中文
相关论文

相关论文: The Tachyonic Higgs and the Inflationary Universe

200 篇论文

In the Standard Model, the Higgs potential develops an instability at high field values when the quartic self-coupling runs negative. Large quantum fluctuations during cosmic inflation could drive the Higgs field beyond the potential…

高能物理 - 唯象学 · 物理学 2026-01-07 G. Franciolini , A. Kehagias , A. Riotto

The Standard Model Higgs potential becomes unstable at large Higgs field values where its quartic coupling becomes negative. While the tunneling lifetime of our current electroweak vacuum is comfortably longer than the age of the universe,…

高能物理 - 唯象学 · 物理学 2022-09-28 Valerio De Luca , Alex Kehagias , Antonio Riotto

The Higgs potential appears to be fine-tuned, hence very sensitive to values of other scalar fields that couple to the Higgs. We show that this feature can lead to a new epoch in the early universe featuring violent dynamics coupling the…

高能物理 - 唯象学 · 物理学 2019-02-20 Mustafa A. Amin , JiJi Fan , Kaloian D. Lozanov , Matthew Reece

We assume the validity of the Standard Model up to an arbitrary high-energy scale and discuss what information on the early stages of the Universe can be extracted from a measurement of the Higgs mass. For Mh < 130 GeV, the Higgs potential…

高能物理 - 唯象学 · 物理学 2009-01-06 J. R. Espinosa , G. Giudice , A. Riotto

It has recently been suggested that at the post-inflationary stage of the mixed Higgs-$R^2$ model of inflation efficient particle production can arise from the tachyonic instability of the Higgs field. It might complete the preheating of…

高能物理 - 唯象学 · 物理学 2021-02-03 Minxi He , Ryusuke Jinno , Kohei Kamada , Alexei A. Starobinsky , Jun'ichi Yokoyama

The Higgs field is an attractive candidate for the inflaton because it is an observationally confirmed fundamental scalar field. Importantly, it can be modeled by the most general renormalizable scalar potential. However, if the classical…

宇宙学与河外天体物理 · 物理学 2021-03-29 Martin Bojowald , Suddhasattwa Brahma , Sean Crowe , Ding Ding , Joseph McCracken

We study the dynamics of the standard model Higgs field in the inflationary cosmology. Since metastability of our vacuum is indicated by the current experimental data of the Higgs boson and top quark, inflation models with a large Hubble…

高能物理 - 唯象学 · 物理学 2015-06-22 Kohei Kamada

The Standard Model Higgs potential becomes unstable at large field values. After clarifying the issue of gauge dependence of the effective potential, we study the cosmological evolution of the Higgs field in presence of this instability…

Measurements of the Higgs boson and top quark masses indicate that the Standard Model Higgs potential becomes unstable around $\Lambda_I \sim 10^{11}$ GeV. This instability is cosmologically relevant since quantum fluctuations during…

高能物理 - 唯象学 · 物理学 2015-06-19 Anson Hook , John Kearney , Bibhushan Shakya , Kathryn M. Zurek

Inflation is nowadays a well-established paradigm consistent with all the observations. The precise nature of the inflaton is however unknown and its role could be played by any candidate able to imitate a scalar condensate in the slow-roll…

高能物理 - 唯象学 · 物理学 2015-09-02 Javier Rubio

Even if nothing but a light Higgs is observed at the LHC, suggesting that the Standard Model is unmodified up to scales far above the weak scale, Higgs physics can yield surprises of fundamental significance for cosmology. As has long been…

高能物理 - 唯象学 · 物理学 2009-05-22 Nima Arkani-Hamed , Sergei Dubovsky , Leonardo Senatore , Giovanni Villadoro

The measured Standard Model parameters lie in a range such that the Higgs potential, once extrapolated up to high scales, develops a minimum of negative energy density. This has important cosmological implications. In particular, during…

高能物理 - 唯象学 · 物理学 2020-05-29 Jacopo Fumagalli , Sébastien Renaux-Petel , John W. Ronayne

The running of the Higgs self coupling may lead to numerous phenomena in early universe cosmology. In this paper we introduce a scenario where the Higgs running induces turns in the trajectory passing a region with tachyonic mass, leading…

高能物理 - 唯象学 · 物理学 2022-10-12 Dhong Yeon Cheong , Kazunori Kohri , Seong Chan Park

The measurements of the Higgs mass and top Yukawa coupling indicate that we live in a very special Universe, at the edge of the absolute stability of the electroweak vacuum. If fully stable, the Standard Model (SM) can be extended all the…

高能物理 - 唯象学 · 物理学 2015-10-27 Fedor Bezrukov , Javier Rubio , Mikhail Shaposhnikov

Within the Standard Model, the current Higgs and top quark data favor metastability of the electroweak vacuum, although the uncertainties are still significant. The true vacuum is many orders of magnitude deeper than ours and the barrier…

高能物理 - 唯象学 · 物理学 2015-06-11 Oleg Lebedev , Alexander Westphal

This paper explores various aspects and implications of the initial configuration of the Standard Model (SM) Higgs field at the beginning of our Universe. It is well known that the SM Higgs field features a deeper, more stable minimum at…

高能物理 - 唯象学 · 物理学 2025-11-13 Bibhushan Shakya

A remarkable prediction of the Standard Model is that, in the absence of corrections lifting the energy density, the Higgs potential becomes negative at large field values. If the Higgs field samples this part of the potential during…

高能物理 - 唯象学 · 物理学 2017-02-09 William E. East , John Kearney , Bibhushan Shakya , Hojin Yoo , Kathryn M. Zurek

So far, the experiments at the Large Hadron Collider (LHC) have shown no sign of new physics beyond the Standard Model. Assuming the Standard Model is correct at presently available energies, we can accurately extrapolate the theory to…

高能物理 - 唯象学 · 物理学 2014-04-23 Archil Kobakhidze , Alexander Spencer-Smith

The properties of the recently discovered Higgs boson together with the absence of new physics at collider experiments allows us to speculate about consistently extending the Standard Model of particle physics all the way up to the Planck…

高能物理 - 唯象学 · 物理学 2019-03-14 Javier Rubio

We study the inflationary evolution of a scalar field $h$ with an unstable potential for the case where the Hubble parameter $H$ during inflation is larger than the instability scale $\Lambda_I$ of the potential. Quantum fluctuations in the…

高能物理 - 理论 · 物理学 2016-03-14 John Kearney , Hojin Yoo , Kathryn M. Zurek
‹ 上一页 1 2 3 10 下一页 ›