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相关论文: Inflation with sterile scalar coupled to massive f…

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I study a fresh inflationary model with a scalar field nonminimally coupled to gravity. An example is examined. I find that, as larger is the value of $p$ (the power of the scale factor), smaller (but larger in its absolute value) is the…

高能物理 - 唯象学 · 物理学 2007-05-23 Mauricio Bellini

We explore the classical and quantum properties of a sterile scalar field coupled to $N$ copies of Dirac fermions in an external gravitational field. We find that the self-interaction scalar potential of a model that is consistent at the…

A new class of gravity-matter model defined with an independent non-Riemannian volume form is studied, in the second order formalism. The action has a global scale invariance symmetry, which can be broken by the equation of motion of the…

广义相对论与量子宇宙学 · 物理学 2019-05-22 David Benisty , Eduardo I. Guendelman

We re-examine large scalar fields within effective field theory, in particular focussing on the issues raised by their use in inflationary models (as suggested by BICEP2 to obtain primordial tensor modes). We argue that when the large-field…

高能物理 - 理论 · 物理学 2015-03-18 C. P. Burgess , M. Cicoli , F. Quevedo , M. Williams

We revisit an extension of the well-known formalism for gauge-invariant scalar metric fluctuations, to study the spectrums for both, the inflaton and gauge invariant (scalar) metric fluctuations in the framework of a single field…

广义相对论与量子宇宙学 · 物理学 2009-11-13 Mariano Anabitarte , Mauricio Bellini

One of the fundamental objectives of contemporary cosmology is to understand the physics of the inflationary universe, owing to its observably verifiable predictions about the very early universe with an energy scale of $\sim 10^{16}$ GeV.…

宇宙学与河外天体物理 · 物理学 2026-04-14 Aayush Randeep , Rajib Saha

We propose a new class of natural inflation models based on a hidden scale invariance. In a very generic Wilsonian effective field theory with an arbitrary number of scalar fields, which exhibits scale invariance via the dilaton, the…

广义相对论与量子宇宙学 · 物理学 2016-04-20 Neil D. Barrie , Archil Kobakhidze , Shelley Liang

We propose a novel scenario in which scalar perturbations, that seed the large scale structure of the Universe, are generated without relying on a scalar field (the inflaton). In this framework, inflation is driven by a de Sitter space-time…

宇宙学与河外天体物理 · 物理学 2024-12-20 Daniele Bertacca , Raul Jimenez , Sabino Matarrese , Angelo Ricciardone

We study the production of fermions through a derivative coupling with a pseudoscalar inflaton and the effects of the produced fermions on the scalar primordial perturbations. We present analytic results for the modification of the scalar…

宇宙学与河外天体物理 · 物理学 2019-11-18 Peter Adshead , Lauren Pearce , Marco Peloso , Michael A. Roberts , Lorenzo Sorbo

We study the cosmology of a toy modified theory of gravity in which gravity shuts off at short distances, as in the fat graviton scenario of Sundrum. In the weak-field limit, the theory is perturbatively local, ghost-free and unitary,…

高能物理 - 理论 · 物理学 2008-11-26 Justin Khoury

If the inflaton is a pseudo-scalar axion, the axion shift symmetry can protect the flatness of its potential from too large radiative corrections. This possibility, known as natural inflation, requires an axion scale which is greater than…

高能物理 - 唯象学 · 物理学 2009-11-10 Jihn E. Kim , Hans Peter Nilles , Marco Peloso

We propose a large class of supergravity models in terms of a single chiral matter superfield, leading to (almost) arbitrary single-field inflationary scalar potentials similar to the F-term in rigid supersymmetry. Those scalar potentials…

高能物理 - 理论 · 物理学 2015-02-25 Sergei V. Ketov , Takahiro Terada

Processes of particle production during inflation can increase the amplitude of the scalar metric perturbations. We show that such a mechanism can naturally arise in supergravity models where an axion-like field, whose potential is…

高能物理 - 唯象学 · 物理学 2021-07-07 Michael A. Roberts , Lorenzo Sorbo

Inflation is often described through the dynamics of a scalar field, slow-rolling in a suitable potential. Ultimately, this inflaton must be identified as the expectation value of a quantum field, evolving in a quantum effective potential.…

高能物理 - 唯象学 · 物理学 2021-05-11 Jens O. Andersen , Magdalena Eriksson , Anders Tranberg

If the conformal invariance of electromagnetism is broken during inflation, then primordial magnetic fields may be produced. If this symmetry breaking is generated by the coupling between electromagnetism and a scalar field---e.g. the…

宇宙学与河外天体物理 · 物理学 2013-05-29 Robert R. Caldwell , Leonardo Motta , Marc Kamionkowski

We consider a subclass of Horndeski theories for studying cosmic inflation. In particular, we investigate models of inflation in which the derivative self-interaction of the scalar field and the non-minimal derivative coupling to gravity…

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

In this paper we consider a new approach to unify inflation and the late universe with dark energy and dark matter formulated in a model that includes a non-Riemannian metric independent measure and a scalar field with spontaneously broken…

广义相对论与量子宇宙学 · 物理学 2025-01-31 Eduardo Guendelman , Ramon Herrera

We study a single field axion inflation model in the presence of an SU(2) gauge field with a small vev. In order to make the analysis as model-independent as possible, we consider an arbitrary potential for the axion that is able to support…

高能物理 - 唯象学 · 物理学 2016-08-24 Azadeh Maleknejad

A single field inflation based on a supergravity model with a shift symmetry and $U(1)$ extension of the MSSM is analyzed. We show that one of the real components of the two $U(1)$ charged scalar fields plays the role of inflaton {with} an…

高能物理 - 唯象学 · 物理学 2015-10-28 Lucien Heurtier , Shaaban Khalil , Ahmad Moursy

Weyl (scale) invariant theories of scalars and gravity can generate all mass scales spontaneously. In this paper we study a particularly simple version -- scale invariant $R^2$ gravity -- and show that, during an inflationary period, it…

广义相对论与量子宇宙学 · 物理学 2019-12-18 Pedro G. Ferreira , Christopher T. Hill , Johannes Noller , Graham G. Ross
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