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相关论文: Probing the Seesaw Mechanism with Cosmological Dat…

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We discuss how the non-minimal coupling $\xi \phi^2 R$ between the inflaton and the Ricci scalar affects predictions of single field inflation models in Palatini formalism. To transition radiation dominated era, the inflaton field $\phi$…

广义相对论与量子宇宙学 · 物理学 2020-11-26 Nilay Bostan

Scalar field with non-minimal coupling to curvature scalar is studied in Robertson-Walker background. The infrared limit of two point function, and, in turn, of the energy-momentum tensor of scalar field have been considered in the power…

广义相对论与量子宇宙学 · 物理学 2020-07-16 Amit Kundu , Prasenjit Paul

It is well known that the non-minimal coupling $\xi\phi^2R$ between the inflaton and the Ricci scalar affects predictions of single field inflation models. In particular, the $\lambda\phi^4$ quartic inflation potential with…

宇宙学与河外天体物理 · 物理学 2019-10-11 Nilay Bostan , Vedat Nefer Şenoğuz

With the growing consensus on simple power law inflation models not being favored by the PLANCK observation, dynamics for the non-standard form of the inflaton potential gain significant interest in the recent past. In this paper, we…

宇宙学与河外天体物理 · 物理学 2019-02-08 Debaprasad Maity , Pankaj Saha

We discuss non-minimal quadratic inflation in supersymmetric (SUSY) and non-SUSY models which entails a linear coupling of the inflaton to gravity. Imposing a lower bound on the parameter cR, involved in the coupling between the inflaton…

高能物理 - 唯象学 · 物理学 2015-03-31 Constantinos Pallis , Qaisar Shafi

Models of cosmic inflation suggest that our universe underwent an early phase of accelerated expansion, driven by the dynamics of one or more scalar fields. Inflationary models make specific, quantitative predictions for several observable…

宇宙学与河外天体物理 · 物理学 2016-05-10 David I. Kaiser

We explore inflationary cosmology in a theory where there are two scalar fields which non-minimally couple to the Ricci scalar and an additional $R^2$ term, which breaks the conformal invariance. Particularly, we investigate the slow-roll…

高能物理 - 理论 · 物理学 2015-07-10 Kazuharu Bamba , Sergei D. Odintsov , Petr V. Tretyakov

We construct a class of single small field models of inflation that can predict, contrary to popular wisdom, an observable gravitational wave signal in the cosmic microwave background anisotropies. The spectral index, its running, the…

宇宙学与河外天体物理 · 物理学 2014-11-20 Ido Ben-Dayan , Ram Brustein

A field kinetic coupling with the Einstein tensor leads to a gravitationally enhanced friction during inflation, by which even steep potentials with theoretically natural model parameters can drive cosmic acceleration. In the presence of…

宇宙学与河外天体物理 · 物理学 2015-06-03 Shinji Tsujikawa

Supersymmetric Unified theories which incorporate a renormalizable Type I seesaw mechanism for small neutrino masses can also provide slow roll inflection point inflation along a flat direction associated with a gauge invariant combination…

高能物理 - 唯象学 · 物理学 2012-09-21 Charanjit S. Aulakh , Ila Garg

It is a longstanding desire of cosmologists, and particle physicists as well, to connect inflation to low energy physics, culminating, for instance, in what is known as Higgs inflation. The condition for the standard Higgs boson playing the…

高能物理 - 唯象学 · 物理学 2017-11-15 J. G. Ferreira , C. A. de S. Pires , J. G. Rodrigues , P. S. Rodrigues da Silva

We discuss realization of cosmic inflation in the $\nu$-gauge mediated supersymmetry breaking scenario, in which a set of 24-dimensional chiral superfields responsible for the type III seesaw mechanism play the role of the messenger fields…

高能物理 - 唯象学 · 物理学 2022-01-05 Shinsuke Kawai , Nobuchika Okada

In a variety of inflation models the motion of the inflaton may trigger the production of some non-inflaton particles during inflation, for example via parametric resonance or a phase transition. Particle production during inflation leads…

宇宙学与河外天体物理 · 物理学 2010-01-07 Neil Barnaby , Zhiqi Huang

We study a model of inflation where the scalar perturbations are almost gaussian while there is sizable (equilateral) nongaussianity in the tensor sector. In this model, a rolling pseudoscalar gravitationally coupled to the inflaton…

宇宙学与河外天体物理 · 物理学 2013-11-28 Jessica L. Cook , Lorenzo Sorbo

The apparent alignment of the cosmic microwave background multipoles on large scales challenges the standard cosmological model. Scalar field inflation is isotropic and cannot account for the observed alignment. We explore the imprints, a…

天体物理学 · 物理学 2010-04-14 Christian G. Boehmer , David F. Mota

We investigate a scenario of cosmological inflation realised along a flat direction of the minimal seesaw model embedded in supergravity with a noncanonical R-parity violating K\"{a}hler potential. It is shown that with appropriate seesaw…

高能物理 - 唯象学 · 物理学 2013-11-07 Masato Arai , Shinsuke Kawai , Nobuchika Okada

We study a variant of the Chromo-Natural Inflation (CNI) mechanism in which the inflaton interacts only gravitationally with the CNI fields. Integrating out all the non-dynamical scalar fields of the model results in a coupling between the…

宇宙学与河外天体物理 · 物理学 2019-09-04 Alexandros Papageorgiou , Marco Peloso , Caner Unal

We perform a combined perturbation and observational investigation of the scenario of non-minimal derivative coupling between a scalar field and curvature. First we extract the necessary condition that ensures the absence of instabilities,…

宇宙学与河外天体物理 · 物理学 2013-12-02 James B. Dent , Sourish Dutta , Emmanuel N. Saridakis , Jun-Qing Xia

Inflationary scenarios motivated by the Minimal Supersymmetric Standard Model (MSSM) where five scalar fields are non-minimally coupled to gravity are considered. The potential of the model and the function of non-minimal coupling are…

高能物理 - 唯象学 · 物理学 2018-06-01 M. N. Dubinin , E. Yu. Petrova , E. O. Pozdeeva , S. Yu. Vernov

This thesis presents a possible inflation scenario as a consequence of non-minimal gravitational couplings in the Conformal Standard Model. That model consists, in comparison to the SM, of additional right-chiral neutrinos and a complex…

广义相对论与量子宇宙学 · 物理学 2019-11-13 Jan Henryk Kwapisz