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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

If the LHC does only find a Higgs boson in the low mass region and no other new physics, then one should reconsider scenarios where the Standard Model with three right-handed neutrinos is valid up to Planck scale. We assume in this spirit…

高能物理 - 唯象学 · 物理学 2012-03-05 Martin Holthausen , Kher Sham Lim , Manfred Lindner

Using a physical renormalisation scheme we derive mass-dependent renormalisation group equations for the running of the Higgs quartic coupling within the Standard Model. Subsequently, we accurately take into account weak scale thresholds,…

高能物理 - 唯象学 · 物理学 2014-07-25 Alexander Spencer-Smith

After the discovery of the Higgs particle the most relevant structures of the SM have been verified and for the first time we know all parameters of the SM within remarkable accuracy. Together with recent calculations of the SM…

高能物理 - 唯象学 · 物理学 2015-06-22 Fred Jegerlehner

We propose a theoretical justification for the anomalous Higgs couplings without extending the particle content of the Standard Model, but rather assuming different realization of the electroweak symmetry and the representation of the Higgs…

高能物理 - 唯象学 · 物理学 2012-08-30 Archil Kobakhidze

In the Standard Model (SM), the Higgs mass around 125 GeV implies that the electroweak vacuum is metastable since the quartic Higgs coupling turns negative at high energies. I point out that a tiny mixing of the Higgs with a heavy singlet…

高能物理 - 唯象学 · 物理学 2015-06-04 Oleg Lebedev

The measured (central) values of the Higgs and top quark masses indicate that the Standard Model (SM) effective potential develops an instability at high field values. The scale of this instability, determined as the Higgs field value at…

高能物理 - 唯象学 · 物理学 2017-03-15 Jose R. Espinosa , Mathias Garny , Thomas Konstandin , Antonio Riotto

In this talk we review the actual situation concerning electroweak phase transition and baryogenesis in the minimal supersymmetric extension of the Standard Model. A strong enough phase transition requires light Higgs and stop eigenstates.…

高能物理 - 唯象学 · 物理学 2014-11-17 Mariano Quiros

Electroweak baryogenesis in the minimal supersymmetric extension of the Standard Model may be realized within the light stop scenario, where the right-handed stop mass remains close to the top-quark mass to allow for a sufficiently strong…

高能物理 - 唯象学 · 物理学 2009-01-06 Marcela Carena , Germano Nardini , Mariano Quiros , Carlos E. M. Wagner

Motivated by the stability of the electroweak Higgs vacuum we consider the possibility that the Standard Model might work up to large scales between about $10^{10}$ GeV and close to the Planck scale. A plausible scenario is an emergent…

高能物理 - 唯象学 · 物理学 2024-02-23 Steven D. Bass

The discovery of the Higgs boson by the LHC and the measurement of its mass at around 125 GeV, taken together with the absence of signals of physics beyond the standard model, make it possible that we might live in a metastable electroweak…

高能物理 - 唯象学 · 物理学 2015-12-04 Jose R. Espinosa

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

We update instability and metastability bounds of the Standard Model electroweak vacuum in view of the recent ATLAS and CMS Higgs results. For a Higgs mass in the range 124--126 GeV, and for the current central values of the top mass and…

高能物理 - 唯象学 · 物理学 2015-06-03 Joan Elias-Miro , Jose R. Espinosa , Gian F. Giudice , Gino Isidori , Antonio Riotto , Alessandro Strumia

We propose that the Standard Model (SM) Higgs is responsible for generating the cosmological perturbations of the universe by acting as an isocurvature mode during a de Sitter inflationary stage. In view of the recent ATLAS and CMS results…

高能物理 - 唯象学 · 物理学 2013-02-11 Andrea De Simone , Antonio Riotto

Light states associated with the hierarchy problem affect the Higgs LHC production and decays. We illustrate this within the MSSM and two simple extensions applying the latest bounds from LHC Higgs searches. Large deviations in the Higgs…

高能物理 - 唯象学 · 物理学 2015-06-03 Asimina Arvanitaki , Giovanni Villadoro

Imposing the constraint that the Standard Model effective Higgs potential should have two degenerate minima ( vacua), one of which should be - order of magnitudewise - at the Planck scale, leads to the top mass being 173 +/- 5 GeV and the…

高能物理 - 唯象学 · 物理学 2009-10-28 C. D. Froggatt , H. B. Nielsen

In this paper we investigate the vacuum stability of the non-minimally coupled Standard-Model Higgs during a phase of kinetic domination following the end of inflation. The non-minimal coupling to curvature stabilises the Higgs fluctuations…

高能物理 - 唯象学 · 物理学 2024-05-01 Giorgio Laverda , Javier Rubio

Based on two postulations that (i) the Higgs boson has a large bare mass $m_H \gg m_h \simeq 125 $ GeV at the characteristic energy scale $M_c$ which defines the standard model (SM) in the ultraviolet region, and (ii) quadratic…

高能物理 - 唯象学 · 物理学 2015-05-26 Dong Bai , Jian-Wei Cui , Yue-Liang Wu

We consider the possibility that the gauge hierarchy is a byproduct of the metastability of the electroweak vacuum, i.e., that whatever mechanism is responsible for the latter also sets the running Higgs mass to a value smaller than its…

高能物理 - 唯象学 · 物理学 2022-04-13 Justin Khoury , Thomas Steingasser

The discovery of Standard-Model like Higgs at 125 GeV may raise more questions than the answers it provides. In particular, the hierarchy problem remains unsolved, and the Standard Model Higgs quartic self-coupling becomes negative below…

高能物理 - 唯象学 · 物理学 2023-03-08 Ash Arsenault , Kivanc Y. Cingiloglu , Mariana Frank