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相关论文: An Analytic Treatment of Underdamped Axionic Blue …

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Large blue tilted spectral index axionic isocurvature perturbations can be produced when the axion sector is far out of equilibrium during inflation through an initial Peccei-Quinn (PQ) symmetry breaking field displacement along a nearly…

宇宙学与河外天体物理 · 物理学 2023-10-02 Daniel J. H. Chung , Sai Chaitanya Tadepalli

Blue axion isocurvature perturbations are both theoretically well-motivated and interesting from a detectability perspective. These power spectra generically have a break from the blue region to a flat region. Previous investigations of the…

宇宙学与河外天体物理 · 物理学 2017-01-11 Daniel J. H. Chung , Amol Upadhye

It is known that if the Peccei-Quinn symmetry breaking field is displaced from its minimum during inflation, the axion isocurvature spectrum is generically strongly blue tilted with a break transition to a flat spectrum. We fit this…

宇宙学与河外天体物理 · 物理学 2018-07-25 Daniel J. H. Chung , Amol Upadhye

CMB limits on cold-dark-matter isocurvature are often interpreted as excluding the simultaneous realization of high-scale inflation and large QCD axion decay constants in pre-inflationary Peccei--Quinn (PQ) scenarios. This conclusion can be…

高能物理 - 唯象学 · 物理学 2026-03-23 Sai Chaitanya Tadepalli

One well known method of generating a large blue spectral index for axionic isocurvature perturbations is through a flat direction not having a quartic potential term for the radial partner of the axion field. In this work, we show how one…

宇宙学与河外天体物理 · 物理学 2024-06-21 Daniel J. H. Chung , Sai Chaitanya Tadepalli

We study adiabatic and isocurvature perturbations produced during a period of cosmological inflation. We compute the power spectra and cross spectra of the curvature and isocurvature modes, as well as the tensor perturbation spectrum in…

天体物理学 · 物理学 2009-11-06 N. Bartolo , S. Matarrese , A. Riotto

We investigate cosmological signatures of uncorrelated isocurvature perturbations whose power spectrum is blue-tilted with spectral index 2<p<4. Such an isocurvature power spectrum can promote early formation of small-scale structure,…

宇宙学与河外天体物理 · 物理学 2015-06-17 Toyokazu Sekiguchi , Hiroyuki Tashiro , Joseph Silk , Naoshi Sugiyama

We show that if a spectator linear isocurvature dark matter field degree of freedom has a constant mass through its entire evolution history, the maximum measurable isocurvature spectral index that is consistent with the current…

宇宙学与河外天体物理 · 物理学 2016-08-31 Daniel J. H. Chung

Blue CDM-photon isocurvature perturbations are attractive in terms of observability and may be typical from the perspective of generic mass relations in supergravity. We present and apply three theorems useful for blue isocurvature…

宇宙学与河外天体物理 · 物理学 2015-04-29 Daniel J. H. Chung , Hojin Yoo

Axions are among the best motivated dark matter candidates. Their production in the early Universe by the vacuum misalignment mechanism gives rise to isocurvature perturbations, which are constrained by cosmic microwave background…

宇宙学与河外天体物理 · 物理学 2021-07-19 Liina Jukko , Arttu Rajantie

We study the problem of passive imaging through convolutive channels. A scene is illuminated with an unknown, unstructured source, and the measured response is the convolution of this source with multiple channel responses, each of which is…

信息论 · 计算机科学 2017-08-25 Kiryung Lee , Felix Krahmer , Justin Romberg

We construct an axion model for generating isocurvature fluctuations with blue spectrum, n_{iso}=2-4, which is suggested by recent analyses of admixture of adiabatic and isocurvature perturbations with independent spectral indices, n_{ad}…

宇宙学与河外天体物理 · 物理学 2009-08-11 Shinta Kasuya , Masahiro Kawasaki

Light scalar fields acquire isocurvature fluctuations during inflation. While these fluctuations could lead to interesting observable signatures at small scales, they are strongly constrained on large scales by cosmic microwave background…

高能物理 - 唯象学 · 物理学 2025-10-15 Saarik Kalia

Consider a linear autonomous Hamiltonian system with a time periodic bound state solution. In this paper we study the structural instability of this bound state ^M relative to time almost periodic perturbations which are small, localized…

斑图形成与孤子 · 物理学 2009-09-25 Eduard Kirr , Michael I. Weinstein

We generalize the treatment of inflationary perturbations to deal with the non-Markovian colored noise emerging from any realistic approach to stochastic inflation. We provide a calculation of the power-spectrum of the gauge-invariant…

天体物理学 · 物理学 2009-11-10 M. Liguori , S. Matarrese , M. Musso , A. Riotto

We revisit the generation of dark matter isocurvature perturbations in the curvaton model in greater detail, both analytically and numerically. As concrete examples, we investigate the cases of thermally decoupled dark matter and axionic…

宇宙学与河外天体物理 · 物理学 2018-01-10 Naoya Kitajima , David Langlois , Tomo Takahashi , Shuichiro Yokoyama

Isocurvature perturbations in the inflationary literature typically involve quantum fluctuations of bosonic field degrees of freedom. In this work, we consider isocurvature perturbations from fermionic quantum fluctuations during inflation.…

宇宙学与河外天体物理 · 物理学 2015-03-05 Daniel J. H. Chung , Hojin Yoo , Peng Zhou

We provide a rigorous derivation of an asymptotic formula for perturbations in the resonance values caused by the presence of finite number of anisotropic imperfections of small shapes with constitutive parameters different from the…

数学物理 · 物理学 2016-02-24 M. Gozzi , A. Khelifi

We study the out of equilibrium dynamics of inflationary phase transitions and compute the resulting spectrum of metric perturbations relevant to observation. We show that simple single field models of inflation may produce an adiabatic…

天体物理学 · 物理学 2016-11-03 D. Cormier , R. Holman

This work presented a perturbational decomposition method for simulating quantum evolution under the one-dimensional Ising model with both longitudinal and transverse fields. By treating the transverse field terms as perturbations in the…

量子物理 · 物理学 2024-12-24 Youning Li , Junfeng Huang , Chao Zhang , Jun Li
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