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相关论文: Oscillating Spin-2 Dark Matter

200 篇论文

We formulate an effective field theory describing large mass scalars and fermions minimally coupled to gravity. The operators of this effective field theory are organized in powers of the transfer momentum divided by the mass of the matter…

高能物理 - 唯象学 · 物理学 2021-01-29 Poul H. Damgaard , Kays Haddad , Andreas Helset

A pedagogical description of a simple ungeometrical approach to General Relativity is given, which follows the pattern of well understood field theories, such as electrodynamics. This leads quickly to most of the important weak field…

天体物理学 · 物理学 2007-05-23 Norbert Straumann

We present a scenario in which a scalar field dark energy is coupled to the trace of the energy momentum tensor of the baryonic matter fields. In the slow-roll regime, this interaction could give rise to the cosmological features of dark…

宇宙学与河外天体物理 · 物理学 2011-02-02 Alejandro Aviles , Jorge L. Cervantes-Cota

Low-mass (sub-eV) spin-0 dark matter particles, which form a coherently oscillating classical field $\phi = \phi_0 \cos(m_\phi t)$, can induce oscillating variations in the fundamental constants through their interactions with the Standard…

原子物理 · 物理学 2016-08-24 Y. V. Stadnik , V. V. Flambaum

The stability of dark matter is normally achieved by imposing extra symmetries beyond those of the Standard Model of Particle Physics. In this paper we present a framework where the dark matter stability emerges as a consequence of the…

高能物理 - 唯象学 · 物理学 2014-09-17 Oscar Cata , Alejandro Ibarra

As a consequence of gravitomagnetism, which is a fundamental weak-field prediction of general relativity and ubiquitous in gravitational phenomena, clocks show a difference in their proper periods when moving along identical orbits in…

广义相对论与量子宇宙学 · 物理学 2007-05-23 H. Lichtenegger , W. Hausleitner , F. Gronwald , B. Mashhoon

We propose and study a new minimal model for two-component dark matter. The model contains only three additional fields, one fermion and two scalars, all singlets under the Standard Model gauge group. Two of these fields, one fermion and…

高能物理 - 唯象学 · 物理学 2015-06-19 Sonja Esch , Michael Klasen , Carlos E. Yaguna

The equations of electrodynamics are altered in the presence of a classical coherent axion dark matter background field, changing the dispersion relation for electromagnetic waves. Careful measurements of the frequency stability in…

高能物理 - 唯象学 · 物理学 2019-05-30 Lawrence M. Krauss

We show that gravitational wave detectors based on a type of atom interferometry are sensitive to ultralight scalar dark matter. Such dark matter can cause temporal oscillations in fundamental constants with a frequency set by the dark…

高能物理 - 唯象学 · 物理学 2018-04-25 Asimina Arvanitaki , Peter W. Graham , Jason M. Hogan , Surjeet Rajendran , Ken Van Tilburg

Two-dimensional quantum fields in electric and gravitational backgrounds can be described by conformal field theories, and hence all the physical (covariant) quantities can be written in terms of the corresponding holomorphic quantities. In…

高能物理 - 理论 · 物理学 2008-11-26 Satoshi Iso , Takeshi Morita , Hiroshi Umetsu

There is a non-trivial four-derivative extension of the gravitational spectrum that is free of ghosts and phenomenologically viable. It is the so called $R^2$-gravity since it is defined by the only addition of a term proportional to the…

广义相对论与量子宇宙学 · 物理学 2011-08-25 Jose A. R. Cembranos

In this paper, we investigate a two dimensional isotropic harmonic oscillator on a time-dependent spherical background. The effect of the background can be represented as a minimally coupled field to the oscillator's Hamiltonian. For a…

量子物理 · 物理学 2015-06-11 Ali Mahdifar , Behrouz Mirza , Rasoul Roknizadeh

We resolve subtleties in calculating the post-Minksowskian dynamics of binary systems, as a spin expansion, from massive scattering amplitudes of fixed finite spin. In particular, the apparently ambiguous spin Casimir terms can be fully…

高能物理 - 理论 · 物理学 2025-04-04 Dogan Akpinar , Fernando Febres Cordero , Manfred Kraus , Michael S. Ruf , Mao Zeng

We study the ultralight axion dark matter with mass around $10^{-22}$ eV in $f(R)$ gravity which might resolve the dark energy problem. In particular, we focus on the fact that the pressure of the axion field oscillating in time produces…

宇宙学与河外天体物理 · 物理学 2017-07-28 Arata Aoki , Jiro Soda

We place model-independent constraints on theories of massive spin-2 particles by considering the positivity of the phase shift in eikonal scattering. The phase shift is an asymptotic $S$-matrix observable, related to the time delay/advance…

高能物理 - 理论 · 物理学 2018-03-16 Kurt Hinterbichler , Austin Joyce , Rachel A. Rosen

We launch a first investigation into how a light scalar field coupled both conformally and disformally to matter influences the evolution of spinning point-like bodies. Working directly at the level of the equations of motion, we derive…

广义相对论与量子宇宙学 · 物理学 2021-03-09 Philippe Brax , Anne-Christine Davis , Scott Melville , Leong Khim Wong

Fermionic alkaline-earth atoms have unique properties that make them attractive candidates for the realization of novel atomic clocks and degenerate quantum gases. At the same time, they are attracting considerable theoretical attention in…

量子气体 · 物理学 2010-04-20 A. V. Gorshkov , M. Hermele , V. Gurarie , C. Xu , P. S. Julienne , J. Ye , P. Zoller , E. Demler , M. D. Lukin , A. M. Rey

It is widely believed that axions are ubiquitous in string theory and could be the dark matter. The peculiar features of the axion dark matter are coherent oscillations and a coupling to the electromagnetic field through the Chern-Simons…

高能物理 - 理论 · 物理学 2018-04-24 Daiske Yoshida , Jiro Soda

We clarify the properties of the behavior of classical cosmological perturbations when the Universe experiences a bounce. This is done in the simplest possible case for which gravity is described by general relativity and the matter content…

高能物理 - 理论 · 物理学 2009-11-10 Jerome Martin , Patrick Peter

We show that if the masses of timelike fields are point-dependent quantities transforming under conformal transformations as $m\rightarrow\Omega^{-1}m$, so the energy density of perfect fluids transforms as $\rho\rightarrow\Omega^{-4}\rho$,…

广义相对论与量子宇宙学 · 物理学 2026-04-20 Israel Quiros