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BEGIN:VEVENT
SUMMARY:Hans Ringström (KTH Stockholm)
DTSTART:20201001T133000Z
DTEND:20201001T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/1
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/1/">
 On highly anisotropic big bang singularities</a>\nby Hans Ringström (KTH 
 Stockholm) as part of JoMaReC - Joint Online Mathematical Relativity Collo
 quium\n\n\nAbstract\nIn cosmology\, the universe is typically modelled by 
 spatially homogeneous and isotropic solutions to Einstein’s equations. H
 owever\, for large classes of matter models\, such solutions are unstable 
 in the direction of the singularity. For this reason\, it is of interest t
 o study the anisotropic setting. \n\nThe purpose of the talk is to describ
 e a framework for studying highly anisotropic singularities. In particular
 \, for analysing the asymptotics of solutions to linear systems of wave eq
 uations on the corresponding backgrounds and deducing information concerni
 ng the geometry.\n\nThe talk will begin with an overview of existing resul
 ts. This will serve as a background and motivation for the problem conside
 red\, but also as a justification for the assumptions defining the framewo
 rk we develop. Following this overview\, the talk will conclude with a rou
 gh description of the results.\n
LOCATION:https://researchseminars.org/talk/jomarec/1/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Greg Galloway (University of Miami)
DTSTART:20201105T143000Z
DTEND:20201105T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/2
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/2/">
 Initial data rigidity results</a>\nby Greg Galloway (University of Miami) 
 as part of JoMaReC - Joint Online Mathematical Relativity Colloquium\n\n\n
 Abstract\nWe present several rigidity results for initial data sets motiva
 ted by the positive mass theorem. An important step in our proofs is to es
 tablish conditions that ensure that a marginally outer trapped surface is 
 “weakly outermost”. A rigidity result for Riemannian manifolds with a 
 lower bound on their scalar curvature is included as a special case.  Rele
 vant background on marginally outer trapped surfaces will be discussed. Th
 is talk is based on joint work with Michael Eichmair and Abraão Mendes.\n
LOCATION:https://researchseminars.org/talk/jomarec/2/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Lydia Bieri (University of Michigan\, Ann Arbor)
DTSTART:20201203T143000Z
DTEND:20201203T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/3
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/3/">
 New structures in gravitational radiation</a>\nby Lydia Bieri (University 
 of Michigan\, Ann Arbor) as part of JoMaReC - Joint Online Mathematical Re
 lativity Colloquium\n\n\nAbstract\nGravitational waves are transporting in
 formation from faraway regions of the Universe. A new era began with the f
 irst detection of gravitational waves by Advanced LIGO in September 2015\,
  and since then several events have been recorded by the LIGO/VIRGO collab
 oration. New challenges await us to unravel the interesting interplay betw
 een physics\, astrophysics and mathematics. Most studies so far have been 
 devoted to sources like binary black hole mergers or neutron star mergers\
 , or generally to sources that are stationary outside of a compact set. We
  describe these systems by asymptotically-flat manifolds solving the Einst
 ein equations. These sources have in common that far away their gravitatio
 nal field decays fast enough towards Minkowski spacetime. In particular\, 
 far away from the source\, the decay behavior can be described by a term t
 hat is homogeneous of degree -1 and lower order terms. I will present new 
 results on gravitational radiation for sources that are not stationary out
 side of a compact set\, but whose gravitational fields decay more slowly t
 owards infinity. A panorama of new gravitational effects opens up when del
 ving deeper into these more general spacetimes. In particular\, whereas th
 e former sources produce memory effects that are of purely electric parity
  (permanent displacement only)\, the latter in addition generate memory of
  magnetic type\, thus allowing for rotation in the system. These new effec
 ts emerge naturally from the Einstein equations.\n
LOCATION:https://researchseminars.org/talk/jomarec/3/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Harvey Reall (University of Cambridge)
DTSTART:20210204T143000Z
DTEND:20210204T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/4
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/4/">
 Well-posed formulation of Lovelock and Horndeski theories</a>\nby Harvey R
 eall (University of Cambridge) as part of JoMaReC - Joint Online Mathemati
 cal Relativity Colloquium\n\n\nAbstract\nLovelock theories are the most ge
 neral diffeomorphism invariant theories of gravity in higher dimensions wi
 th second order equations of motion. Horndeski theories are the most gener
 al diffeomorphism invariant theories of gravity coupled to a scalar field 
 in four dimensions with second order equations of motion. In this talk I w
 ill discuss well-posedness of the initial value problem for these theories
 . Previous work has shown that (generalised) harmonic gauge does not give 
 a well-posed initial value problem. I will describe recent work with Aron 
 Kovacs in which we introdued a modification of harmonic gauge that does gi
 ve a well-posed initial value problem provided that the theory remains “
 weakly coupled”. Our modified harmonic gauge may also have applications 
 in conventional GR.\n
LOCATION:https://researchseminars.org/talk/jomarec/4/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Igor Rodnianski (Princeton University)
DTSTART:20210304T143000Z
DTEND:20210304T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/5
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/5/">
 On naked singularities in Einstein equations</a>\nby Igor Rodnianski (Prin
 ceton University) as part of JoMaReC - Joint Online Mathematical Relativit
 y Colloquium\n\n\nAbstract\nI will describe recent and ongoing work with Y
 . Shlapentokh-Rothman on a construction of solutions to the Einstein vacuu
 m equations  corresponding to a naked singularity forming from a regular p
 ast. The talk will focus on a new geometric phenomenon\, corresponding to 
 twisting of null geodesics\, new type of self-similarity\, dynamical appro
 ach to the problem\, and on the comparisons with the naked singularity sol
 utions constructed by Christodoulou for the spherically symmetric Einstein
 -scalar field model.\n
LOCATION:https://researchseminars.org/talk/jomarec/5/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Martín Reiris (Universidad de la República\, Montevideo)
DTSTART:20210401T133000Z
DTEND:20210401T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/6
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/6/">
 New results on compact Cauchy horizons of smooth vacuum spacetimes</a>\nby
  Martín Reiris (Universidad de la República\, Montevideo) as part of JoM
 aReC - Joint Online Mathematical Relativity Colloquium\n\n\nAbstract\nCauc
 hy horizons are rather unique and peculiar objects that have been studied 
 for decades. In this talk I will first review old and new breakthroughs on
  the subject by Isenberg and Moncrief\, and by Petersen and Rácz\, and th
 en discuss joint recent work together with I. Bustamante where it is prove
 d that non-degenerate compact Cauchy horizons on smooth vacuum spacetimes 
 (shortly CHs) have indeed constant non-zero temperature. It then follows b
 y the work of Petersen and Petersen-Rácz that CHs are Killing horizons\, 
 and by the work of  Beig-Chruściel-Schoen that such objects are non-gener
 ic on the initial data (in agreement with the Cosmic Censorship conjecture
 ). A null-orbital and topological classification of CHs will also be comme
 nted.\n
LOCATION:https://researchseminars.org/talk/jomarec/6/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Lan-Hsuan Huang (University of Conneticut)
DTSTART:20210506T133000Z
DTEND:20210506T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/7
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/7/">
 Existence of static vacuum extensions</a>\nby Lan-Hsuan Huang (University 
 of Conneticut) as part of JoMaReC - Joint Online Mathematical Relativity C
 olloquium\n\n\nAbstract\nThe study of static vacuum Riemannian metrics ari
 ses naturally in general relativity and differential geometry. A static va
 cuum metric produces a static spacetime by a warped product\, and it is re
 lated to scalar curvature deformation and gluing. The well-known Uniquenes
 s Theorem of Static Black Holes says that an asymptotically flat\, static 
 vacuum metric with black hole boundary must belong to the Schwarzschild fa
 mily. In contrast to the rigidity phenomenon\, R. Bartnik conjectured that
  there are asymptotically flat\, static vacuum metric realizing certain ar
 bitrarily specified boundary data. I will discuss recent progress toward t
 his conjecture. It is based on joint work with Zhongshan An. \n \nIn the s
 econd part of the talk (if time permits)\, I will discuss related topics i
 n the non-time-symmetric case. In many ways\, a stationary vacuum initial 
 data set is a generalization of a static vacuum metric. However\, from the
  point of view of deforming the dominant energy condition\, we discover th
 at a “ground state” initial data set need not be stationary vacuum but
  can sit in a null dust spacetime with a global Killing vector field\, suc
 h as the pp-waves. This part is based on joint work with Dan Lee.\n
LOCATION:https://researchseminars.org/talk/jomarec/7/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Piotr Chruściel (University of Vienna)
DTSTART:20210603T133000Z
DTEND:20210603T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/8
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/8/">
 The hyperbolic positive energy theorem</a>\nby Piotr Chruściel (Universit
 y of Vienna) as part of JoMaReC - Joint Online Mathematical Relativity Col
 loquium\n\n\nAbstract\nI will review the notion of mass of asymptotically 
 locally hyperbolic manifolds\, and sketch the proof of positivity of the e
 nergy for manifolds with spherical conformal infinity.\n\nTalk based on jo
 int work with Erwann Delay in arXiv: 1901.05263 [math.DG]\n
LOCATION:https://researchseminars.org/talk/jomarec/8/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Georgios Moschidis (University of California\, Berkeley)
DTSTART:20210701T133000Z
DTEND:20210701T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/9
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/9/">
 The instability of Anti-de Sitter spacetime for the Einstein-scalar field 
 system</a>\nby Georgios Moschidis (University of California\, Berkeley) as
  part of JoMaReC - Joint Online Mathematical Relativity Colloquium\n\n\nAb
 stract\nThe AdS instability conjecture provides an example of weak turbule
 nce appearing in the dynamics of the Einstein equations in the presence of
  a negative cosmological constant. The conjecture claims the existence of 
 arbitrarily small perturbations to the initial data of Anti-de Sitter spac
 etime which\, under evolution by the vacuum Einstein equations with reflec
 ting boundary conditions at conformal infinity\, lead to the formation of 
 black holes after sufficiently long time. In this talk\, I will present a 
 rigorous proof of the AdS instability conjecture in the setting of the sph
 erically symmetric Einstein-scalar field system. The construction of the u
 nstable initial data will require carefully designing a family of initial 
 configurations of localized matter beams and estimating the exchange of en
 ergy taking place between interacting beams over long periods of time\, as
  well as estimating the decoherence rate of those beams. I will also discu
 ss possible paths for extending these ideas to the vacuum case.\n
LOCATION:https://researchseminars.org/talk/jomarec/9/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Mihalis Dafermos (Princeton University and University of Cambridge
 )
DTSTART:20211007T133000Z
DTEND:20211007T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/10
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/10/"
 >The black hole stability problem in general relativity</a>\nby Mihalis Da
 fermos (Princeton University and University of Cambridge) as part of JoMaR
 eC - Joint Online Mathematical Relativity Colloquium\n\n\nAbstract\nI will
  review the current status of the black hole stability problem in general 
 relativity and discuss joint work Holzegel\, Rodnianski and Taylor.\n
LOCATION:https://researchseminars.org/talk/jomarec/10/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Jim Isenberg (University of Oregon)
DTSTART:20220602T133000Z
DTEND:20220602T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/11
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/11/"
 >Stability of AVTD behavior for polarized T^2-symmetric space-times</a>\nb
 y Jim Isenberg (University of Oregon) as part of JoMaReC - Joint Online Ma
 thematical Relativity Colloquium\n\n\nAbstract\nOne of the most effective 
 tools for proving that Strong Cosmic Censorship holds for a family of cosm
 ological solutions of Einstein’s equations is to verify that these solut
 ions all exhibit Asymptotically Velocity Term Dominated (AVTD) behavior in
  a neighborhood of their Big Bang singularities. After presenting some bac
 kground history of known results and conjectures concerning the behavior o
 f the gravitational field near the Big Bang in cosmological solutions of E
 instein’s equations\, we discuss recent work with Ellery Ames\, Florian 
 Beyer\, and Todd Oliynyk in which we prove that polarized T^2-Symmetric va
 cuum solutions in a neighborhood of Kasner solutions all exhibit AVTD beha
 vior close to the initial singularity. We also discuss our very recent ext
 ension of these results to the case of non-vanishing cosmological constant
 .\n
LOCATION:https://researchseminars.org/talk/jomarec/11/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Melanie Graf (University of Tübingen)
DTSTART:20211104T143000Z
DTEND:20211104T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/12
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/12/"
 >Singularity theorems in low regularity</a>\nby Melanie Graf (University o
 f Tübingen) as part of JoMaReC - Joint Online Mathematical Relativity Col
 loquium\n\n\nAbstract\nThe singularity theorems of R. Penrose and S. Hawki
 ng from the 1960s show that a spacetime satisfying certain physically reas
 onable curvature and causality conditions cannot be causal geodesically co
 mplete. Despite their great success these classical theorems still have so
 me drawbacks\, one of them being that they require smoothness of the metri
 c while in many physical models the metric is less regular. In my talk I w
 ill present work on singularity theorems based on distributional energy co
 nditions for metrics that are merely continuously differentiable – a reg
 ularity where one still has existence but not uniqueness for solutions of 
 the geodesic equation. We will see that an approximation-based approach to
  the low-regularity issue is closely linked to establishing singularity th
 eorems under weakened energy conditions and while the improvements necessa
 ry are still entirely straightforward in the present case\, attempting to 
 lower the regularity further would require some new methods.\n
LOCATION:https://researchseminars.org/talk/jomarec/12/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Stefan Czimek (Brown University)
DTSTART:20211202T143000Z
DTEND:20211202T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/13
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/13/"
 >The characteristic gluing problem of general relativity</a>\nby Stefan Cz
 imek (Brown University) as part of JoMaReC - Joint Online Mathematical Rel
 ativity Colloquium\n\n\nAbstract\nIn this talk we introduce and solve the 
 characteristic gluing problem for the Einstein vacuum equations. We prove 
 that obstructions to characteristic gluing come from an infinite-dimension
 al space of conservation laws along null hypersurfaces for the linearized 
 equations at Minkowski. We show that this obstruction space splits into an
  infinite-dimensional space of gauge-dependent charges and a 10-dimensiona
 l space of gauge-invariant charges. We identify the 10 gauge-invariant cha
 rges to be related to the energy\, linear momentum\, angular momentum and 
 center-of-mass of the spacetime. Based on this identification\, we explain
  how to characteristically glue a given spacetime to a suitably chosen Ker
 r black hole spacetime. As corollary we get an alternative proof of the Co
 rvino-Schoen spacelike gluing to Kerr. Moreover\, we apply our characteris
 tic gluing method to localise characteristic initial data along null hyper
 surfaces. In particular\, this yields a new proof of the Carlotto-Schoen s
 pacelike localization where our method yields no loss of decay\, thus reso
 lving an open problem in this direction. We also outline further applicati
 ons. This is joint work with S. Aretakis (Toronto) and I. Rodnianski (Prin
 ceton).\n
LOCATION:https://researchseminars.org/talk/jomarec/13/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Eric Ling (Rutgers University)
DTSTART:20220203T143000Z
DTEND:20220203T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/14
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/14/"
 >On the discrete Dirac spectrum of a point electron in the zero-gravity Ke
 rr-Newman spacetime</a>\nby Eric Ling (Rutgers University) as part of JoMa
 ReC - Joint Online Mathematical Relativity Colloquium\n\n\nAbstract\nIn re
 lativistic quantum mechanics\, the point spectrum of the Dirac hamiltonian
  with a Coulomb potential famously agrees with Sommerfeld’s fine structu
 re formula for the hydrogen atom. In the Coulomb approximation\, the proto
 n is assumed to only have a positive electric charge. However\, the physic
 al proton also appears to have a magnetic moment which yields a hyperfine 
 structure of the hydrogen atom that’s normally computed perturbatively. 
 Aiming towards a non-perturbative approach\, Pekeris in 1987 proposed taki
 ng the Kerr-Newman spacetime with its ring singularity as a source for the
  proton’s electric charge and magnetic moment. Given the proton’s mass
  and electric charge\, the resulting Kerr-Newman spacetime lies well withi
 n the naked singularity sector which possess closed timelike loops. In 201
 4 Tahvildar-Zadeh showed that the zero-gravity limit of the Kerr-Newman sp
 acetime (zGKN) produces a flat but topologically nontrivial spacetime that
 ’s no longer plagued by closed timelike loops. In 2015 Tahvildar-Zadeh a
 nd Kiessling studied the hydrogen problem with Dirac’s equation on the z
 GKN spacetime and found that the hamiltonian is essentially self-adjoint a
 nd contains a nonempty discrete spectrum. In this talk\, we show how their
  ideas can be extended to classify the discrete spectrum completely and re
 late it back to the known hydrogenic Dirac spectrum but yielding hyperfine
 -like and Lamb shift-like effects.\n
LOCATION:https://researchseminars.org/talk/jomarec/14/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Christina Sormani (City University of New York)
DTSTART:20220505T133000Z
DTEND:20220505T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/15
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/15/"
 >Towards a Spacetime Intrinsic Flat Convergence</a>\nby Christina Sormani 
 (City University of New York) as part of JoMaReC - Joint Online Mathematic
 al Relativity Colloquium\n\n\nAbstract\nIn order to define a spacetim
 e intrinsic flat convergence\, Carlos Vega and I defined the null
  distance to convert spacetimes endowed with regular cosmological time
 s into metric spaces. Currently Anna Sakovich and I have been explo
 ring the properties of these metric spaces. We can prove that on
 e can recover the causal structure from the null distance and the cosm
 ological time. We can prove that a distance-preserving time-preserving bij
 ection between the spacetimes endowed with a null distance is in fact a Lo
 rentzian isometry under suitable conditions.  Next we will prove there ar
 e biLipschitz charts so that we may view the spacetimes endowed with the n
 ull distance as integral current spaces. This allows us to rigorously def
 ine the spacetime intrinsic flat convergence for spacetimes that a
 rise as the future maximal developments of initial\ndata sets. For 
 more information about intrinsic flat convergence see https://sites.googl
 e.com/site/intrinsicflatconvergence/\n
LOCATION:https://researchseminars.org/talk/jomarec/15/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Robert Wald (University of Chicago)
DTSTART:20220407T133000Z
DTEND:20220407T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/16
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/16/"
 >The memory effect and infrared divergences</a>\nby Robert Wald (Universit
 y of Chicago) as part of JoMaReC - Joint Online Mathematical Relativity Co
 lloquium\n\n\nAbstract\nThe “memory effect” is the permanent relative 
 displacement of test particles after the passage of gravitational radiatio
 n. It is associated with both the propagation of massive bodies out to tim
 elike infinity (“ordinary memory”) or the propagation of radiation out
  to null infinity (“null memory”). The memory effect can be characteri
 zed by the failure of the shear tensor at order 1/r to return to zero at l
 ate times\, even though it is “pure gauge.” Closely analogous effects 
 occur in electromagnetism\, where the vector potential at order 1/r fails 
 to return to zero even though it is “pure gauge.” In both cases\, the 
 Fourier transform of the radiative field has divergent behavior at low fre
 quencies. This gives rise to infrared divergences (i.e.\, infinite numbers
  of “soft” gravitons/photons) in the quantum field theory description 
 if one attempts to describe these states as vectors in the usual Fock Hilb
 ert space representation. To obtain a mathematically sensible quantum scat
 tering theory\, one must allow states with nonvanishing memory in the “i
 n” and “out” Hilbert spaces. An elegant solution to this problem in 
 massive quantum electrodynamics was given by Kulish and Fadeev\, who const
 ructed a Hilbert space of incoming/outgoing charged particle states that a
 re “dressed” with radiative fields of corresponding memory\, so as to 
 yield vanishing large gauge charges at spatial infinity. However\, we show
  that this type of construction fails in quantum gravity. The primary unde
 rlying reason is that the “dressing” contributes to null memory\, ther
 eby invalidating the construction of eigenstates of large gauge charges. I
 n quantum gravity\, there does not appear to be any choice of (separable) 
 Hilbert space of incoming/outgoing states that can accommodate all scatter
 ing states. Thus\, we argue that scattering should be described at the lev
 el of algebraic incoming/outgoing states rather than attempting to artific
 ially restrict states to a particular Hilbert space.\n
LOCATION:https://researchseminars.org/talk/jomarec/16/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Zoe Wyatt (University of Cambrdige)
DTSTART:20220303T143000Z
DTEND:20220303T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/17
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/17/"
 >Global Stability of Spacetimes with Supersymmetric Compactifications</a>\
 nby Zoe Wyatt (University of Cambrdige) as part of JoMaReC - Joint Online 
 Mathematical Relativity Colloquium\n\n\nAbstract\nSpacetimes with compact 
 directions which have special holonomy\, such as Calabi-Yau spaces\, play 
 an important role in supergravity and string theory. In this talk I will d
 iscuss a recent work with Lars Andersson\, Pieter Blue and Shing-Tung Yau\
 , where we show the global\, nonlinear stability a spacetime which is a ca
 rtesian product of a high dimensional Minkowski space with a compact Ricci
  flat internal space with special holonomy. This stability result is relat
 ed to a conjecture of Penrose concerning the validity of string theory. Ou
 r proof uses the intersection of methods for quasilinear wave and Klein-Go
 rdon equations\, and so towards the end of the talk I will also comment mo
 re generally on coupled wave–Klein-Gordon equations.\n
LOCATION:https://researchseminars.org/talk/jomarec/17/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Thomas Körber (University of Vienna)
DTSTART:20220707T133000Z
DTEND:20220707T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/18
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/18/"
 >Uniqueness of large area-constrained Willmore spheres in initial data set
 s</a>\nby Thomas Körber (University of Vienna) as part of JoMaReC - Joint
  Online Mathematical Relativity Colloquium\n\n\nAbstract\nThe Hawking mass
  of an area-constrained Willmore sphere is a useful quasi-local measure fo
 r the strength of the gravitational field of an initial data set for the E
 instein field equations. If the scalar curvature satisfies certain asympto
 tic assumptions\, the asymptotic region of such an initial data set is fol
 iated by large area-constrained Willmore spheres with non-negative Hawking
  mass. It has been conjectured that these are the only such spheres. In th
 is talk\, I will present a proof of this conjecture for all large area-con
 strained Willmore spheres with non-negative Hawking mass and outer radius 
 less than the logarithm of the inner radius. This is joint work with Micha
 el Eichmair\, Jan Metzger\, and Felix Schulze.\n
LOCATION:https://researchseminars.org/talk/jomarec/18/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Badri Krishnan (Radboud University Nijmegen)
DTSTART:20220901T133000Z
DTEND:20220901T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/19
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/19/"
 >A quasi-local view of black hole mergers</a>\nby Badri Krishnan (Radboud 
 University Nijmegen) as part of JoMaReC - Joint Online Mathematical Relati
 vity Colloquium\n\n\nAbstract\nIn this talk I will summarize recent progre
 ss and open mathematical problems in understanding black hole mergers quas
 i-locally\, i.e. by using marginally trapped surfaces instead of event hor
 izons.\n
LOCATION:https://researchseminars.org/talk/jomarec/19/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Marcus Khuri (Stony Brook University)
DTSTART:20221006T133000Z
DTEND:20221006T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/20
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/20/"
 >Level Set Methods in Mathematical GR</a>\nby Marcus Khuri (Stony Brook Un
 iversity) as part of JoMaReC - Joint Online Mathematical Relativity Colloq
 uium\n\n\nAbstract\nWe will review recent developments concerning the use 
 of level set techniques associated with solutions to elliptic equations\, 
 in particular spacetime harmonic functions\, and their application to posi
 tive mass theorems and comparison geometry.\n
LOCATION:https://researchseminars.org/talk/jomarec/20/
END:VEVENT
BEGIN:VEVENT
SUMMARY:José Natário (Instituto Superior Técnico)
DTSTART:20221103T143000Z
DTEND:20221103T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/21
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/21/"
 >Relativistic elasticity and compactness bounds</a>\nby José Natário (In
 stituto Superior Técnico) as part of JoMaReC - Joint Online Mathematical 
 Relativity Colloquium\n\n\nAbstract\nAfter reviewing the basics of relativ
 istic elasticity theory\, I will introduce a general framework to study sp
 herically symmetric self-gravitating elastic bodies systematically within 
 general relativity\, and apply it to investigate compactness bounds in thi
 s context.\n
LOCATION:https://researchseminars.org/talk/jomarec/21/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Elena Giorgi (Columbia University)
DTSTART:20221201T143000Z
DTEND:20221201T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/22
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/22/"
 >Physical-space estimates on black hole perturbations</a>\nby Elena Giorgi
  (Columbia University) as part of JoMaReC - Joint Online Mathematical Rela
 tivity Colloquium\n\n\nAbstract\nMost works on the analysis of the wave eq
 uation on Kerr black holes rely on a combination of the vector field metho
 d and Fourier decomposition\, with the notable exception of a generalized 
 vector field method introduced by Andersson-Blue. Their method allows for 
 commutation with second order differential operators entirely in physical-
 space by supplementing the Killing vector fields with the Carter operator 
 of Kerr to obtain a local energy decay identity at the level of three deri
 vatives of the solution for sufficiently small |a|. I this talk I will des
 cribe the main ideas of Andersson-Blue's method and explain its advantages
  in two recent applications where physical space-estimates have been cruci
 al: the linear stability of Kerr-Newman black hole to coupled gravitationa
 l-electromagnetic perturbations and our proof of the non-linear stability 
 of the slowly rotating Kerr family with Klainerman-Szeftel.\n
LOCATION:https://researchseminars.org/talk/jomarec/22/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Jérémie Szeftel (Sorbonne Université)
DTSTART:20230202T143000Z
DTEND:20230202T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/23
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/23/"
 >The nonlinear stability of Kerr for small angular momentum</a>\nby Jéré
 mie Szeftel (Sorbonne Université) as part of JoMaReC - Joint Online Mathe
 matical Relativity Colloquium\n\n\nAbstract\nI will introduce the celebrat
 ed black hole stability conjecture according to which the Kerr family of m
 etrics are stable as solutions to the Einstein vacuum equations of general
  relativity. I will then discuss the history of this problem\, including a
  recent work on the resolution of the black hole stability conjecture for 
 small angular momentum.\n
LOCATION:https://researchseminars.org/talk/jomarec/23/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Robert J. McCann (University of Toronto)
DTSTART:20230302T143000Z
DTEND:20230302T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/24
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/24/"
 >A nonsmooth approach to Einstein's theory of gravity</a>\nby Robert J. Mc
 Cann (University of Toronto) as part of JoMaReC - Joint Online Mathematica
 l Relativity Colloquium\n\n\nAbstract\nWhile Einstein's theory of gravity 
 is formulated in a smooth setting\, the celebrated singularity theorems of
  Hawking and Penrose describe many physical situations in which this smoot
 hness must eventually breakdown. In positive-definite signature\, there is
  a highly successful theory of metric and metric-measure geometry which in
 cludes Riemannian manifolds as a special case\,  but permits the extractio
 n of nonsmooth limits under dimension and curvature bounds analogous to th
 e energy conditions in relativity: here sectional curvature is reformulate
 d through triangle comparison\,  while Ricci curvature is reformulated usi
 ng entropic convexity along geodesics of probability measures. This lectur
 e explores recent progress in the development of an analogous theory in Lo
 rentzian signature\, whose ultimate goal is to provide a nonsmooth theory 
 of gravity.\n
LOCATION:https://researchseminars.org/talk/jomarec/24/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Oliver Lindblad Petersen (KTH Stockholm)
DTSTART:20230406T133000Z
DTEND:20230406T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/25
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/25/"
 >Wave equations in subextremal Kerr-de Sitter spacetimes</a>\nby Oliver Li
 ndblad Petersen (KTH Stockholm) as part of JoMaReC - Joint Online Mathemat
 ical Relativity Colloquium\n\n\nAbstract\nIn 2013\, Vasy proved that solut
 ions to linear wave equations in Kerr-de Sitter spacetimes have asymptotic
  expansions in quasinormal modes up to an exponentially decaying term\, as
 suming the angular momentum of the black hole satisfies certain bounds. Th
 is was the first step towards the proof of non-linear stability for slowly
  rotating Kerr-de Sitter black holes by Hintz and Vasy in 2018. In this ta
 lk\, we extend Vasy's result to the full subextremal range of Kerr-de Sitt
 er spacetimes\, by removing the restrictions on the angular momentum of th
 e black hole. The proof is based on a new Fredholm setup and a new analysi
 s of the trapping of photons around a Kerr-de Sitter black hole. This is j
 oint work with Andras Vasy.\n
LOCATION:https://researchseminars.org/talk/jomarec/25/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Ettore Minguzzi (University of Florence)
DTSTART:20230504T133000Z
DTEND:20230504T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/26
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/26/"
 >Abstract Lorentzian metric spaces and their Gromov-Hausdorff convergence<
 /a>\nby Ettore Minguzzi (University of Florence) as part of JoMaReC - Join
 t Online Mathematical Relativity Colloquium\n\n\nAbstract\nA definition fo
 r `bounded Lorentzian metric space' is presented and discussed. This is an
  abstract notion of Lorentzian metric space that is sufficiently general t
 o comprise compact causally convex subsets of globally hyperbolic (smooth)
  spacetimes\, and causets.\nIt is shown that a generalization of the Gromo
 v-Hausdorff distance and convergence can be applied to these spaces. Furth
 ermore\, two additional axioms of timelike connectedness and existence of 
 maximizers\, which are stable under GH-convergence\, lead to suitable noti
 ons of Lorentzian pre-length and length spaces. Similarly\, sectional curv
 ature bounds stable under GH-convergence can be introduced. A (pre)compact
 ness theorem is also mentioned and its limitations are discussed. Talk bas
 ed on joint work with Stefan Suhr (Bochum).\n
LOCATION:https://researchseminars.org/talk/jomarec/26/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Virginia Agostiniani (University of Trento)
DTSTART:20230601T133000Z
DTEND:20230601T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/27
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/27/"
 >A Green’s function proof of the positive mass theorem and related topic
 s</a>\nby Virginia Agostiniani (University of Trento) as part of JoMaReC -
  Joint Online Mathematical Relativity Colloquium\n\n\nAbstract\nIn this ta
 lk\, we will explore the role of harmonic and p-harmonic functions in esta
 blishing fundamental geometric inequalities in mathematical relativity\, s
 uch as the positive mass theorem and the Penrose inequality. We will intro
 duce new monotonicity formulas along the level flow of these functions\, w
 hich provide simple proofs for these inequalities. Additionally\, we will 
 discuss how these formulas can be used to characterize the nonnegativity o
 f the scalar curvature\, suggesting a synthetic notion of this concept app
 licable in non-smooth contexts.\n
LOCATION:https://researchseminars.org/talk/jomarec/27/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Cécile Huneau (École Polytechnique)
DTSTART:20230706T133000Z
DTEND:20230706T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/28
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/28/"
 >High frequency solutions in general relativity and the Burnett’s conjec
 ture</a>\nby Cécile Huneau (École Polytechnique) as part of JoMaReC - Jo
 int Online Mathematical Relativity Colloquium\n\n\nAbstract\nIn this talk\
 , I will review some works in collaboration with Jonathan Luk on the behav
 iour of high frequency solutions to the Einstein equations. In the eightie
 s\, the physicist Burnett conjectured that the adherence of the solutions 
 to the Einstein equations\, converging strongly at the level of the metric
 \, and with boudedness assumptions at the level of derivative of the metri
 c\, are the solutions to the Einstein-massless Vlasov equations. I will fo
 cus on the resolution of this conjecture with the additionnal assumption o
 f a translation symmetry\, and explain how to approximate a solution to th
 e Einstein-Vlasov equations by vacuum solutions.\n
LOCATION:https://researchseminars.org/talk/jomarec/28/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Gerhard Huisken (University of Tübingen)
DTSTART:20231102T143000Z
DTEND:20231102T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/29
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/29/"
 >Some observations on quasi-local mass and quasi-local radius</a>\nby Gerh
 ard Huisken (University of Tübingen) as part of JoMaReC - Joint Online Ma
 thematical Relativity Colloquium\n\n\nAbstract\nThe lecture examines older
  and newer concepts of quasi-local mass for one domain relative to another
 \nas well as concepts of quasi-local radius in relation to the hoop-conjec
 ture.\n
LOCATION:https://researchseminars.org/talk/jomarec/29/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Rick Schoen (University of California\, Irvine)
DTSTART:20231207T143000Z
DTEND:20231207T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/30
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/30/"
 >How minimal hypersurface and MOTS singularities affect relativity theorem
 s</a>\nby Rick Schoen (University of California\, Irvine) as part of JoMaR
 eC - Joint Online Mathematical Relativity Colloquium\n\n\nAbstract\nSome t
 heorems in relativity work directly only in low dimensions because of the 
 possibility of singularities in area minimizing hypersurfaces and MOTS. Th
 ese include both Riemannian and spacetime positive mass theorems as well a
 s the Riemannian Penrose inequality. In some cases the singularities are r
 elatively easy to work around and in others they present significant probl
 ems to overcome. This will be a general lecture which will attempt to give
  perspective and more clarity to this issue.\n
LOCATION:https://researchseminars.org/talk/jomarec/30/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Spyros Alexakis (University of Toronto)
DTSTART:20240201T143000Z
DTEND:20240201T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/31
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/31/"
 >Squeezing a fixed amount of gravitational energy to arbitrarily small sca
 les\, in U(1) symmetry</a>\nby Spyros Alexakis (University of Toronto) as 
 part of JoMaReC - Joint Online Mathematical Relativity Colloquium\n\n\nAbs
 tract\nWe discuss a construction of polarized U(1) space-times of a “fix
 ed size”\, where the initial data contains a given amount η>0 of incomi
 ng gravitational energy which is allowed to be supported at arbitrarily sm
 all scales\, without affecting the time of existence. More specialized exa
 mples can be constructed where any chosen fraction of this initial incomin
 g energy can stay focused along a null geodesic\, in the U(1) picture. We 
 discuss the relationship of this result with one direction of Thorne’s h
 oop conjecture. The work relies on a special structure of the Einstein equ
 ations in this symmetry class\, a new re-scaling of the equations and larg
 e-time control\, along with a new local Klainerman-Sobolev estimate. Time 
 permitting\, some comparisons of the result and the methods with large-dat
 a constructions for the Einstein equations over the last decade will also 
 be presented.\n
LOCATION:https://researchseminars.org/talk/jomarec/31/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Rita Teixeira da Costa (Princeton University\, University of Cambr
 idge)
DTSTART:20240307T143000Z
DTEND:20240307T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/32
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/32/"
 >The Teukolsky equation on Kerr in the full subextremal range</a>\nby Rita
  Teixeira da Costa (Princeton University\, University of Cambridge) as par
 t of JoMaReC - Joint Online Mathematical Relativity Colloquium\n\n\nAbstra
 ct\nThe Teukolsky equation is one of the fundamental equations governing l
 inear gravitational perturbations of the Kerr black hole family as solutio
 ns to the vacuum Einstein equations. I will discuss joint work with Yakov 
 Shlapentokh-Rothman (Toronto)\, where we show that solutions arising from 
 suitably regular initial data decay inverse polynomially in time. Our proo
 f holds for the entire subextremal range of Kerr black hole parameters (|a
 | < M).\n
LOCATION:https://researchseminars.org/talk/jomarec/32/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Dan Lee (City University of New York)
DTSTART:20240404T133000Z
DTEND:20240404T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/33
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/33/"
 >The equality case of the positive mass theorem</a>\nby Dan Lee (City Univ
 ersity of New York) as part of JoMaReC - Joint Online Mathematical Relativ
 ity Colloquium\n\n\nAbstract\nWe will review the equality case of the posi
 tive mass theorem for initial data sets and discuss its proof in the gener
 al (not necessarily spin) setting. This is joint work with Lan-Hsuan Huang
 .\n
LOCATION:https://researchseminars.org/talk/jomarec/33/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Christoph Kehle (ETH Zürich)
DTSTART:20240502T133000Z
DTEND:20240502T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/34
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/34/"
 >Retiring the third law of black hole thermodynamics</a>\nby Christoph Keh
 le (ETH Zürich) as part of JoMaReC - Joint Online Mathematical Relativity
  Colloquium\n\n\nAbstract\nExtremal black holes are special types of black
  holes which have exactly zero temperature. I will present a proof that ex
 tremal black holes form in finite time in gravitational collapse of charge
 d matter. In particular\, this construction provides a definitive disproof
  of the "third law" of black hole thermodynamics. We also show that extrem
 al black holes take on a central role in gravitational collapse\, giving r
 ise to a new conjectural picture of "extremal critical collapse." This is 
 joint work with Ryan Unger (Princeton).\n
LOCATION:https://researchseminars.org/talk/jomarec/34/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Juan Valiente Kroon (Queen Mary University of London)
DTSTART:20240606T133000Z
DTEND:20240606T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/35
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/35/"
 >BMS-supertranslation charges at the critical sets of null infinity</a>\nb
 y Juan Valiente Kroon (Queen Mary University of London) as part of JoMaReC
  - Joint Online Mathematical Relativity Colloquium\n\n\nAbstract\nFor asym
 ptotically flat spacetimes\, a conjecture by Strominger states that asympt
 otic BMS-supertranslations and their associated charges at past null infin
 ity can be related to those at future null infinity via an antipodal map a
 t spatial infinity. We analyse the validity of this conjecture using Fried
 rich's formulation of spatial infinity\, which gives rise to a regular ini
 tial value problem for the conformal field equations at spatial infinity. 
  We show that for a generic class of asymptotically Euclidean and regular 
 initial data\, BMS-supertranslation charges are not well-defined at the cr
 itical sets where null infinity meets spatial infinity unless the initial 
 data satisfies an extra regularity condition. We also show that given init
 ial data that satisfy the regularity condition\, BMS-supertranslation char
 ges at the critical sets are fully determined by the initial data and that
  the relation between the charges at past null infinity and those at futur
 e null infinity directly follows from our regularity condition. This is jo
 int work with Mariem Magdy Ali Mohamed and Kartik Prabhu.\n
LOCATION:https://researchseminars.org/talk/jomarec/35/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Carsten Gundlach (University of Southampton)
DTSTART:20241003T140000Z
DTEND:20241003T150000Z
DTSTAMP:20260422T225927Z
UID:jomarec/36
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/36/"
 >The interplay of mathematics and numerics in understanding naked singular
 ity formation in critical collapse</a>\nby Carsten Gundlach (University of
  Southampton) as part of JoMaReC - Joint Online Mathematical Relativity Co
 lloquium\n\n\nAbstract\nI will give an overview of numerical evidence that
  codimension one-sets of smooth initial data for matter coupled to GR form
  naked singularities - from scalar fields and fluids in spherical symmetry
 \, where the evidence is strong\, to vacuum GR\, where the evidence is sti
 ll confusing\, but at least now beginning to be agreed by independent code
 s. Can one hope to prove some form of this naked singularity conjecture? I
 n the last ten years or so\, there has been considerable mathematical prog
 ress on the existence and stability of smooth self-similar blowup solution
 s in dispersive PDEs\, and on naked singularity formation in GR. I will hi
 ghlight some of these papers that particularly interest me as steps on the
  way to a future proof of naked singularity formation from codimension-one
  smooth initial data.\n
LOCATION:https://researchseminars.org/talk/jomarec/36/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Zhongshan An (University of Michigan\, Ann Arbor)
DTSTART:20241107T143000Z
DTEND:20241107T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/37
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/37/"
 >Einstein manifolds with boundary</a>\nby Zhongshan An (University of Mich
 igan\, Ann Arbor) as part of JoMaReC - Joint Online Mathematical Relativit
 y Colloquium\n\n\nAbstract\nWe will talk about existence of Einstein metri
 cs on manifolds with boundary\, while prescribing the induced conformal me
 tric and mean curvature of the boundary. In dimension 3\, this becomes the
  existence of conformal embeddings of surfaces into constant sectional cur
 vature space forms\, with prescribed mean curvature. We will show existenc
 e of such conformal emebeddings near generic Einstein background. We will 
 also discuss the existence question in higher dimensions\, where things be
 come more subtle and a non-degenerate boundary condition is used to constr
 uct metrics with nonpositive Einstein constant.\n
LOCATION:https://researchseminars.org/talk/jomarec/37/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Peter Hintz (ETH Zurich)
DTSTART:20241205T143000Z
DTEND:20241205T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/38
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/38/"
 >Gluing small black holes along timelike geodesics</a>\nby Peter Hintz (ET
 H Zurich) as part of JoMaReC - Joint Online Mathematical Relativity Colloq
 uium\n\n\nAbstract\nSuppose we are given a globally hyperbolic spacetime $
 (M\,g)$ solving the Einstein vacuum equations\, and a timelike geodesic in
  M. I will explain how to construct\, on any compact subset of M\, a solut
 ion geps of the Einstein vacuum equations which is approximately equal to 
 g far from the geodesic but near any point along the geodesic approximatel
 y equal to the metric of a Kerr black hole with masseps. As an application
 \, we can construct spacetimes which describe the merger of a very light b
 lack hole with a unit mass black hole\, followed by the relaxation of the 
 resulting single black hole to its equilibrium (Kerr or Kerr-de Sitter) st
 ate.\n
LOCATION:https://researchseminars.org/talk/jomarec/38/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Simon Brendle (Columbia University)
DTSTART:20250306T143000Z
DTEND:20250306T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/39
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/39/"
 >Systolic inequalities and the Horowitz-Myers conjecture</a>\nby Simon Bre
 ndle (Columbia University) as part of JoMaReC - Joint Online Mathematical 
 Relativity Colloquium\n\n\nAbstract\nI will discuss joint work with Pei-Ke
 n Hung on the\nHorowitz-Myers conjecture in dimension at most 7. Our appro
 ach relies\non a new geometric inequality. For a Riemannian metric on $B^2
  \\times\nT^{n-2}$ with scalar curvature at least $-n(n-1)$\, this inequal
 ity\nrelates the systole of the boundary to the mean curvature of the\nbou
 ndary.\n
LOCATION:https://researchseminars.org/talk/jomarec/39/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Stefan Suhr (Ruhr-University Bochum)
DTSTART:20250206T143000Z
DTEND:20250206T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/40
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/40/"
 >Optimal Transport in Lorentzian Geometry</a>\nby Stefan Suhr (Ruhr-Univer
 sity Bochum) as part of JoMaReC - Joint Online Mathematical Relativity Col
 loquium\n\n\nAbstract\nIn recent years the theory of optimal transportatio
 n has made an impact on Lorentzian geometry\, mainly through synthetic def
 initions of timelike Ricci curvature bounds for Lorentzian manifolds and L
 orentzian length spaces. But there are also other aspects of Lorentzian op
 timal transport relevant to general relativity. I will give an overview of
  the basic ideas of Lorentzian optimal transport and recent results. Furth
 er I will indicate some open problems in this context.\n
LOCATION:https://researchseminars.org/talk/jomarec/40/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Sergiu Klainerman (Princeton University)
DTSTART:20250403T133000Z
DTEND:20250403T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/41
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/41/"
 >On the legacy of Y. Choquet-Bruhat (1923-2025)</a>\nby Sergiu Klainerman 
 (Princeton University) as part of JoMaReC - Joint Online Mathematical Rela
 tivity Colloquium\n\nAbstract: TBA\n
LOCATION:https://researchseminars.org/talk/jomarec/41/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Marc Mars (University of Salamanca)
DTSTART:20250508T134000Z
DTEND:20250508T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/42
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/42/"
 >Null geometry and applications to existence of spacetimes</a>\nby Marc Ma
 rs (University of Salamanca) as part of JoMaReC - Joint Online Mathematica
 l Relativity Colloquium\n\n\nAbstract\nNon-null hypersurfaces can be easil
 y viewed as geometric objects detached from the spacetime where they are e
 mbedded. This process of "detachment" is more complicated in the case of n
 ull hypersurfaces. In this talk I will introduce the notion of "null manif
 old"\, together with related concepts such as "ruled null manifold" or "me
 tric hypersurface data"\, as a way to study null hypersurfaces from a full
 y detached point of view. With this framework at hand\, I will then discus
 s three applications related to existence of spacetimes. Specifically\, I 
 will present a detached version of the characteristic initial value proble
 m\, a general analysis of transverse expansions across a null hypersurface
  and an existence and asymptotic uniqueness result of $\\Lambda$-vacuum sp
 acetimes from data on a (detached) non-degenerate Killing horizon. The thr
 ee applications are joint work with Gabriel Sánchez Pérez.\n\nwill be st
 reamed from the GAPs conference at IMAG https://www.birs.ca/events/2025/5-
 day-workshops/25w5397\n
LOCATION:https://researchseminars.org/talk/jomarec/42/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Warren Li (Stanford University)
DTSTART:20251002T133000Z
DTEND:20251002T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/44
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/44/"
 >Progress towards the BKL Proposal</a>\nby Warren Li (Stanford University)
  as part of JoMaReC - Joint Online Mathematical Relativity Colloquium\n\n\
 nAbstract\nAround 50 years ago\, physicists Belinski\, Khalatnikov and Lif
 shitz provided heuristics describing the behaviour of near-singularity sol
 utions to the Einstein equations as spacelike\, local and oscillatory. Vag
 uely speaking\, they suggest that dynamics corresponding to different spat
 ial points on the singularity decouple and resemble a chaotic cascade of s
 o-called “Kasner epochs”. In this talk\, we present a mathematical for
 mulation of this “BKL Conjecture” and progress towards the conjecture 
 in the case of Gowdy symmetric spacetimes.\n
LOCATION:https://researchseminars.org/talk/jomarec/44/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Raphaela Wutte (Arizona State University)
DTSTART:20250605T133000Z
DTEND:20250605T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/45
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/45/"
 >Hyperbolic Mass in 2+1 Dimensions</a>\nby Raphaela Wutte (Arizona State U
 niversity) as part of JoMaReC - Joint Online Mathematical Relativity Collo
 quium\n\n\nAbstract\nSolutions to general relativity with a negative cosmo
 logical constant have received significant attention due to the conjecture
 d AdS/CFT correspondence\, a particularly well-understood example of which
  is exhibited in 2+1 dimensions.\n\nI will review known vacuum solutions t
 o general relativity with a negative cosmological constant in 2+1 dimensio
 ns and discuss the difficulties in defining mass\, which are resolved via 
 minimisation using a positive energy theorem. I will present a gluing theo
 rem for vacuum time-symmetric general-relativistic initial data sets in tw
 o spatial dimensions. By gluing two given time-symmetric vacuum initial da
 ta sets at conformal infinity\, we obtain new time-symmetric vacuum initia
 l data sets. I will sketch the derivation of the mass formulae of the resu
 lting manifolds. Our gluing theorem yields complete manifolds with any mas
 s aspect function\, which are smooth except for one conical singularity.\n
 \nBased on joint work with P. T. Chruściel.\n
LOCATION:https://researchseminars.org/talk/jomarec/45/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Jacques Smulevici (Sorbonne Université)
DTSTART:20251106T143000Z
DTEND:20251106T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/46
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/46/"
 >Non-linear waves and time-periodicity</a>\nby Jacques Smulevici (Sorbonne
  Université) as part of JoMaReC - Joint Online Mathematical Relativity Co
 lloquium\n\n\nAbstract\nI will give an overview talk concerning the possib
 le existence and stability of solutions to non-linear wave equations which
  are periodic in time. Such solutions can arise in a variety of mathematic
 al models\, from fluid dynamics\, elasticity\, and general relativity\, wh
 ere in particular\, there were investigated numerically by Maliborski and 
 Rostworowski (2013) for the Einstein-scalar-field model in spherically sym
 metry near the Anti-de-Sitter spacetime. \n\nI will start the presentation
  with some reminder concerning the linear wave equation on Anti-de-Sitter 
 before presenting some results and methods for semi-linear wave equations.
  In a second part\, I will describe a recent construction of special coord
 inates for 1+1 Lorentzian metric on \\mathbb{R}\\times\\mathcal{S}^1 with 
 time-periodic coefficients\, which is expected to be an essential step to 
 extend the previous results to quasi linear wave equations.\n\nThis a join
 t work with Athanasios Chatzikaleas (National and Kapodistrian University 
 of Athens ).\n
LOCATION:https://researchseminars.org/talk/jomarec/46/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Annachiara Piubello (University of Copenhagen)
DTSTART:20251204T143000Z
DTEND:20251204T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/47
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/47/"
 >A geometric choice of asymptotically Euclidean coordinates via STCMC-foli
 ations</a>\nby Annachiara Piubello (University of Copenhagen) as part of J
 oMaReC - Joint Online Mathematical Relativity Colloquium\n\n\nAbstract\nAs
 ymptotically Euclidean initial data sets (IDS) in General Relativity model
  instants in time for isolated systems. In this talk\, we show that an IDS
  is asymptotically Euclidean if it admits a cover by closed hypersurfaces 
 of constant spacetime mean curvature (STCMC)\, provided these hypersurface
 s satisfy certain geometric estimates\, some weak foliation properties\, a
 nd each surface exhibits generalized stability. Building on the work of Ce
 derbaum and Sakovich (2021)\, which established that every asymptotically 
 Euclidean IDS has a unique STCMC foliation\, we conclude that the existenc
 e of such a foliation characterizes asymptotically Euclidean IDS. Furtherm
 ore\, we explore the connections to the center of mass and show why these 
 coordinates seem well-adapted to describe this concept. This is joint work
  with O. Vičánek Martínez.\n
LOCATION:https://researchseminars.org/talk/jomarec/47/
END:VEVENT
BEGIN:VEVENT
SUMMARY:David Maxwell (University of Alaska\, Fairbanks)
DTSTART:20260205T143000Z
DTEND:20260205T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/48
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/48/"
 >Einstein-fluid initial data</a>\nby David Maxwell (University of Alaska\,
  Fairbanks) as part of JoMaReC - Joint Online Mathematical Relativity Coll
 oquium\n\n\nAbstract\nFluids are a standard matter source for gravitation\
 , going back to the early days of general relativity. Nevertheless\, const
 ructing initial data for this family of matter models is surprisingly nuan
 ced. In this talk we describe a novel approach to building Einstein-fluid 
 initial data based on a recently established phase-space technique for con
 structing non-vacuum initial data sets. Compared to prior approaches to wo
 rking with fluids\, the input parameters allow for more direct specificati
 on of physical quantities\, such as the number of particles in any given r
 egion. We focus on perfect fluids but also touch on extensions of these id
 eas\nto viscous models.\n
LOCATION:https://researchseminars.org/talk/jomarec/48/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Gilbert Weinstein (Ariel University\, Israel)
DTSTART:20260305T143000Z
DTEND:20260305T153000Z
DTSTAMP:20260422T225927Z
UID:jomarec/49
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/49/"
 >The mass angular momentum inequality</a>\nby Gilbert Weinstein (Ariel Uni
 versity\, Israel) as part of JoMaReC - Joint Online Mathematical Relativit
 y Colloquium\n\n\nAbstract\nIn this talk\,I will discuss our recent result
 . Either there is a counterexample to black hole uniqueness\, or the follo
 wing statement holds. Axisymmetric\, complete\, simply connected\, maximal
  initial data sets for the Einstein equations of nonnegative energy densit
 y with ends that are either asymptotically flat or asymptotically cylindri
 cal\, admit an ADM mass lower bound given by the square root of total angu
 lar momentum. Moreover\, equality is achieved only for a constant time sli
 ce of an extreme Kerr spacetime. The proof is based on a novel flow of sin
 gular harmonic maps with hyperbolic plane target\, under which the renorma
 lized harmonic energy is monotonically nonincreasing. Relevant properties 
 of the flow are achieved through a refined asymptotic analysis of solution
 s to the linearized harmonic map equations.\n\nThis is joint work with Qin
 g Han\, Marcus Khuri\, and Jingang Xiong.\n
LOCATION:https://researchseminars.org/talk/jomarec/49/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Mariem Magdy (Perimeter Institute and Fields Institute\, Canada)
DTSTART:20260402T133000Z
DTEND:20260402T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/50
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/50/"
 >Estimates for spinor fields using the space-spinor formalism</a>\nby Mari
 em Magdy (Perimeter Institute and Fields Institute\, Canada) as part of Jo
 MaReC - Joint Online Mathematical Relativity Colloquium\n\n\nAbstract\nI w
 ill discuss recent work on estimates for spinor fields obeying first-order
  equations\, formulated within the space–spinor framework. The approach 
 is motivated by the positive commutator method presented in the work of P.
  Hintz and A. Vasy\, originally designed for tensor fields satisfying seco
 nd-order equations. In this talk\, I will outline how these ideas can be a
 dapted to the spinorial setting and how the resulting estimates fit natura
 lly into the first-order structure of the equations.\n
LOCATION:https://researchseminars.org/talk/jomarec/50/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Roya Mohayaee (Sorbonne University\, France)
DTSTART:20260507T133000Z
DTEND:20260507T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/51
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/51/"
 >Optimal Transport theory and its applications in cosmology</a>\nby Roya M
 ohayaee (Sorbonne University\, France) as part of JoMaReC - Joint Online M
 athematical Relativity Colloquium\n\n\nAbstract\nI will begin with a conci
 se review of the fundamental ideas underlying optimal transport theory\, b
 efore illustrating how these concepts naturally emerge in cosmological con
 texts and provide a powerful framework for addressing the problem of cosmo
 logical reconstruction. I will then highlight how optimal transport extend
 s beyond its analytical utility in handling big data\, and demonstrate int
 riguing connections with certain theories of modified gravity.\n
LOCATION:https://researchseminars.org/talk/jomarec/51/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Miguel Sánchez (University of Granada\, Spain)
DTSTART:20260604T133000Z
DTEND:20260604T143000Z
DTSTAMP:20260422T225927Z
UID:jomarec/52
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/jomarec/52/"
 >Globally hyperbolic spacetimes-with-timelike-boundary: global splitting\,
  asymptotically AdS spacetimes and null-convexity</a>\nby Miguel Sánchez 
 (University of Granada\, Spain) as part of JoMaReC - Joint Online Mathemat
 ical Relativity Colloquium\n\n\nAbstract\nGlobally hyperbolic spacetimes w
 ith a timelike boundary model spacetimes with naked singularities distribu
 ted on a timelike hypersurface\, potentially admitting conditions on both 
 the boundary and a Cauchy hypersurface. Typically\, the boundary can serve
  as: (1) a cut-off for the system under consideration\, or (2) a conformal
  completion of the spacetime\, as in the case of asymptotically Anti-de Si
 tter spacetimes.\n\nFirst\, we will review some of their general propertie
 s\, including those related to causality\, the existence of global orthogo
 nal splittings\, and the relationship between the properties of the bounda
 ry and the interior of the spacetime. Then\, we will focus on the null-con
 vexity of the boundary. This is a natural assumption satisfied by asymptot
 ically AdS spacetimes\, which implies that the interior of the spacetime r
 etains most of the geometric properties of the boundaryless case\, such as
  being causally simple with a Hausdorff space of lightlike geodesics.\n\nB
 ased in joint work with L. Aké and JL. Flores (arxiv: 1808.04412) and wit
 h J. Herrera (arxiv: 2506.09032).\n
LOCATION:https://researchseminars.org/talk/jomarec/52/
END:VEVENT
END:VCALENDAR
