BEGIN:VCALENDAR
VERSION:2.0
PRODID:researchseminars.org
CALSCALE:GREGORIAN
X-WR-CALNAME:researchseminars.org
BEGIN:VEVENT
SUMMARY:Andreas Mantziris (Imperial College)
DTSTART:20210408T140000Z
DTEND:20210408T150000Z
DTSTAMP:20260423T003256Z
UID:IFTWeb/43
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/IFTWeb/43/">
 Cosmological implications of electroweak vacuum instability: constraints o
 n the Higgs curvature coupling from inflation</a>\nby Andreas Mantziris (I
 mperial College) as part of IFT-Madrid Webinars\n\n\nAbstract\nThe current
  experimentally measured parameters of the Standard Model (SM) suggest tha
 t our universe lies in a metastable electroweak vacuum\, where the Higgs f
 ield could decay to a lower vacuum state with catastrophic consequences. O
 ur measurements dictate that such an event has not happened yet\, despite 
 the many different mechanisms that could have triggered it during our past
  light-cone. Via this observation\, we can establish a promising link betw
 een cosmology and particle physics and thus constrain important parameters
  of our theories. The focus of our work has been to explore this possibili
 ty by calculating the probability of the false vacuum to decay during the 
 period of inflation and using it to constrain the last unknown renormalisa
 ble SM parameter $\\xi$\, which couples the Higgs field with space-time cu
 rvature. In our latest study\, we derived lower bounds for the Higgs-curva
 ture coupling from vacuum stability in three inflationary models: quadrati
 c and quartic chaotic inflation\, and Starobinsky-like power-law inflation
 . In contrast to most previous studies we took the time-dependence of the 
 Hubble rate into account both in the geometry of our past light-cone and i
 n the Higgs effective potential\, which is approximated with three-loop re
 normalisation group improvement supplemented with one-loop curvature corre
 ctions. We find that in all three models\, the lower bound is $\\xi \\gtrs
 im 0.051 ... 0.066$ depending on the top quark mass. We also demonstrated 
 that vacuum decay is most likely to happen a few e-foldings before the end
  of inflation.\n
LOCATION:https://researchseminars.org/talk/IFTWeb/43/
END:VEVENT
END:VCALENDAR
