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SUMMARY:The Standard Model Higgs and the nature of gravity
DTSTART:20230327T161500Z
DTEND:20230327T180000Z
DTSTAMP:20260928T112524Z
UID:0bed0237-801c-4329-a0a2-b342b96c9699
SEQUENCE:2
CREATED:20230327T144431Z
DESCRIPTION:Abstract:The properties of the Higgs boson together with the a
 bsence of new physics at the Large Hadron Collider allow us to speculate a
 bout consistently extending the Standard Model all the way up to the Planc
 k scale while staying in the perturbative regime. In this context\, the SM
  Higgs non-minimally coupled to gravity could be responsible for the symme
 try properties of the Universe at large scales and the generation of the p
 rimordial spectrum of temperature fluctuations seen in the Cosmic Microwav
 e Background (CMB).In this work we show how Higgs-Inflation and its scale-
 invariant extension\, known as Higgs-Dilaton inflation\, can be embedded i
 n Einstein-Cartan gravity.In particular we will discuss some phenomenologi
 cal features emerging from the inflationary and post-inflationary dynamics
 .
LAST-MODIFIED:20230327T144449Z
LOCATION:Sala de Formação Avançada do DF (Sala 2-8.11 - 2º Piso do Pav
 ilhão de Física)
URL:http://df.vps.tecnico.ulisboa.pt/pt/eventos/the-standard-model-higgs-a
 nd-the-nature-of-gravity/
X-ALT-DESC;FMTTYPE=text/html:<p data-block-key="l6aes">Abstract:<br/>The p
 roperties of the Higgs boson together with the absence of new physics at t
 he Large Hadron Collider allow us to speculate about consistently extendin
 g the Standard Model all the way up to the Planck scale while staying in t
 he perturbative regime.<br/><br/> In this context\, the SM Higgs non-minim
 ally coupled to gravity could be responsible for the symmetry properties o
 f the Universe at large scales and the generation of the primordial spectr
 um of temperature fluctuations seen in the Cosmic Microwave Background (CM
 B).<br/><br/>In this work we show how Higgs-Inflation and its scale-invari
 ant extension\, known as Higgs-Dilaton inflation\, can be embedded in Eins
 tein-Cartan gravity.<br/>In particular we will discuss some phenomenologic
 al features emerging from the inflationary and post-inflationary dynamics.
 </p>
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