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相关论文: Higgs inflation with loop corrections in the Palat…

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We consider critical Higgs inflation, namely Higgs inflation with a rising inflection point at smaller field values than those of the plateau induced by the non-minimal coupling to gravity. It has been proposed that such configuration is…

高能物理 - 唯象学 · 物理学 2018-09-12 Isabella Masina

We analyse the self-consistency of inflation in the Standard Model, where the Higgs field has a large non-minimal coupling to gravity. We determine the domain of energies in which this model represents a valid effective field theory as a…

高能物理 - 唯象学 · 物理学 2011-03-07 F. Bezrukov , A. Magnin , M. Shaposhnikov , S. Sibiryakov

The action of loop quantum gravity includes the Holst term and/or the Nieh-Yan term in addition to the Ricci scalar. These terms are expected to couple non-minimally to the Higgs. Thus the Holst and Nieh-Yan terms contribute to the…

宇宙学与河外天体物理 · 物理学 2021-04-28 Miklos Långvik , Juha-Matti Ojanperä , Sami Raatikainen , Syksy Rasanen

We present a class of non-supersymmetric models in which so-called critical Higgs inflation ($\xi<100$) naturally can be realized without using specific values for Higgs and top quark masses. In these scenarios, the Standard Model (SM)…

高能物理 - 唯象学 · 物理学 2021-05-18 Heng-Yu Chen , Ilia Gogoladze , Shan Hu , Tianjun Li , Lina Wu

We study preheating following Higgs inflation in the Palatini formulation of gravity. We numerically evolve perturbations of the radial mode of the Higgs field and that of three scalars modeling the gauge bosons. We compare the two…

高能物理 - 唯象学 · 物理学 2022-09-20 Frédéric Dux , Adrien Florio , Juraj Klarić , Andrey Shkerin , Inar Timiryasov

We study single field slow-roll inflation in the presence of $F(R)$ gravity in the Palatini formulation. In contrast to metric $F(R)$, when rewritten in terms of an auxiliary field and moved to the Einstein frame, Palatini $F(R)$ does not…

广义相对论与量子宇宙学 · 物理学 2022-07-12 Christian Dioguardi , Antonio Racioppi , Eemeli Tomberg

We consider models of a scalar field coupled to quadratic $R\!+\!R^2$ gravity in the framework of the Palatini formulation. The resulting Einstein-frame generalized $k$-inflation effective theory is analyzed assuming that the constant-roll…

广义相对论与量子宇宙学 · 物理学 2020-04-29 Ignatios Antoniadis , Angelos Lykkas , Kyriakos Tamvakis

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 present three features which can be used to distinguish the R^2-inflation Higgs-inflation from with ongoing, upcoming and planned experiments, assuming no new physics (apart form sterile neutrinos) up to inflationary scale. (i) Slightly…

高能物理 - 唯象学 · 物理学 2012-08-30 Fedor Bezrukov , Dmitry Gorbunov

We propose a novel possibility for Higgs inflation where the perturbative unitarity below the Planck scale is ensured by construction and the successful predictions for inflation are accommodated. The conformal gravity coupling for the…

高能物理 - 唯象学 · 物理学 2023-10-17 Simon Cléry , Hyun Min Lee , Adriana G. Menkara

We analyze a two-field inflationary model consisting of the Ricci scalar squared ($R^2$) term and the standard Higgs field non-minimally coupled to gravity in addition to the Einstein $R$ term. Detailed analysis of the power spectrum of…

宇宙学与河外天体物理 · 物理学 2018-06-13 Minxi He , Alexei A. Starobinsky , Jun'ichi Yokoyama

We have recently suggested [1,2] that Inflation could have started in a local minimum of the Higgs potential at field values of about $10^{15}-10^{17}$ GeV, which exists for a narrow band of values of the top quark and Higgs masses and thus…

高能物理 - 唯象学 · 物理学 2015-06-04 Isabella Masina , Alessio Notari

We consider a possibility that the Higgs field in the Standard Model (SM) serves as an inflaton when its value is around the Planck scale. We assume that the SM is valid up to an ultraviolet cutoff scale \Lambda, which is slightly below the…

高能物理 - 唯象学 · 物理学 2014-02-11 Yuta Hamada , Hikaru Kawai , Kin-ya Oda

We investigate inflationary Higgs dynamics and constraints on the Standard Model parameters assuming the Higgs potential, computed to next-to-next leading order precision, is not significantly affected by new physics. For a high…

高能物理 - 唯象学 · 物理学 2015-06-19 Kari Enqvist , Tuukka Meriniemi , Sami Nurmi

We consider an extension of Higgs inflation in which the Higgs field is non-minimally coupled to gravity through its kinetic term. We analyzed power-law coupling functions with positive or negative integer power and found that the Higgs…

广义相对论与量子宇宙学 · 物理学 2020-05-18 L. N. Granda , D. F. Jimenez , W. Cardona

If the inflaton and the quintessence fields are identified, the background geometry evolves through a stiff epoch undershooting the expansion rate of a radiation-dominated plasma. For some classes of inflationary potentials this scenario is…

广义相对论与量子宇宙学 · 物理学 2020-01-08 Massimo Giovannini

We revisit Higgs inflation in the framework of a minimal extension of the Standard Model gauge symmetry by a $U(1)_{B-L}$ factor. Various aspects are taken into account with particular focus on the role of the supersymmetry breaking (SUSY)…

高能物理 - 唯象学 · 物理学 2021-09-29 Waqas Ahmed , Athanasios Karozas , George K. Leontaris

It has been pointed out that a large non-minimal coupling $\xi$ between the Higgs and the Ricci scalar can source higher derivative operators, which may change the predictions of Higgs inflation. A variant, called critical Higgs inflation,…

高能物理 - 唯象学 · 物理学 2018-04-03 Alberto Salvio

Higgs inflation and $R^2$-inflation (Starobinsky model) are two limits of the same quantum model, hereafter called Starobinsky-Higgs. We analyse the two-loop action of the Higgs-like scalar $\phi$ in the presence of: 1) non-minimal coupling…

高能物理 - 唯象学 · 物理学 2018-12-05 D. M. Ghilencea

In cosmic inflation driven by a scalar gauge singlet field with a tree level Higgs potential, the scalar to tensor ratio r is estimated to be larger than 0.036, provided the scalar spectral index n_s >= 0.96. We discuss quantum smearing of…

宇宙学与河外天体物理 · 物理学 2011-02-28 Mansoor Ur Rehman , Qaisar Shafi