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The known direction of motion of dark matter particles relative to the Earth may be a key for their unambiguous identification even in the presence of backgrounds. We describe a prototype detector that is able to reconstruct direction…

It is a well-known fact that the gravitational effect of dark matter in galaxies is only noticeable when the orbital accelerations drop below $a_0 \simeq 2\times 10^{-8}$ cm s$^{-1}$ (Milgrom's Law). This peculiarity of the dynamic…

Cosmology and Nongalactic Astrophysics · Physics 2011-11-08 L. Acedo

The dark matter density distribution in small-scale astrophysical objects may indicate that dark matter is self-interacting, while observations from clusters of galaxies suggest that the corresponding cross section depends on the velocity.…

High Energy Physics - Phenomenology · Physics 2019-02-27 Xiaoyong Chu , Camilo Garcia-Cely , Hitoshi Murayama

Evidence of fast variations in the Earth's core field are seen both in magnetic observatory and satellite records. We present here how they have been identified at the Earth's surface from ground-based observatory records and how their…

Geophysics · Physics 2022-01-17 V. Lesur , N. Gillet , M. D. Hammer , M. Mandea

A small admixture of dark matter gravitationally bound to the proto-Solar gas cloud could be adiabatically contracted into Earth-crossing orbits with a local density comparable to (or even exceeding) the Galactic halo density. We show that…

High Energy Physics - Phenomenology · Physics 2020-07-23 Noah B. Anderson , Angelina Partenheimer , Timothy D. Wiser

We present for the first time hourly variations of the spatial density gradient of 50 GeV cosmic rays within a sample solar rotation period in 2006. By inversely solving the transport equation, including diffusion, we deduce the gradient…

To gain a better understanding of the surfaces of planets and small bodies in the solar system, the flow behavior of granular material for various gravity levels is of utmost interest. We performed a set of reduced-gravity measurements to…

Earth and Planetary Astrophysics · Physics 2009-07-22 Paul G. Hofmeister , Jürgen Blum , Daniel Heißelmann

The climate and circulation of a terrestrial planet are governed by, among other things, the distance to its host star, its size, rotation rate, obliquity, atmospheric composition and gravity. Here we explore the effects of the last of…

Earth and Planetary Astrophysics · Physics 2019-08-21 Stephen I. Thomson , Geoffrey K. Vallis

We study the effect of the scattering of gravitational waves on planetary motions, say the motion of the Moon around the Earth. Though this effect has a negligible influence on dissipation, it dominates fluctuations and the associated…

Quantum Physics · Physics 2009-11-07 Serge Reynaud , Paulo A. Maia Neto , Astrid Lambrecht , Marc-Thierry Jaekel

We calculate the ``seeing'' effect on distant sources due to a gravitational wave background. We derive the limit in strain and energy density of the gravitational wave based on the limit of detectability of this effect with the present day…

Astrophysics · Physics 2007-05-23 Francine Marleau , Glenn Starkman

As known from Einstein's theory of general relativity, the propagation of light in the presence of a massive object is affected by gravity. In this work, we discuss whether the effect of gravitational light bending can be observed in…

General Relativity and Quantum Cosmology · Physics 2020-07-13 Sebastian Ulbricht , Johannes Dickmann , Robert A. Müller , Stefanie Kroker , Andrey Surzhykov

The evidence for the existence of dark matter (DM) is compelling, yet its nature remains elusive. A minimal scenario involves DM interacting solely through gravity. However, the detection would be extremely challenging. In the early…

High Energy Physics - Phenomenology · Physics 2025-04-22 Yong Xu

If dark matter interacts too strongly with nuclei, it could be slowed to undetectable speeds in Earth's crust or atmosphere before ever reaching a detector. For sub-GeV dark matter, analytic approximations appropriate for heavier dark…

High Energy Physics - Phenomenology · Physics 2023-08-30 Christopher Cappiello

A sample of 11 thousand galaxies with radial velocities V_ LG < 3500 km/s is used to study the features of the local distribution of luminous (stellar) and dark matter within a sphere of radius of around 50 Mpc around us. The average…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 I. D. Karachentsev

GravityCam is a new concept of ground-based imaging instrument capable of delivering significantly sharper images from the ground than is normally possible without adaptive optics. Advances in optical and near infrared imaging technologies…

If there is a fifth force in the dark sector and dark sector particles interact non-gravitationally with ordinary matter, quantum corrections generically lead to a fifth force in the visible sector. We show how the strong experimental…

High Energy Physics - Phenomenology · Physics 2009-04-08 Jo Bovy , Glennys R. Farrar

We investigate the effects of dark matter annihilation on objects with masses close to the sub-stellar limit, finding that the minimum mass for stable hydrogen burning is larger than the $\sim0.075 M_\odot $ value predicted in the Standard…

High Energy Physics - Phenomenology · Physics 2025-09-09 Djuna Croon , Jeremy Sakstein , Juri Smirnov , Jack Streeter

It is shown that quantum aspects of the energy-momentum tensor reveal dark matter and dark energy behavior for general relativity. Special meaning is assigned to the operator X^2d^2/dX^2 +2Xd/dX, for any field X that is part of the…

General Physics · Physics 2010-01-01 M. Spaans

Radiative, gravitational surface waves are investigated at the interface of high density and low temperature, magnetized incompressible electron-ion plasmas in the presence of dense radiation electromagnetic radiation pressure (DEMRP). The…

Plasma Physics · Physics 2023-11-28 A. Asma , Ch. Rozina , I. Zafar , S. Poedts

We extract at redshift z=0 a Milky Way sized object including gas, stars and dark matter (DM) from a recent, high-resolution cosmological N-body simulation with baryons. Its resolution is sufficient to witness the formation of a rotating…

Astrophysics of Galaxies · Physics 2014-11-20 F. -S. Ling , E. Nezri , E. Athanassoula , R. Teyssier