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相关论文: Higher order corrections to Heterotic M-theory inf…

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Motivated by trans-Planckian issues in inflation, we determine the Hilbert space and amplitudes of quantum perturbations in the general low-energy effective theory of (multi-)field inflation without relying on the sub-horizon limit. The…

高能物理 - 理论 · 物理学 2026-05-29 Andrea Ambrosi de Magistris , Alberto Salvio

We study the phase space of initial conditions for brane inflation, and find that including the effects of the Dirac-Born-Infeld (DBI) kinetic term dramatically improves previous estimates on the amount of fine tuning of initial conditions…

高能物理 - 理论 · 物理学 2008-12-18 Bret Underwood

A class of non-canonical inflationary models is identified, where the leading-order contribution to the non-Gaussianity of the curvature perturbation is determined by the sound speed of the fluctuations in the inflaton field. Included in…

高能物理 - 理论 · 物理学 2008-11-26 Ian Huston , James E. Lidsey , Steven Thomas , John Ward

During inflation, higher derivative terms in the gravitational action may play a significant role. Building on new stable formulations of four-derivative scalar-tensor theories, we study the impact of these corrections in the case where the…

广义相对论与量子宇宙学 · 物理学 2025-05-26 Sam E. Brady , Katy Clough , Pau Figueras , Áron D. Kovács

If the recent measurement of B-mode polarization by BICEP2 is due to primordial gravitational waves, it implies that inflation was driven by energy densities at the GUT scale $M_{GUT} \sim 2\times 10^{16} GeV$. This favors single-field…

高能物理 - 理论 · 物理学 2014-07-09 Nemanja Kaloper , Albion Lawrence

It was pointed out that brane-anti-brane inflation without warped geometry is not viable due to compactification effects (in the simplified scenario where the inflaton is decoupled from the compactification moduli). We show that the…

高能物理 - 理论 · 物理学 2009-11-10 Sarah Shandera , Benjamin Shlaer , Horace Stoica , S. -H. Henry Tye

We study the evolution of scalar curvature perturbations in a brane-world inflation model in a 5D Anti-de Sitter spacetime. The inflaton perturbations are confined to a 4D brane but they are coupled to the 5D bulk metric perturbations. We…

高能物理 - 理论 · 物理学 2009-02-05 Takashi Hiramatsu , Kazuya Koyama

We propose that under certain conditions the universal open string tachyon can drive topological inflation in moduli stabilised frameworks. Namely, the presence of electric field in the world volume of the D-brane can slow down its decay…

高能物理 - 理论 · 物理学 2009-11-11 Daniel Cremades

We present a new approximation scheme that allows us to increase the accuracy of analytical predictions of the power spectra of inflationary perturbations for two specific classes of inflationary models. Among these models are chaotic…

天体物理学 · 物理学 2015-06-24 C. A. Terrero-Escalante , D. J. Schwarz , A. A. Garcia

The scenario of brane inflation without using the conventional slow-roll approximations has been investigated. Based on the mechanism of generating the curvature perturbations at the end of inflation, a new brane inflation paradigm was…

天体物理学 · 物理学 2010-10-27 Tomohiro Matsuda

We discuss a brane based inflationary scenario in which an initially non-supersymmetric configuration involving a D4 brane is dynamically transformed into a supersymmteric one in a background space-time geometry determined by a stack of D6…

高能物理 - 唯象学 · 物理学 2011-05-12 Bumseok Kyae , Qaisar Shafi

We argue that brane anti-brane inflation in string theory de-Sitter vacua of Kachru-Kallosh-Linde-Trivedi (KKLT) is captured by the dynamics of a D3-brane probe in the local KKLT model constructed in hep-th/0203041. This provides a…

高能物理 - 理论 · 物理学 2010-04-05 Alex Buchel , Radu Roiban

We analyze the Randal Sundrum brane-world inflation scenario in the context of the latest CMB constraints from Planck. We summarize constraints on the most popular classes of models and explore some more realistic inflaton effective…

宇宙学与河外天体物理 · 物理学 2018-03-19 Mayukh R. Gangopadhyay , Grant J. Mathews

We consider the brane gas picture of the early universe. At later stages, when there are no winding modes and the background is free to expand, we show that a moving 3-brane, which we identify with our universe, can inflate even though it…

高能物理 - 唯象学 · 物理学 2009-11-07 M. F. Parry , D. A. Steer

I review some aspects of obtaining inflation from string theory, in particular brane-antibrane inflation within the framework of KKLMMT, and racetrack inflation. Further, I discuss recent work on the problem of reheating after…

高能物理 - 理论 · 物理学 2007-05-23 James M. Cline

The constraint of trans-Planckian censorship conjecture on brane inflation model is considered. The conjectures put an upper bound on the main parameter including temperature, inflation time, potential, and the tensor-to-scalar ratio…

高能物理 - 理论 · 物理学 2021-12-15 Abolhassan Mohammadi , Tayeb Golanbari , Jamil Enayati

We derive an $\alpha=1/3$ - attractor potential of slow-roll inflation in the geometric set-up of three intersecting $D7$ branes under $T^6/Z_N$ type of $CY_3$-compactification within type IIB/F theory with some near-conifold regions. The…

高能物理 - 理论 · 物理学 2024-05-01 Arunoday Sarkar , Buddhadeb Ghosh

We present a novel inflationary scenario in theories with low scale (TeV) quantum gravity, in which the standard model particles are localized on the branes whereas gravity propagates in the bulk of large extra dimensions. This inflationary…

高能物理 - 唯象学 · 物理学 2009-10-31 Gia Dvali , S. -H. Henry Tye

We extend the Randall-Sundrum(RS) model by adding a fundamental scalar field in the bulk, then study the multi-field assisted inflationary solution on brane. We will show that this model satisfies not only the observation, but also provides…

高能物理 - 唯象学 · 物理学 2019-08-17 Yun_Song Piao , Wenbin Lin , Xinmin Zhang , Yuan-Zhong Zhang

We propose a chaotic inflation model in which the lightest right-handed sneutrino serves as the inflaton and the predicted values of the spectral index and tensor-to-scalar ratio are consistent with the Planck data. Interestingly, the…

高能物理 - 唯象学 · 物理学 2014-01-28 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida
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