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We develop a theory of turbulence of weak random gravity waves on surface of deep water in which the main nonlinear process at high-frequency part of the spectrum is a nonlocal interaction with a strong low-frequency component. The latter…

流体动力学 · 物理学 2024-09-05 A. O. Korotkevich , S. V. Nazarenko , Y. Pan , J. Shatah

Motivated by some of the recent swampland conjectures, we study a model of dark energy, in which a quintessence axion slowly rolls in a steep potential due to its interactions with a U(1) or an SU(2) gauge field. The gauge fields produced…

宇宙学与河外天体物理 · 物理学 2020-11-13 Alexandros Papageorgiou

The nonlinear turbulent interactions between acoustic gravity waves are investigated using two dimensional nonlinear fluid simulations. The acoustic gravity waves consist of velocity and density perturbations and propagate across the…

大气与海洋物理 · 物理学 2015-05-13 Dastgeer Shaikh , Padma K Shukla , Lennart Stenflo

In theories of supersymmetry breaking, it is often the case that there is more than one metastable vacuum. First-order phase transitions among such metastable vacua may generate a stochastic background of gravitational waves, the…

高能物理 - 唯象学 · 物理学 2009-02-18 Nathaniel J. Craig

We present a new derivation of the kinetic equation for weak, non-hydrostatic internal gravity wave turbulence. The equation is equivalent to the one obtained by Caillol & Zeitlin (2000), but it takes a canonical form. We show that it…

This work investigates the echoes in axial gravitational perturbations in compact objects. To this end, we propose an alternative scheme of the finite difference method implemented in two coordinate systems, where the initial conditions are…

广义相对论与量子宇宙学 · 物理学 2023-09-04 Kai Lin , Wei-Liang Qian

In this work, we consider a general gravitational wave detector of gravitational wave interacting with an incoming gravitational wave carrying plus polarization only placed inside a harmonic trap. This model can be well acquainted with the…

高能物理 - 理论 · 物理学 2024-07-12 Soham Sen , Sunandan Gangopadhyay , Sukanta Bhattacharyya

For low-mass (frequency $\ll$ GHz) axions, dark matter detection experiments searching for an axion-photon-photon coupling generally have suppressed sensitivity, if they use a static background magnetic field. This geometric suppression can…

高能物理 - 唯象学 · 物理学 2020-07-22 Robert Lasenby

Recently Mendonca and Cardoso [Phys. Rev. D, vol. 66, 104009 (2002)] considered nonlinear gravitational wave packets propagating in flat space-time. They concluded that the evolution equation - to third order in amplitude - takes a similar…

天体物理学 · 物理学 2009-11-07 M. Servin , M. Marklund , G. Brodin , J. T. Mendonca , V. Cardoso

We experimentally study nonlinear generation of the second harmonic by backward volume spin waves propagating in microscopic magnonic waveguides fabricated from a low-loss magnetic insulator with a thickness of several tens of nanometers.…

介观与纳米尺度物理 · 物理学 2025-02-27 K. O. Nikolaev , S. R. Lake , B. Das Mohapatra , G. Schmidt , S. O. Demokritov , V. E. Demidov

A self-gravitating cylindrical domain wall is considered as an example of non-spherical wall to clarify the interaction between a domain wall and gravitational waves. We consider the time evolution from a momentarily static initial…

广义相对论与量子宇宙学 · 物理学 2007-05-23 K. Nakamura , H. Ishihara

The combination of non-minimal couplings to gravity with the post-inflationary kinetic-dominated era typically appearing in quintessential inflation scenarios may lead to the spontaneous symmetry breaking of internal symmetries and its…

宇宙学与河外天体物理 · 物理学 2019-02-18 Dario Bettoni , Guillem Domènech , Javier Rubio

The motion of a container filled with fluid perturbs the free surface and may result in spilling. In practice, most of the energy is localized in the modes of lowest frequencies (the gravest modes), and sloshing can be predicted once the…

流体动力学 · 物理学 2019-01-14 Guillaume Michel

Magnetohydrodynamic (MHD) waves are routinely observed in the solar atmosphere. These waves are important in the context of solar physics as it is widely believed they can contribute to the energy budget of the solar atmosphere and are a…

太阳与恒星天体物理 · 物理学 2021-12-22 Samuel Skirvin , Viktor Fedun , Suzana Silva , Gary Verth

We theoretically study the non-linear response of interacting neutral bosonic gas in a synthetically driven one-dimensional optical lattice. In particular, we examine the bosonic analogue of electronic higher harmonic generation in a strong…

量子气体 · 物理学 2021-05-12 Arko Roy , Soumya Bera , Kush Saha

Using a metric perturbation method, we study gravitational waves from a test particle scattered by a spherically symmetric relativistic star. We calculate the energy spectrum and the waveform of gravitational waves for axial modes. Since…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Kazuhiro Tominaga , Motoyuki Saijo , Kei-ichi Maeda

We exploit polarization self-rotation in atomic rubidium vapor to observe spontaneous symmetry breaking and bistability of polarization patterns. We pump the vapor cell with horizontally polarized light while the vertical polarization,…

量子物理 · 物理学 2024-11-26 K. S. Manannikov , E. I. Mironova , A. S. Poliakov , A. Mikhaylov , A. E. Ulanov , A. I. Lvovsky

Gravitational wave observations have significantly broadened our capacity to explore fundamental physics beyond the Standard Model, providing crucial insights into dark matter that are inaccessible through conventional methods. Here, we…

宇宙学与河外天体物理 · 物理学 2025-10-21 Jeong Han Kim , Xing-Yu Yang

We study the gravitational radiation produced by the collisions of bubble walls or thin fluid shells in cosmological phase transitions. Using the so-called envelope approximation, we obtain analytically the asymptotic behavior of the…

宇宙学与河外天体物理 · 物理学 2022-01-05 Ariel Megevand , Agustin Membiela

In the present paper in the assumption of the slowness of variation of the vertically stratified medium parameters in the horizontal direction within the time we have analyzed the evolution of the non-harmonic wave trains of the internal…

流体动力学 · 物理学 2007-05-23 Vitaly V. Bulatov , Yuriy V. Vladimirov