:20211118T160000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/43
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 3/">Neutrino and Leptogenesis</a>\nby Brian Shuve as part of CERN BSM Foru
 ms\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/43/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Apostolos Pilaftsis
DTSTART:20211125T123000Z
DTEND:20211125T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/44
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 4/">Are We Already Living on a Supermanifold?</a>\nby Apostolos Pilaftsis 
 as part of CERN BSM Forums\n\n\nAbstract\nFor more than half a century\, c
 ovariant and differential geometric methods have been playing a central ro
 le in the development of Quantum Field Theory (QFT).  After a brief histor
 ic overview of the major scientific achievements using these methods\, I w
 ill focus on the covariant and differential geometric formalism originally
  proposed by Vilkovisky and DeWitt (VDW).  I will discuss recent developme
 nts made in addressing the uniqueness of the path-integral measure of the 
 VDW effective action\, and so address the problem of quantum frame depende
 nce in cosmologically relevant scalar-tensor theories beyond the classical
  approximation.  I will then turn my attention to a long-standing problem 
 concerning the obstacles that the VDW formalism is facing from its origina
 l conception in describing generic QFTs that include fermions. I will show
  how in addition to bosons the VDW effective action can be extended to sup
 ermanifolds to include fermions.  The so-extended formulation appears to b
 e very promising for a complete geometrisation of realistic theories of mi
 cro-cosmos\, such as the Standard Model and its gravitational sector.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/44/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Itay Bloch
DTSTART:20211202T123000Z
DTEND:20211202T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/45
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 5/">The NASDUCK collaboration: using quantum magnetometers to look for ult
 ralight dark matter</a>\nby Itay Bloch as part of CERN BSM Forums\n\n\nAbs
 tract\nWhen DM bosons have an ultra-light mass\, they can act as a classic
 al\, coherent field. In many cases\, and specifically in some ALP models\,
  this field has magnetic properties\, and it can therefore be measured by 
 quantum magnetometers. The Noble and Alkali Spin Detectors for Ultralight 
 Coherent darK matter (NASDUCK) collaboration\, was formed last year in ord
 er to measure such DM. Recently\, the collaboration released its first res
 ults from the "NASDUCK-Floquet" experiment\, which looks for DM roughly in
  the femto to pico eV mass range. The new experiment places the most strin
 gent terrestrial constraints to date on ultra-light axion-like particles c
 oupled to neutrons. The constraints are comparable to those from stellar c
 ooling\, providing a complementary probe. In my talk I will discuss the th
 eory behind the NASDUCK-Floquet experiment. I will also discuss future pro
 spects of the NASDUCK collaboration\, and some of our planned experiments.
 \n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/45/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Sebastian Ellis
DTSTART:20211209T123000Z
DTEND:20211209T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/46
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 6/">Stellar Shocks</a>\nby Sebastian Ellis as part of CERN BSM Forums\n\nA
 bstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/46/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Ofri Telem
DTSTART:20220113T150000Z
DTEND:20220113T160000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/47
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 7/">Confinement and Chiral Symmetry Breaking in Near-SUSY Theories</a>\nby
  Ofri Telem as part of CERN BSM Forums\n\n\nAbstract\nThe study of non-sup
 ersymmetric\, strongly coupled gauge theories is notoriously hard\, and ex
 act results are scarce. In this talk\, I present a new way to study the va
 cua of near-supersymmetric theories by perturbing their supersymmetric ver
 sions with Anomaly Mediated Supersymmetry Breaking (AMSB). Thanks to the U
 V-insensitivity of AMSB\, SUSY results can be perturbed with no ambiguitie
 s\, even when applied to composite fields. Using our method\, we analyze t
 he phases of 𝑆𝑂(𝑁) gauge theory with flavors. The abelian Coulomb
  and free magnetic phases do not survive supersymmetry breaking and collap
 se to a confining phase\, providing one of the first demonstrations of tru
 e confinement with chiral symmetry breaking in a non-supersymmetric vacuum
 . Our results are exact in the small SUSY breaking limit\, and we briefly 
 discuss the prospects of extrapolating them to large SUSY breaking.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/47/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Joseph Davighi
DTSTART:20220127T123000Z
DTEND:20220127T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/48
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 8/">Electroweak flavour unification</a>\nby Joseph Davighi as part of CERN
  BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/48/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Daniele Teresi
DTSTART:20220203T123000Z
DTEND:20220203T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/49
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/4
 9/">Sliding Naturalness</a>\nby Daniele Teresi as part of CERN BSM Forums\
 n\n\nAbstract\nI will present a novel framework to solve simultaneously th
 e electroweak hierarchy problem and the strong-CP problem. A small but fin
 ite Higgs vacuum expectation value and a small θ-angle are selected after
  the QCD phase transition\, without relying on the Peccei-Quinn mechanism 
 or other traditional solutions. This novel solution predicts a distinctive
  pattern of correlated signals at hadronic EDM\, fuzzy dark matter and axi
 on experiments. I will then discuss other incarnations of the mechanism in
  more generality\, with different phenomenology\, and attempt to draw a (r
 elatively) unified picture of cosmological approaches to the Higgs hierarc
 hy problem.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/49/
END:VEVENT
BEGIN:VEVENT
SUMMARY:David William Sutherland
DTSTART:20220217T123000Z
DTEND:20220217T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/50
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 0/">SMEFT vs HEFT</a>\nby David William Sutherland as part of CERN BSM For
 ums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/50/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Gauthier Durieux
DTSTART:20220224T123000Z
DTEND:20220224T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/51
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 1/">Amplitudes</a>\nby Gauthier Durieux as part of CERN BSM Forums\n\nAbst
 ract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/51/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Kevin James Kelly
DTSTART:20220303T123000Z
DTEND:20220303T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/52
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 2/">Looking for Right-Handed Neutrinos in all the Wrong(?) Places</a>\nby 
 Kevin James Kelly as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/52/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Juri Smirnov
DTSTART:20220310T123000Z
DTEND:20220310T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/53
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 3/">Thermal Squeezeout of Dark Matter and local Accidental Asymmetry</a>\n
 by Juri Smirnov as part of CERN BSM Forums\n\n\nAbstract\nI will discuss  
 a detailed study of the confinement phase transition in a dark sector with
  a SU (N ) gauge group and a single generation of dark heavy quark. We foc
 us on heavy enough quarks such that their abundance freezes out before the
  phase transition and the phase transition is of first-order. We find that
  during this phase transition the quarks are trapped inside contracting po
 ckets of the deconfined phase and are compressed enough to interact at a s
 ignificant rate\, giving rise to a second stage of annihilation that can d
 ramatically change the resulting dark matter abundance. As a result\, the 
 dark matter can be heavier than the often-quoted unitarity bound of ∼ 10
 0 TeV.\n\nFinally I will show a concrete example where the link between th
 e dark sector and the standard model is facilitated by a simple Z’ model
 .\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/53/
END:VEVENT
BEGIN:VEVENT
SUMMARY:David Kaplan
DTSTART:20220317T123000Z
DTEND:20220317T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/54
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 4/">A Modification of Quantum Mechanics</a>\nby David Kaplan as part of CE
 RN BSM Forums\n\n\nAbstract\nWe present a modification of quantum mechanic
 s in which a specific class of state-dependent term is added to the Schroe
 dinger Equation.  We show that this term produces non-trivial effects whic
 h amount to the ‘wave function talking to itself’.  We show that these
  effects are nevertheless causal (don’t violate relativity) while having
  profound experimental consequences.  We also show that this modification 
 has a simple embedding in local quantum field theory.  While the physical 
 effects are dramatic\, they are also fickle\, in that their strength depen
 ds on the cosmological history of the wave function of the universe.  We w
 ill present proposals for laboratory (e.g.\, AMO)\, astrophysical\, and co
 smological tests that could be done to discover such an effect.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/54/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Justin Khoury
DTSTART:20220324T150000Z
DTEND:20220324T160000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/55
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 5/">Criticality in Eternal Inflation</a>\nby Justin Khoury as part of CERN
  BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/55/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Tania Robens
DTSTART:20220331T113000Z
DTEND:20220331T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/56
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 6/">Extended scalar sectors at current and future colliders</a>\nby Tania 
 Robens as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/56/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Latham Boyle
DTSTART:20220407T140000Z
DTEND:20220407T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/57
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 7/">A two-sheeted\, CPT-symmetric universe</a>\nby Latham Boyle as part of
  CERN BSM Forums\n\n\nAbstract\nAfter reviewing some key hints and puzzles
  from the early universe\, I will introduce recent work with Neil Turok su
 ggesting a rigid and predictive new approach to addressing them.\n\nOur un
 iverse seems to be dominated by radiation at early times\, and positive va
 cuum energy at late times.  Taking the symmetry and analyticity properties
  of such a universe seriously suggests a picture in which spacetime has tw
 o sheets\, exchanged by a symmetry that\, in turn\, selects a preferred (C
 PT-symmetric) vacuum state for the quantum fields that live on the spaceti
 me.  In this picture\, the Big Bang may be regarded as a kind of mirror.  
 \n\nI will explain how this line of thought suggests new explanations for 
 a number of observed properties of the universe\, including: its homogenei
 ty\, isotropy and flatness\; the arrow of time\; several properties of the
  primordial perturbations\; the nature of dark matter (which\, in this pic
 ture\, is a right-handed neutrino\, radiated from the Big Bang like Hawkin
 g radiation from a black hole)\; and even the existence of three generatio
 ns of standard model fermions.  I will also mention some observational pre
 dictions that will be tested in the coming decade\, and some key open ques
 tions.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/57/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Valerie Domcke
DTSTART:20220414T113000Z
DTEND:20220414T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/58
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 8/">A novel search for high-frequency gravitational waves with low-mass ax
 ion haloscopes</a>\nby Valerie Domcke as part of CERN BSM Forums\n\nAbstra
 ct: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/58/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Liam McAllister
DTSTART:20220421T130000Z
DTEND:20220421T140000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/59
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/5
 9/">PQ Axiverse</a>\nby Liam McAllister as part of CERN BSM Forums\n\nAbst
 ract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/59/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Yuber Perez-Gonzalez
DTSTART:20220428T113000Z
DTEND:20220428T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/60
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 0/">Primordial Black Holes as Particle Factories in the Early Universe</a>
 \nby Yuber Perez-Gonzalez as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/60/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Marzia Bordone
DTSTART:20220505T113000Z
DTEND:20220505T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/61
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 1/">The Vcb puzzle</a>\nby Marzia Bordone as part of CERN BSM Forums\n\nAb
 stract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/61/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Benjamin Stefanek
DTSTART:20220512T113000Z
DTEND:20220512T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/62
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 2/">Flavor hierarchies\, flavor anomalies\, and the Higgs mass from a warp
 ed extra dimension</a>\nby Benjamin Stefanek as part of CERN BSM Forums\n\
 nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/62/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Sarah Geller
DTSTART:20220519T113000Z
DTEND:20220519T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/63
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 3/">Primordial Black Holes from Multifield Inflation with Non-minimal Coup
 lings</a>\nby Sarah Geller as part of CERN BSM Forums\n\n\nAbstract\nPrimo
 rdial Black Holes (PBHs)\, first postulated more than half a century ago\,
  remain an active and fascinating area of research and provide an exciting
  prospect for accounting for Dark Matter. In this talk I will discuss the 
 possibilities for production of PBHs near to Dark Matter mass scales from 
 realistic multi-field inflation models that arise naturally from supergrav
 ity. These models fit neatly within the current status of inflationary mod
 els as constrained by CMB observations\; they behave effectively as a sing
 le-field models for much of their evolution\, and the isocurvature modes r
 emain heavy throughout. Moreover\, such models yield efficient post-inflat
 ion reheating with N_reh ~ O(1) e-folds after the end of inflation. I will
  demonstrate how our two-field model in particular gives rise to inflation
 ary dynamics that yield predictions for observables in close agreement wit
 h recent empirical data\, such as the spectral index and ratio of power sp
 ectra for tensor to scalar perturbations. As has been noted in previous st
 udies of PBH formation resulting from a period of ultra slow-roll inflatio
 n\, we found that at least one dimensionless parameter must be highly fine
 -tuned\, but I will show that we nonetheless find such models yield accura
 te predictions for a significant number of observable quantities using a s
 maller number of free parameters.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/63/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Henning Bahl
DTSTART:20220602T113000Z
DTEND:20220602T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/64
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 4/">CP violation in the Higgs sector by Henning Bahl</a>\nby Henning Bahl 
 as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/64/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Josef Pradler
DTSTART:20220616T113000Z
DTEND:20220616T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/65
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 5/">The photon mass as the portal to new physics</a>\nby Josef Pradler as 
 part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/65/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Elena Pinetti
DTSTART:20220623T113000Z
DTEND:20220623T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/66
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 6/">Particle dark matter searches with cosmic voids</a>\nby Elena Pinetti 
 as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/66/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Alex Pomarol
DTSTART:20220630T113000Z
DTEND:20220630T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/67
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 7/">Wilson Coefficients and Natural Zeros from the On-Shell Viewpoint</a>\
 nby Alex Pomarol as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/67/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Simone Blasi
DTSTART:20220707T113000Z
DTEND:20220707T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/68
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 8/">Domain walls seeding the electroweak phase transition</a>\nby Simone B
 lasi as part of CERN BSM Forums\n\n\nAbstract\nTopological defects can act
  as local impurities that seed cosmological phase transitions. We will foc
 us on domain walls and discuss their impact on the electroweak phase trans
 ition in the minimal extension of the SM including a scalar singlet (xSM)\
 , odd under a Z_2 symmetry. When the transition is two-step\, the early br
 eaking of the Z_2 implies the formation of domain walls\, which can then a
 ct as seeds for the second and final step. The rate of the seeded phase tr
 ansition can be evaluated within a 3d theory on the domain wall surface\, 
 and it is generically faster than the standard homogeneous tunneling. We w
 ill comment on the phenomenological implications of this type of transitio
 n.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/68/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Tom Melia
DTSTART:20220714T113000Z
DTEND:20220714T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/69
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/6
 9/">Time evolution in quantum cosmology</a>\nby Tom Melia as part of CERN 
 BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/69/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Alex Pomarol
DTSTART:20220721T113000Z
DTEND:20220721T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/70
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 0/">Wilson Coefficients and Natural Zeros from the On-Shell Viewpoint</a>\
 nby Alex Pomarol as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/70/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Diego Blas Temino
DTSTART:20220728T113000Z
DTEND:20220728T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/71
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 1/">Bridging gaps and jumping into the void: new opportunities in the spec
 trum of GWs</a>\nby Diego Blas Temino as part of CERN BSM Forums\n\n\nAbst
 ract\nIn this talk I’ll highlight the existence of gaps in the spectrum 
 of GWs poorly explored by current observations and that may contain inform
 ation about BSM physics or primordial cosmology. I’ll focus on the muHz 
 gap\, and explain how to use the resonance absorption of GWs by binary sys
 tems (as the Earth-Moon system or binary pulsars) to access this band. I
 ’ll also highlight the potential of high frequency (\\omega > kHz) GWs. 
 The focus of this second part will be the use of cavities to detect these 
 signals\, together with a brief discussion of sources and what can be lear
 ned from them.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/71/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Dong Woo Kang
DTSTART:20220811T113000Z
DTEND:20220811T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/72
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 2/">Cosmic birefringence mediated by dark U(1)</a>\nby Dong Woo Kang as pa
 rt of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/72/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Rachel Houtz
DTSTART:20220825T113000Z
DTEND:20220825T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/73
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 3/">Discrete Goldstone Bosons</a>\nby Rachel Houtz as part of CERN BSM For
 ums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/73/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Nicholas Llewellyn Rodd
DTSTART:20220901T113000Z
DTEND:20220901T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/74
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 4/">Positivity and the Topography of the SMEFT</a>\nby Nicholas Llewellyn 
 Rodd as part of CERN BSM Forums\n\n\nAbstract\nIf the UV completion of the
  Standard Model (SM) is unitary\, local\, and causal\, then a rigid struct
 ure emerges in the IR description of the physics provided by the SMEFT. In
  this talk I will outline how these restrictions emerge\, describe how the
 y apply to the SMEFT\, and mention the experimental implications\, includi
 ng for existing collider searches. The constraints require the positivity 
 of various SMEFT Wilson coefficients\, but also require a deep connection 
 between effects that conserve and violate flavor and CP in the theory. I w
 ill present the sharp statements that can be made at dimension eight\, but
  also detail what additional assumptions are required to extend the result
 s to dimension six.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/74/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Rafael Aoude
DTSTART:20220922T113000Z
DTEND:20220922T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/75
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 5/">Classical gravitational scattering from spinning amplitudes</a>\nby Ra
 fael Aoude as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/75/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Chia-Hsien Shen
DTSTART:20220929T140000Z
DTEND:20220929T150000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/76
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 6/">Radiated Angular Momentum and Dissipative Effects in Classical Scatter
 ing</a>\nby Chia-Hsien Shen as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/76/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Nico Gubernari
DTSTART:20221013T113000Z
DTEND:20221013T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/77
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 7/">Standard Model Predictions and Global Fits for 𝑏→𝑠𝜇+𝜇-</
 a>\nby Nico Gubernari as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/77/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Gilly Elor
DTSTART:20221020T113000Z
DTEND:20221020T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/78
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 8/">Mesogenesis</a>\nby Gilly Elor as part of CERN BSM Forums\n\nAbstract:
  TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/78/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Reuven Balkin
DTSTART:20221027T113000Z
DTEND:20221027T123000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/79
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/7
 9/">Searching for light new physics from stars to tabletop</a>\nby Reuven 
 Balkin as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/79/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Andreas Helset
DTSTART:20221103T123000Z
DTEND:20221103T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/80
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 0/">Geometry in Scattering Amplitudes</a>\nby Andreas Helset as part of CE
 RN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/80/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Alan Barr
DTSTART:20221110T123000Z
DTEND:20221110T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/81
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 1/">Quantum foundations at colliders</a>\nby Alan Barr as part of CERN BSM
  Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/81/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Yonatan Kahn
DTSTART:20221117T133000Z
DTEND:20221117T143000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/82
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 2/">Axion wind detection with the homogeneous precession domain of superfl
 uid helium-3</a>\nby Yonatan Kahn as part of CERN BSM Forums\n\nAbstract: 
 TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/82/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Cedric Delaunay
DTSTART:20221124T123000Z
DTEND:20221124T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/83
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 3/">Muon magnetic moment from Muonium</a>\nby Cedric Delaunay as part of C
 ERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/83/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Jeremie Quevillon
DTSTART:20221208T123000Z
DTEND:20221208T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/84
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 4/">From axions to quantum anomalies with EFTs</a>\nby Jeremie Quevillon a
 s part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/84/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Julia Gehrlein
DTSTART:20230112T123000Z
DTEND:20230112T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/85
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 5/">New neutrino interactions and where to find them.</a>\nby Julia Gehrle
 in as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/85/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Peter Stangl
DTSTART:20230119T123000Z
DTEND:20230119T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/86
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 6/">Automating BSM Phenomenology</a>\nby Peter Stangl as part of CERN BSM 
 Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/86/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Vedran Brdar
DTSTART:20230126T123000Z
DTEND:20230126T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/87
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 7/">The Neutrino Magnetic Moment Portal: Phenomenology and UV Completions<
 /a>\nby Vedran Brdar as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/87/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Prof. Sungwoo Hong
DTSTART:20230202T123000Z
DTEND:20230202T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/88
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 8/">Neutrino Masses from Generalized Symmetry Breaking</a>\nby Prof. Sungw
 oo Hong as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/88/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Gilad Perez
DTSTART:20230209T123000Z
DTEND:20230209T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/89
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/8
 9/">New insights on ultralight dark matter searches: oscillating charge ra
 dius and solar halo</a>\nby Gilad Perez as part of CERN BSM Forums\n\nAbst
 ract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/89/
END:VEVENT
BEGIN:VEVENT
SUMMARY:THOMAS HAMBYE
DTSTART:20230216T123000Z
DTEND:20230216T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/90
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/9
 0/">Gauge symmetry stabilization of the dark matter particles</a>\nby THOM
 AS HAMBYE as part of CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/90/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Mario Reig
DTSTART:20230223T123000Z
DTEND:20230223T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/91
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/9
 1/">Axion couplings in Grand Unified Theories</a>\nby Mario Reig as part o
 f CERN BSM Forums\n\n\nAbstract\nIn this talk (based on 2206.07053) I disc
 uss axion couplings to gauge bosons in Grand Unified Theories where the St
 andard Model is embedded in a simple 4D gauge group. The topological natur
 e of these couplings allows them to be matched from the UV to the IR\, and
  the ratio of the anomaly with photons and gluons for any axion is fixed b
 y unification. I will show that this implies that there is a single axion\
 , the QCD axion\, with an anomalous coupling to photons. Other light axion
 -like particles can couple to photons by mixing through the QCD axion port
 al and lie to the right of the QCD line prediction in the mass-coupling pl
 ane. Axions which break the unification relation between gluon and photon 
 couplings are necessarily charged under the GUT gauge group and become hea
 vy from perturbative mass contributions. A discovery of an axion to the le
 ft of the QCD line can rule out simple Grand Unified models.\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/91/
END:VEVENT
BEGIN:VEVENT
SUMMARY:(TBC)
DTSTART:20230316T123000Z
DTEND:20230316T133000Z
DTSTAMP:20260422T212603Z
UID:CERNbsmFor/92
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CERNbsmFor/9
 2/">Dark matter searches with atom interferometry</a>\nby (TBC) as part of
  CERN BSM Forums\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/CERNbsmFor/92/
END:VEVENT
END:VCALENDAR