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相关论文: Relic gravitons and non-stationary processes

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A large population of binary systems in the Universe emitting gravitational waves (GW) would produce a stochastic noise, known as the gravitational wave background (GWB). The properties of the GWB directly depend on the attributes of its…

广义相对论与量子宇宙学 · 物理学 2024-12-04 Mikel Falxa , Hippolyte Quelquejay Leclere , Alberto Sesana

We investigate a generic source of stochastic gravitational wave background due to the parametric resonance of oscillating scalar fields in the early Universe. By systematically analyzing benchmark models through lattice simulations and…

高能物理 - 唯象学 · 物理学 2024-07-19 Yanou Cui , Pankaj Saha , Evangelos I. Sfakianakis

We calculate the spectrum of the relic gravitational wave due to the trans-Planckian effect in which the standard linear dispersion relations may be modified. Of the modified dispersion relations suggested in literatures which have…

高能物理 - 理论 · 物理学 2011-03-28 Seoktae Koh

If the refractive index of the tensor modes increases during a conventional inflationary stage of expansion the relic graviton spectrum is tilted towards high frequencies. Two apparently diverse parametrizations of this effect are shown to…

广义相对论与量子宇宙学 · 物理学 2018-07-04 Massimo Giovannini

In weakly nonlinear dispersive wave systems, long-time dynamics are typically governed by time resonances, where wave phases evolve coherently due to exact frequency matching. Recent advances in spatio-temporal spectrum measurements,…

斑图形成与孤子 · 物理学 2025-12-09 Michal Shavit , Fabio Pusateri , Zhou Zhang , Yulin Pan , Davide Maestrini , Miguel Onorato , Jalal Shatah

We argue that in at least a portion of the history of the universe the relic background neutrinos are spatially-extended, coherent superpositions of mass states. We show that an appropriate quantum mechanical treatment affects the neutrino…

天体物理学 · 物理学 2010-04-30 George M. Fuller , Chad T. Kishimoto

I report recent studies on the evolution of perturbations in the context of the ``pre-big-bang" scenario typical of string cosmology, with emphasis on the formation of a stochastic background of relic photons and gravitons, and its possible…

高能物理 - 理论 · 物理学 2009-09-25 M. Gasperini

The frequencies of quasi-periodic oscillations around neutron stars are believed to be related to characteristic frequencies in the gravitational fields of the compact objects. In different variability models, these include the Keplerian,…

天体物理学 · 物理学 2007-05-23 Simon DeDeo , Dimitrios Psaltis

Physical scenarios, leading to highly energetic stochastic gravitational waves backgrounds (for frequencies ranging from the $\mu$Hz up to the GHz) are examined. In some cases the typical amplitude of the logarithmic energy spectrum can be…

高能物理 - 唯象学 · 物理学 2016-11-03 Massimo Giovannini

The review is devoted to consideration of possible observational consequences of modified gravity theories, suggested for explanation of the contemporary accelerated expansion of the universe. The major attention is paid to F(R)-models. It…

广义相对论与量子宇宙学 · 物理学 2019-11-11 Elena Arbuzova

Primordial gravitational waves propagate almost unimpeded from the moment they are generated to the present epoch. Nevertheless, they are subject to convolution with a non-trivial transfer function. Within the standard thermal history,…

宇宙学与河外天体物理 · 物理学 2025-06-02 Annet Konings , Mariia Marinichenko , Oleksii Mikulenko , Subodh P. Patil

We study the classical radiation emitted by free-falling charges in de Sitter spacetime coupled to different kinds of fields. Specifically we consider the cases of the electromagnetic field, linearized gravity and scalar fields with…

广义相对论与量子宇宙学 · 物理学 2010-10-11 E. T. Akhmedov , Albert Roura , A. Sadofyev

We review recent developments on quantum scattering from mesoscopic systems. Various spatial geometries whose closed analogs shows diffusive, localized or critical behavior are considered. These are features that cannot be described by the…

无序系统与神经网络 · 物理学 2009-11-11 Tsampikos Kottos

We investigate the dynamics of gravity coupled to a scalar field using a non-canonical form of the kinetic term. It is shown that its singular point represents an attractor for classical solutions and the stationary value of the field may…

高能物理 - 理论 · 物理学 2015-06-26 H. Kroger , G. Melkonyan , F. Paradis , S. G. Rubin

We consider the framework of quintessential inflation in the warm background which is caused by the dissipation of the scalar field energy density into relativistic degrees of freedom. The dissipation process has important consequences for…

宇宙学与河外天体物理 · 物理学 2021-03-03 Mayukh R. Gangopadhyay , Shynaray Myrzakul , Mohammad Sami , Mohit K. Sharma

Real scalar fields, e.g. the axion, cannot condensate into stationary solitonic configurations to form star-like structures, eventually either dispersing or collapsing. However, by relaxing the stationarity condition on the metric, it has…

广义相对论与量子宇宙学 · 物理学 2026-01-01 Nicolas Aimar , Caio F. B. Macedo , João Luís Rosa , Diego Rubiera-Garcia

We make rigorous spectral stability analysis for non-resonant capillary-gravity waves as well as resonant Wilton ripples of sufficiently small amplitude. Our analysis is based on a periodic Evans function approach, developed recently by the…

偏微分方程分析 · 数学 2026-05-13 Vera Mikyoung Hur , Zhao Yang

Quasi-periodic oscillations (QPOs) are an important key to understand the dynamic behavior of astrophysical objects during transient events like gamma-ray bursts, solar flares, and magnetar flares. Searches for QPOs often use the…

高能天体物理现象 · 物理学 2022-03-30 Moritz Huebner , Daniela Huppenkothen , Paul D. Lasky , Andrew R. Inglis

The coherence of the relic gravitons is investigated within a quantum mechanical perspective. After introducing the notion and the properties of the generalized Glauber correlators valid in the tensor case, the degrees of first- and…

高能物理 - 理论 · 物理学 2019-06-19 Massimo Giovannini

We estimate the spectral properties of the stochastic background of gravitational radiation emitted by a cosmological population of hot, young, rapidly rotating neutron stars. Their formation rate as a function of redshift is deduced from…

天体物理学 · 物理学 2009-10-30 Valeria Ferrari , Sabino Matarrese , Raffaella Schneider