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相关论文: Supersymmetric inflation and large-scale structure

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We identify a new mechanism in supergravity theories which leads to successful inflation without any need for fine tuning. The simplest model yields a spectrum of density fluctuations tilted away from scale-invariance and negligible…

高能物理 - 唯象学 · 物理学 2014-11-17 Jennifer A. Adams , Graham G. Ross , Subir Sarkar

The temperature fluctuations in the cosmic microwave background observed by COBE provide strong support for an inflationary phase in the early universe, below the GUT scale. We argue that a singlet field in a hidden sector of an effective…

高能物理 - 唯象学 · 物理学 2007-05-23 Subir Sarkar

We reconsider the problems of cosmological inflation in effective supergravity theories. A singlet field in a hidden sector is demonstrated to yield an acceptable inflationary potential, without fine tuning. In the simplest such model, the…

高能物理 - 唯象学 · 物理学 2011-02-16 G. G. Ross , S. Sarkar

We propose a new class of inflationary models in which the scalar field potential governing inflation is generated by the same non-perturbative gauge dynamics that may lead to supersymmetry breaking. Such models satisfy constraints from…

高能物理 - 唯象学 · 物理学 2011-05-23 William H. Kinney , Antonio Riotto

We show that a moduli space of the form predicted by string theory, lifted by supersymmetry breaking, gives rise to successful inflation for large regions of parameter space without any modification or fine tuning. This natural realization…

高能物理 - 唯象学 · 物理学 2009-11-10 Kenji Kadota , Ewan D. Stewart

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

Inflation generates gravitational waves, which may be observable in the low multipoles of the cosmic microwave background (cmb) anisotropy but only if the inflaton field variation is at least of order the Planck scale. Such a large…

高能物理 - 唯象学 · 物理学 2009-10-28 David H. Lyth

High-scale string inflationary models are in well-known tension with low-energy supersymmetry. A promising solution involves models where the inflaton is the volume of the extra dimensions so that the gravitino mass relaxes from large…

高能物理 - 理论 · 物理学 2016-01-20 Michele Cicoli , Francesco Muia , Francisco Gil Pedro

Supergravity, a locally supersymmetric gauge theory, may provide to describe new physics beyond the Standard Model (BSM). In this sense, cosmological applications of supergravity can be the arena for probing outcomes of supergravity. It is…

高能物理 - 理论 · 物理学 2022-06-29 Hun Jang

The cosmological implication of a double inflation model with hybrid + new inflations in supergravity is studied. The hybrid inflation drives an inflaton for new inflation close to the origin through supergravity effects and new inflation…

高能物理 - 唯象学 · 物理学 2009-10-31 Toshiyuki Kanazawa , M. Kawasaki , Naoshi Sugiyama , T. Yanagida

We present a supergravity inflationary scenario in which the inflaton field takes values considerably larger than the Planck scale. It is based on a class of inflationary potentials which can be derived from ``singular'' Kaehler potentials…

高能物理 - 唯象学 · 物理学 2009-10-31 C. Panagiotakopoulos

Inflation may have been driven by a component which violated the Null-Energy Condition, thereby leading to {\it super inflation}. We provide the formalism to study cosmological perturbations when such a component is described by a scalar…

天体物理学 · 物理学 2010-09-21 Marco Baldi , Fabio Finelli , Sabino Matarrese

Moduli fields, which parameterize perturbative flat directions of the potential in supersymmetric theories, are natural candidates to act as inflatons. An inflationary potential on moduli space can result if the scale of dynamical SUSY…

高能物理 - 理论 · 物理学 2009-10-28 Scott Thomas

The most important criteria for a successful inflation are to explain the observed temperature anisotropy in the cosmic microwave background radiation, and exiting inflation in a vacuum where it can excite the Standard Model quarks and…

高能物理 - 理论 · 物理学 2011-05-31 Michele Cicoli , Anupam Mazumdar

An exploratory study of the cosmology of moduli in string theory. Moduli are argued to be natural inflaton fields and lead to a robust inflationary cosmology in which inflation takes place at the top of domain walls. The amplitude of…

高能物理 - 理论 · 物理学 2016-09-06 T. Banks , M. Berkooz , G. Moore , S. H. Shenker , P. J. Steinhardt

We investigate the possibility that a heavy scalar field, whose mass exceeds the Hubble scale during inflation, could leave non-negligible signatures in the Cosmic Microwave Background (CMB) temperature anisotropy power spectrum through the…

宇宙学与河外天体物理 · 物理学 2015-06-05 Ryo Saito , Masahiro Nakashima , Yu-ichi Takamizu , Jun'ichi Yokoyama

Cosmological inflation remains to be a unique mechanism of generation of plausible initial conditions in the early universe. In particular, it generates the primordial quasiclassical perturbations with power spectrum determined by the…

宇宙学与河外天体物理 · 物理学 2010-03-23 Yuri Shtanov

Cosmological inflation is not the only early universe scenario consistent with current observational data. I will discuss the criteria for a successful early universe cosmology, compare a couple of the proposed scenarios (inflation,…

高能物理 - 理论 · 物理学 2019-11-15 Robert Brandenberger

The "central" region of moduli space of M- and string theories is where the string coupling is about unity and the volume of compact dimensions is about the string volume. Here we argue that in this region the non-perturbative potential…

高能物理 - 理论 · 物理学 2009-11-07 R. Brustein , S. P. de Alwis , E. G. Novak

We show that simple strongly coupled supersymmetric gauge theories with quantum moduli spaces can naturally lead to hybrid inflation. These theories contain no input dimensionful or small parameters. The effective superpotential is linear…

高能物理 - 唯象学 · 物理学 2009-10-30 Savas Dimopoulos , Gia Dvali , Riccardo Rattazzi
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