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相关论文: Bayesian Analysis of Inflation: Parameter Estimati…

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In this paper we will analyze generic predictions of an inflection-point model of inflation with Hubble-induced corrections and study them in light of the Planck data. Typically inflection-point models of inflation can be embedded within…

高能物理 - 唯象学 · 物理学 2013-07-29 Sayantan Choudhury , Anupam Mazumdar , Supratik Pal

We investigate the impact of different choice of prior's range for the reheating epoch on cosmic inflation parameter inference in light of cosmic microwave background (CMB) anisotropy measurements from the {\em Planck} 2018 legacy release…

宇宙学与河外天体物理 · 物理学 2025-01-30 Mario Ballardini

A class of inflationary models that involve rapid bursts of particle productions predict observational signatures, such as bump-like features in the primordial scalar power spectrum. In this work, we analyze such models by comparing their…

宇宙学与河外天体物理 · 物理学 2023-06-07 Suvedha Suresh Naik , Kazuyuki Furuuchi , Pravabati Chingangbam

We investigate constraints on power spectra of the primordial curvature and tensor perturbations with priors based on single-field slow-roll inflation models. We stochastically draw the Hubble slow-roll parameters and generate the…

宇宙学与河外天体物理 · 物理学 2014-11-20 Masahiro Kawasaki , Toyokazu Sekiguchi

We present and discuss a new approach increasing by orders of magnitude the speed of performing Bayesian inference and parameter estimation within the framework of slow-roll inflation. The method relies on the determination of an effective…

宇宙学与河外天体物理 · 物理学 2014-06-03 Christophe Ringeval

We confront the warm inflation observational predictions directly with the latest CMB data. We focus on a linear temperature (T) dissipative coefficient combined with the simplest model of inflation, a quartic chaotic potential. Although…

宇宙学与河外天体物理 · 物理学 2018-03-06 Mar Bastero-Gil , Sukannya Bhattacharya , Koushik Dutta , Mayukh Raj Gangopadhyay

Bayesian model comparison penalizes models with more free parameters that are allowed to vary over a wide range, and thus offers the most robust method to decide whether some given data require new parameters. In this paper, we ask a simple…

宇宙学与河外天体物理 · 物理学 2015-07-28 Tommaso Giannantonio , Eiichiro Komatsu

We exploit a new numerical technique for evaluating the tree order contributions to the primordial scalar and tensor power spectra for scalar potential models of inflation. Among other things we use the formalism to develop a good analytic…

宇宙学与河外天体物理 · 物理学 2017-09-06 D. J. Brooker , N. C. Tsamis , R. P. Woodard

With an energy scale that can be as high as $10^{14}\,{\rm GeV}$, inflation may provide a unique probe of high-energy physics. Both scalar and tensor fluctuations generated during this early accelerated expansion contain crucial information…

宇宙学与河外天体物理 · 物理学 2020-08-25 Laura Iacconi , Matteo Fasiello , Hooshyar Assadullahi , Emanuela Dimastrogiovanni , David Wands

In this paper, we undertake a detailed study of real scalar inflation by employing LATTICEEASY simulations to investigate preheating phenomena. Generally, the scalar inflation potential with non-minimal coupling can be approximated by a…

宇宙学与河外天体物理 · 物理学 2024-03-15 Wei Cheng , Tong Qin , Jiujiang Jiang , Ruiyu Zhou

We discuss whether an unaccounted contribution to the Cosmic Microwave Background polarization $B$-mode by primordial magnetic fields (PMFs) can bias future constraints on inflationary gravitational waves. As a case-study, we consider a…

宇宙学与河外天体物理 · 物理学 2018-09-05 Fabrizio Renzi , Giovanni Cabass , Eleonora Di Valentino , Alessandro Melchiorri , Luca Pagano

In the lights of current BICEP2 observations accompanied with the PLANCK satellite results, it has been observed that the simple single field chaotic inflationary models provide a good agreement with their spectral index n_s and large…

高能物理 - 唯象学 · 物理学 2014-10-20 Xin Gao , Tianjun Li , Pramod Shukla

Standard Clocks in the primordial epoch leave a special type of features in the primordial perturbations, which can be used to directly measure the scale factor of the primordial universe as a function of time a(t), thus discriminating…

宇宙学与河外天体物理 · 物理学 2015-06-19 Xingang Chen , Mohammad Hossein Namjoo

We construct models of inflation with many randomly interacting fields and use these to study the generation of cosmological observables. We model the potentials as multi-dimensional Gaussian random fields (GRFs) and identify powerful…

宇宙学与河外天体物理 · 物理学 2018-02-28 Theodor Bjorkmo , M. C. David Marsh

Recent measurements by the {\it Planck} experiment of the power spectrum of temperature anisotropies in the cosmic microwave background radiation (CMB) reveal a deficit of power in low multipoles compared to the predictions from best-fit…

宇宙学与河外天体物理 · 物理学 2014-03-19 Katelin Schutz , Evangelos I. Sfakianakis , David I. Kaiser

We study the implications of the recently proposed Trans-Planckian Censorship Conjecture (TCC) for early universe cosmology and in particular inflationary cosmology. The TCC leads to the conclusion that if we want inflationary cosmology to…

高能物理 - 理论 · 物理学 2020-05-06 Alek Bedroya , Robert Brandenberger , Marilena Loverde , Cumrun Vafa

A new family of inflationary models is introduced and analysed. The behaviour of the parameters characterising the models suggest preferred values, which generate the most interesting testable predictions. Results are further improved if…

高能物理 - 唯象学 · 物理学 2016-09-20 Konstantinos Dimopoulos , Charlotte Owen

The current flow of high accuracy astrophysical data, among which are the Cosmic Microwave Background (CMB) measurements by the Planck satellite, offers an unprecedented opportunity to constrain the inflationary theory. This is however a…

宇宙学与河外天体物理 · 物理学 2024-12-20 Jerome Martin , Christophe Ringeval , Vincent Vennin

The spectrum of primordial fluctuations from inflation can be obtained using a mathematically controlled, and systematically extendable, uniform approximation. Closed-form expressions for power spectra and spectral indices may be found…

天体物理学 · 物理学 2008-11-26 Salman Habib , Andreas Heinen , Katrin Heitmann , Gerard Jungman , Carmen Molina-Paris

Modern cosmological data demand modern data analysis techniques. We introduce BayOp, a new likelihood sampling and maximisation method which is based on the Bayesian Optimisation algorithm and learns a function instead of randomly sampling…

宇宙学与河外天体物理 · 物理学 2022-04-15 Jan Hamann , Julius Wons