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By studying the chameleon model during inflation, we investigate whether it can be a successful inflationary model, wherein we employ the common typical potential usually used in the literature. Thus, in the context of the slow-roll…

广义相对论与量子宇宙学 · 物理学 2018-04-13 Nasim Saba , Mehrdad Farhoudi

Inflation generally assumes a field with nonzero potential that leads to inflationary expansion happening at arbitrarily early times. We demonstrate potentially observable consequences of inflation with a finite initial time in a model in…

高能物理 - 理论 · 物理学 2025-12-05 Rashmish K. Mishra , Michael Nee , Lisa Randall

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

Quantum origin of the early inflationary Universe from the no-boundary and tunnelling quantum states is considered in the one-loop approximation of quantum cosmology. A universal effective action algorithm for the distribution function of…

广义相对论与量子宇宙学 · 物理学 2011-04-15 A. O. Barvinsky , A. Yu. Kamenshchik

We attempt to incorporate inflation into a string theory realization of the chameleon mechanism. Previously, it was found that the volume modulus, stabilized by the supersymmetric potential used by Kachru, Kallosh, Linde and Trivedi (KKLT)…

高能物理 - 理论 · 物理学 2013-08-19 Kurt Hinterbichler , Justin Khoury , Horatiu Nastase , Rogerio Rosenfeld

A model of inflation is proposed in which compact extra dimensions allow a graceful exit without recourse to flat potentials or super-Planckian field values. Though bubbles of true vacuum are too sparse to uniformly reheat the Universe by…

高能物理 - 理论 · 物理学 2008-12-18 Adam R. Brown

A model of a universe without big bang singularity is presented, which displaysanearly inflationary period ending just before a phase transition to a deflationary epoch. The model produces enough heavy particles so as to reheat the universe…

广义相对论与量子宇宙学 · 物理学 2016-09-05 Jaume de Haro , Emilio Elizalde

We study the constraint on the inflationary energy scale from the recently proposed Trans-Planckian Censorship Conjecture (TCC). We find a universal upper bound on the inflationary Hubble expansion rate $H_\text{inf}$ which is solely…

宇宙学与河外天体物理 · 物理学 2020-07-29 Shuntaro Mizuno , Shinji Mukohyama , Shi Pi , Yun-Long Zhang

We present a new approach to constructing inflationary models in closed universes. Conformal embedding of closed-universe models in a de Sitter background suggests a quantisation condition on the available conformal time. This condition…

天体物理学 · 物理学 2009-11-10 Anthony Lasenby , Chris Doran

A brief review of the modern state of quantum cosmology is presented as a theory of quantum initial conditions for inflationary scenario. The no-boundary and tunneling states of the Universe are discussed as a possible source of probability…

广义相对论与量子宇宙学 · 物理学 2017-08-23 A. O. Barvinsky

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

We investigate the modifications to inflationary observables that arise when adopting an $\alpha$-vacuum instead of the standard Bunch--Davies vacuum for quantum fluctuations during inflation. Within the Starobinsky inflationary model, we…

广义相对论与量子宇宙学 · 物理学 2026-05-11 Melo Wood-Saanaoui , Rudnei O. Ramos , Arjun Berera

In the context of inflationary models with a pre-inflationary stage, in which the Einstein equations are obeyed, the weak energy condition is satisfied, and spacetime topology is trivial, we argue that homogeneity on super-Hubble scales…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Tanmay Vachaspati , Mark Trodden

We discuss inflation in models with large extra dimensions, driven by a bulk scalar field. The brane inflaton is then a single effective field, obtained from the bulk scalar field by scaling. The self interaction terms of the effective…

高能物理 - 唯象学 · 物理学 2008-11-26 R. N. Mohapatra , A. Pérez-Lorenzana , C. A. de S. Pires

We consider supersymmetric inflation with the hybrid-type potential. In the absence of the symmetry that forbids Hubble-induced mass terms, the inflaton mass will be as large as the Hubble scale during inflation. We consider gravitational…

高能物理 - 唯象学 · 物理学 2010-02-15 Tomohiro Matsuda

In this study, we provide an alternatively reformulated interpretation of Gibbons-Hawking radiation as well as inflation. By using a spacetime quantization procedure, proposed recently by L.C. C\'eleri et al., in anti-de Sitter space we…

广义相对论与量子宇宙学 · 物理学 2020-05-08 Naouel Boulkaboul

We study quantum gravity constraints on inflationary model building. Our approach is based on requiring the entropy associated to a given inflationary model to be less than that of the de Sitter entropy. We give two prescriptions for…

高能物理 - 理论 · 物理学 2015-06-04 Joseph P. Conlon

Predictions of inflationary schemes can be influenced by the presence of extra dimensions. This could be of particular relevance for the spectrum of gravitational waves in models where the extra dimensions provide a brane-world solution to…

高能物理 - 唯象学 · 物理学 2018-03-09 Sang Hui Im , Hans Peter Nilles , Andreas Trautner

Possibly, the most general action in the background of isotropic and homogeneous space-time has been considered to study the quantum evolution of the early universe, apart from a cosmological constant. The hermiticity of the effective…

高能物理 - 理论 · 物理学 2020-10-30 Ranajit Mandal , Dalia Saha , Mohosin Alam , Abhik Kumar Sanyal

The tunneling hamiltonian has proven to be a useful method in many body physics to treat particle tunneling between different states represented as wave functions. Here we apply a generalization of a way we formed appropriate wave…

数学物理 · 物理学 2007-05-23 A. W. Beckwith