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A dark matter overdensity around a black hole may significantly alter the dynamics of the black hole's merger with another compact object. We consider here intermediate mass-ratio inspirals of stellar-mass compact objects with…

广义相对论与量子宇宙学 · 物理学 2021-12-23 Bradley J. Kavanagh , David A. Nichols , Gianfranco Bertone , Daniele Gaggero

A regular rotating MOG (modified gravity) compact object is derived that reduces to the Kerr black hole when the parameter $\alpha=0$. Physical consequences of the dark compact object, which is regular everywhere in spacetime for $\alpha >…

广义相对论与量子宇宙学 · 物理学 2021-02-15 J. W. Moffat

One of the abiding mysteries in the so-called standard cosmological model is the nature of the dark matter. It is universally accepted that there is an abundance of matter in the universe which is non-luminous, due to their very weak…

天体物理学 · 物理学 2007-05-23 Shibaji Banerjee , Abhijit Bhattacharyya , Sanjay K. Ghosh , Sibaji Raha , Bikash Sinha

Theoretical models of self-interacting dark matter represent a promising answer to a series of open problems within the so-called collisionless cold dark matter (CCDM) paradigm. In case of asymmetric dark matter, self-interactions might…

高能天体物理现象 · 物理学 2017-08-02 Andrea Maselli , Pantelis Pnigouras , Niklas Gønlund Nielsen , Chris Kouvaris , Kostas D. Kokkotas

In this study, we investigate a scenario that dark matter (DM) has only gravitational interaction. In the framework of effective field theory of gravity, we find that DM is still stable at tree level even if there is no symmetry to protect…

高能物理 - 唯象学 · 物理学 2016-06-07 Yong Tang , Yue-Liang Wu

We show that the Earth acts as a high-efficiency gravitational collector of low-velocity flow of dark matter (DM). The focal point appears on the Earth's surface, when the DM flow speed is about 17 km/s with respect to the geo-center. We…

高能天体物理现象 · 物理学 2020-05-21 Yoshiaki Sofue

Dark matter could take the form of dark massive compact halo objects (dMACHOs); i.e., composite objects that are made up of dark-sector elementary particles, that could have a macroscopic mass from the Planck scale to above the solar mass…

宇宙学与河外天体物理 · 物理学 2020-10-05 Yang Bai , Andrew J. Long , Sida Lu

We reinterpret the results of the direct searches for dark matter in terms of composite dark matter, i.e. dark matter particles that form neutral bound states, generically called dark atoms, either with ordinary particles, or with other…

高能物理 - 唯象学 · 物理学 2016-01-20 Quentin Wallemacq

It has been suggested ``that DM particles are strongly interacting composite macroscopically large objects ... made of well known light quarks (or ... antiquarks)." In doing so it is argued that these compact composite objects (CCOs) are…

天体物理学 · 物理学 2008-11-26 Daniel T. Cumberbatch , Glenn D. Starkman , Joseph Silk

Many experiments have searched for supersymmetric WIMP dark matter, with null results. This may suggest to look for more exotic possibilities, for example compact ultra-dense quark nuggets, widely discussed in literature with several…

Ordinary baryonic particles (such as protons and neutrons) account for only one-sixth of the total matter in the Universe. The remainder is a mysterious "dark matter" component, which does not interact via electromagnetism and thus neither…

If cosmic strings have an irreducible core, then dark matter may consist of entities that are core-sized string remnants. As such they may interact solely by gravity. These talons may be many orders of magnitude more massive than any known…

综合物理 · 物理学 2020-05-15 Richard Packard

When rotation is not taken into account, the measurement of the Gravitational Redshift can provide unique information about the compactness ($M/R$) of the star. Rotation alters the gravitational redshift rendering thereby a unique…

天体物理学 · 物理学 2011-06-10 Paul Nunez , Marek Nowakowski

Astronomical and cosmological observations of the past 80 years build solid evidence that atomic matter makes up only a small fraction of the matter in the universe. The dominant fraction does not interact with electromagnetic radiation,…

宇宙学与河外天体物理 · 物理学 2015-05-27 Wolfgang Rau

A comet-like, but magnitudes smaller, extremely low albedo interstellar meteoroid population of fragile aggregates with solar type composition, measured in space and terrestrially, is most probably the universal dark matter. Although…

天体物理学 · 物理学 2007-05-23 Robert K. Soberman , Maurice Dubin

Near a black hole or an ultracompact star, motion of particles is governed by strong gravitational field. Electrically charged particles feel also electromagnetic force arising due to currents inside the star or plasma circling around. We…

天体物理学 · 物理学 2009-06-23 Jiri Kovar , Zdenek Stuchlik , Vladimir Karas

Recent results of microlensing surveys, show that 10-20% of the dark halo mass of the Milky Way consists of compact objects. The masses of these compact objects range from 0.1 to 1 solar mass. New theoretical cooling models for white…

天体物理学 · 物理学 2007-05-23 Jelte de Jong , Konrad Kuijken , Mark Neeser

Dark matter exists in our Universe, but its nature remains mysterious. The remarkable sensitivity of the Laser Interferometer Gravitational-Wave Observatory (LIGO) may be able to solve this mystery. A good dark matter candidate is the…

高能物理 - 唯象学 · 物理学 2019-12-12 Huai-Ke Guo , Keith Riles , Feng-Wei Yang , Yue Zhao

In many models, dark matter particles can elastically scatter with nuclei in planets, causing those particles to become gravitationally bound. While the energy expected to be released through the subsequent annihilations of dark matter…

地球与行星天体物理 · 物理学 2015-05-27 Dan Hooper , Jason H. Steffen

The cold dark matter (CDM) cosmological model unambigously predicts that a large number of haloes should survive as subhaloes when they are accreted into a larger halo. The CDM model would be ruled out if such substructures were shown not…

宇宙学与河外天体物理 · 物理学 2016-04-27 Ran Li , Carlos S. Frenk , Shaun Cole , Liang Gao , Sownak Bose , Wojciech A. Hellwing