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We investigate dark matter candidates emerging in recently proposed technicolor theories. We determine the relic density of the lightest, neutral, stable technibaryon having imposed weak thermal equilibrium conditions and overall electric…

高能物理 - 唯象学 · 物理学 2008-11-26 Sven Bjarke Gudnason , Chris Kouvaris , Francesco Sannino

I first outline new results on the angular modulation of WIMP dark matter scattering on targets in terrestrial laboratories, based on our uncertainties of the WIMP halo distribution, I then outline an exciting new result which indicates…

天体物理学 · 物理学 2009-10-30 Lawrence M. Krauss

We apply our recent results on orbital dynamics around a mass-varying central body to the phenomenon of accretion of Dark Matter-assumed not self-annihilating-on the Sun and the major bodies of the solar system due to its motion throughout…

广义相对论与量子宇宙学 · 物理学 2012-07-31 Lorenzo Iorio

We improve, using a larger set of observations including Voyager 2 Neptune flyby data, previous bounds on the amount of dark matter (DM) trapped in a spherically symmetric distribution about the sun. We bound DM by noting that such a…

高能物理 - 唯象学 · 物理学 2016-09-01 John D. Anderson , Eunice L. Lau , Timothy P. Krisher , Duane A. Dicus , Doris C. Rosenbaum , Vigdor L. Teplitz

We calculate the mean density profiles for luminous and dark matter on distance scales $D \sim(1 - 100)$ Mpc around us using recent all-sky catalogs of galaxy groups. Within the Local Volume $( D < 11 ~\rm Mpc)$ we derived the mean stellar…

星系天体物理 · 物理学 2018-12-26 I. D. Karachentsev , K. N. Telikova

The AMS experiment onboard the International Space Station has recently provided cosmic ray electron and positron data with unprecedented precision in the range from 0.5 to 350 GeV. The observed rise in the positron fraction at energies…

高能天体物理现象 · 物理学 2013-10-29 Lars Bergstrom , Torsten Bringmann , Ilias Cholis , Dan Hooper , Christoph Weniger

The criticism contained in the recent preprint arxiv:1004.5258 is based essentially on misquoting the articles criticized therein. As to the conclusion advocated in that preprint, according to which the density of dark matter bound to the…

地球与行星天体物理 · 物理学 2010-05-12 I. B. Khriplovich

While it is possible to estimate the dark matter density at the Sun distance from the galactic center, this does not give information on actual dark matter density in the Solar system. There can be considerable local enhancement of dark…

高能物理 - 唯象学 · 物理学 2024-08-21 Dmitry Budker , Joshua Eby , Marianna S. Safronova , Oleg Tretiak

The dark matter content of the Universe is likely to be a mixture of matter and antimatter, perhaps comparable to the measured asymmetric mixture of baryons and antibaryons. During the early stages of the Universe, the dark matter particles…

太阳与恒星天体物理 · 物理学 2012-09-18 Ilidio Lopes , Joseph Silk

Recently, several papers have appeared that examine the process of capturing dark-matter particles from the Galactic halo to orbits bound to the Solar System. The authors of these papers predict large enhancements to the local dark-matter…

地球与行星天体物理 · 物理学 2015-03-17 Joakim Edsjo , Annika H. G. Peter

One method to search for particle dark matter is to hunt down its annihilation products. In the Solar System, three potential types of signals of annihilation have been identified: neutrinos and gamma-rays from the Sun, and neutrinos from…

高能天体物理现象 · 物理学 2009-05-19 Annika H. G. Peter

For the first time, we have a plausible, complete accounting of matter and energy in the Universe. Expressed a fraction of the critical density it goes like this: neutrinos, between 0.3% and 15%; stars, 0.5%; baryons (total), 5%; matter…

天体物理学 · 物理学 2007-05-23 Michael S. Turner

In the present letter we examine the possibility of constraining dyon black holes based on the available observational data at the scale of the Solar system. For this we consider the classical tests of general relativity, viz., the…

广义相对论与量子宇宙学 · 物理学 2018-11-27 Farook Rahaman , Sabiruddin Molla , Amna Ali , Saibal Ray

If dark matter is efficiently captured by a planet, energy released in its annihilation can exceed that planet's total heat output. Building on prior work, we treat Earth's composition and dark matter capture in detail and present improved…

高能物理 - 唯象学 · 物理学 2020-02-12 Joseph Bramante , Andrew Buchanan , Alan Goodman , Eesha Lodhi

The accumulation of dark matter near the Earth is considered. We analyze the case of long range interaction forces. Additional density of the dark matter at the Earth's surface is calculated. We show that this density exceeds the mean…

核实验 · 物理学 2011-09-16 M. S. Onegin , A. P. Serebrov , O. M. Zherebtsov

For the first time, we have a plausible and complete accounting of matter and energy in the Universe. Expressed a fraction of the critical density it goes like this: neutrinos, between 0.3% and 15%; stars, between 0.3% and 0.6%; baryons…

天体物理学 · 物理学 2009-10-31 Michael S. Turner

The scattering of light dark matter off thermal electrons inside the Sun produces a "fast" sub-component of the dark matter flux that may be detectable in underground experiments. We update and extend previous work by analyzing the…

高能物理 - 唯象学 · 物理学 2023-09-27 Haipeng An , Haoming Nie , Maxim Pospelov , Josef Pradler , Adam Ritz

We investigate the effects of a magnetic dipole moment of asymmetric dark matter (DM) in the evolution of the Sun. The dipole interaction can lead to a sizable DM scattering cross section even for light DM, and the asymmetric dark matter…

太阳与恒星天体物理 · 物理学 2014-02-05 Ilídio Lopes , Kenji Kadota , Joseph Silk

This article reviews recent progress in observational determination of the properties of dark matter on small astrophysical scales, and progress towards the European Extremely Large Telescope. Current results suggest some surprises: the…

天体物理学 · 物理学 2007-05-23 Gerard Gilmore

This paper aims to put constraints on the parameters of the Scalar Field Dark Matter (SFDM) model, when dark matter is described by a free real scalar field filling the whole Universe, plus a cosmological constant term. By using a…

宇宙学与河外天体物理 · 物理学 2022-01-05 A. A. Escobal , J. F. Jesus , S. H. Pereira