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相关论文: Note about leptogenesis from gravity waves in mode…

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We show that the scalar-tensor $\sigma$-model action is conformally equivalent to general relativity with a minimally coupled wavemap with a particular target metric. Inflation on the source manifold is then shown to occur in a natural way…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Spiros Cotsakis , John Miritzis

We show that both the baryon asymmetry of the Universe and the dark matter abundance can be explained within a single framework that makes use of maximally helical hypermagnetic fields produced during pseudoscalar inflation and the chiral…

高能物理 - 唯象学 · 物理学 2019-10-10 Yann Cado , Eray Sabancilar

We study Affleck-Dine leptogenesis via the L H_u flat direction in supersymmetric theories. We find that the baryon asymmetry is enhanced when the energy scale of the inflation is sufficiently low. Especially, we consider models of low…

高能物理 - 唯象学 · 物理学 2009-11-07 T. Asaka

Whichever could be the real theory of gravitation, the corresponding low-energy effective lagrangian will probably contain higher derivative terms. In this work we study the general conditions on those terms in order to produce enough…

高能物理 - 唯象学 · 物理学 2014-11-17 A. Dobado , A. Lopez

We argue that the Higgs boson of the Standard Model can lead to inflation and produce cosmological perturbations in accordance with observations. An essential requirement is the non-minimal coupling of the Higgs scalar field to gravity; no…

高能物理 - 理论 · 物理学 2008-11-26 F. L. Bezrukov , M. E. Shaposhnikov

In standard inflationary cosmology, scalar and tensor perturbations grew as the Universe expanded and froze when their wavelengths exceeded the Hubble horizon, producing a tell-tale signature in the fluctuation spectrum and amplitude of the…

广义相对论与量子宇宙学 · 物理学 2023-07-21 Fulvio Melia

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 show that an inflationary background might be realized by using any p-form non-minimally coupled to gravity. Standard scalar field inflation corresponds to the 0-form case and vector inflation to the 1-form. Moreover, we show that the 2-…

宇宙学与河外天体物理 · 物理学 2009-11-13 Cristiano Germani , Alex Kehagias

In a recent paper, which has been published in Nature, the LIGO Scientific Collaboration (LSC) obtained an upper limit on the stochastic gravitational-wave background of cosmological origin by using the data from a two-year science run of…

广义相对论与量子宇宙学 · 物理学 2015-05-19 Christian Corda

In this article we discuss the role of current and future CMB measurements in pinning down the model of inflation responsible for the generation of primordial curvature perturbations. By considering a parameterization of the effective field…

高能物理 - 理论 · 物理学 2014-10-03 Rhiannon Gwyn , Gonzalo A. Palma , Mairi Sakellariadou , Spyros Sypsas

In a previous work, a mechanism was presented by which baryon asymmetry can be generated during inflation from elliptically polarized gravitons. Nonetheless, the mechanism only generated a realistic baryon asymmetry under special…

高能物理 - 理论 · 物理学 2009-11-10 Stephon H. S. Alexander , S. James Gates

The shortcomings of the Standard Big Bang Cosmological Model as well as their resolution in the context of inflationary cosmology are discussed. The inflationary scenario and the subsequent oscillation and decay of the inflaton field are…

高能物理 - 唯象学 · 物理学 2007-05-23 G. Lazarides

If inflation was preceded by a radiation era then at the time of inflation there will exist a decoupled thermal distribution of gravitons. Gravitational waves generated during inflation will be amplified by the process of stimulated…

天体物理学 · 物理学 2008-11-26 Kaushik Bhattacharya , Subhendra Mohanty , Akhilesh Nautiyal

We review the recent attempts of unifying inflation with quintessence. It appears natural to join the two ends in the framework of brane world cosmology. The models of quintessential inflation belong to the class of {\it non-oscillatory}…

高能物理 - 理论 · 物理学 2007-05-23 M. Sami , N. Dadhich

The detection of a stochastic background of long-wavelength gravitational waves (tensors) in the cosmic microwave background (CMB) anisotropy would be an invaluable probe of the high energy physics of the early universe. Unfortunately a…

天体物理学 · 物理学 2007-05-23 J. P. Zibin , Douglas Scott , Martin White

In single-field, slow-roll inflationary models, scalar and tensorial (Gaussian) perturbations are both characterized by a zero mean and a non-zero variance. In position space, the corresponding variance of those fields diverges in the…

广义相对论与量子宇宙学 · 物理学 2014-11-20 I. Agullo , J. Navarro-Salas , Gonzalo J. Olmo , Leonard Parker

We propose a novel and minimal setup where the observed baryon asymmetry of the Universe and neutrino oscillation data can be satisfied with only one right-handed neutrino (RHN) and a second Higgs doublet with the latter being also…

高能物理 - 唯象学 · 物理学 2026-04-22 Disha Bandyopadhyay , Debasish Borah , Suruj Jyoti Das , Nobuchika Okada

Anisotropies in the cosmic microwave background radiation due to gravity waves are investigated. An initial spectrum of gravity waves may have been induced during an epoch of inflation. We study the propagation of such a spectrum in a…

天体物理学 · 物理学 2008-02-03 Ruth Durrer , Tina Kahniashvili

We further analyze phenomenological implications of double axion monodromy inflation proposed in Ref. Phys. Rev. D 104, L081302 (2021), in gravitational wave physics. We show that in addition to chiral gravitational waves (GW) originating…

广义相对论与量子宇宙学 · 物理学 2022-11-22 Medeu Abishev , Aigerim Abylayeva , Andrea Addazi , Yermek Aldabergenov , Daulet Berkimbayev

We study inflation in a recently proposed gravitational effective field theory describing the trace anomaly. The theory requires an additional scalar which is massless in the early universe. This scalar -- referenced as an anomalyon --…

高能物理 - 理论 · 物理学 2025-03-17 Gregory Gabadadze , David N. Spergel , Giorgi Tukhashvili
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