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Related papers: Dark-Matter Harmonics Beyond Annual Modulation

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For many years annually modulating $\sim$ keV scintillations have been observed in the DAMA/NaI and DAMA/Libra experiments. A dark matter - electron scattering interpretation is now favoured given the stringent constraints on nuclear recoil…

High Energy Physics - Phenomenology · Physics 2016-07-01 R. Foot

It has recently been demonstrated that, in the event of a putative signal in dark matter direct detection experiments, properly identifying the underlying dark matter-nuclei interaction promises to be a challenging task. Given the most…

High Energy Physics - Phenomenology · Physics 2017-03-08 Samuel J. Witte , Vera Gluscevic , Samuel D. McDermott

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…

High Energy Physics - Phenomenology · Physics 2018-04-25 Asimina Arvanitaki , Peter W. Graham , Jason M. Hogan , Surjeet Rajendran , Ken Van Tilburg

We compute the decay spectrum for dark matter (DM) with masses above the scale of electroweak symmetry breaking, all the way to the Planck scale. For an arbitrary hard process involving a decay to the unbroken standard model, we determine…

High Energy Physics - Phenomenology · Physics 2021-07-07 Christian W. Bauer , Nicholas L. Rodd , Bryan R. Webber

We study a simple model of dark matter that is gravitationally clustered around the sun in the form of a spherical halo of a degenerate gas of heavy neutrinos. It is shown that for neutrino masses $m_{\nu} \stackrel {\textstyle <}{\sim}…

Astrophysics · Physics 2007-05-23 F. Munyaneza , R. D. Viollier

In the present work we study possible time dependent effects in Axion Dark Matter searches employing resonant cavities. We find that the width of the resonance, which depends on the axion mean square velocity in the local frame, will show…

High Energy Physics - Phenomenology · Physics 2015-12-09 Y. Semertzidis , J. D. Vergados

Dark matter comprises the bulk of the matter in the universe but its particle nature and cosmological origin remain mysterious. Knowledge of the dark matter density distribution in the Milky Way Galaxy is crucial to both our understanding…

The modulation effect in the direct detection of supersymmetric Cold Dark Matter (CDM) particles is investigated. It is shown that, while normally the modulation effect in the total event rate is small, $\leq 5% $, in some special cases it…

High Energy Physics - Phenomenology · Physics 2014-11-17 J. D. Vergados

Future multi-tonne Direct Detection experiments will be sensitive to solar neutrino induced nuclear recoils which form an irreducible background to light Dark Matter searches. Indeed for masses around 6 GeV the spectra of neutrinos and Dark…

High Energy Physics - Phenomenology · Physics 2015-03-10 Jonathan H. Davis

We point out that for a range of parameters, the flux of DM may be stopped significantly by its interactions with the Earth. This can significantly degrade the sensitivity of direct detection experiments to DM candidates with large…

High Energy Physics - Phenomenology · Physics 2015-04-02 Chris Kouvaris , Ian M. Shoemaker

We investigate the interactions of large composite dark matter (DM) states with the Standard Model (SM) sector. Elastic scattering with SM nuclei can be coherently enhanced by factors as large as A^2, where A is the number of constituents…

High Energy Physics - Phenomenology · Physics 2021-01-21 Edward Hardy , Robert Lasenby , John March-Russell , Stephen M. West

Techniques for inferring the radial and geometric form of dark matter halos and the results they have produced to date are reviewed. Dark halos appear to extend to at least ~50 kpc with total enclosed masses that rise linearly with radius…

Astrophysics · Physics 2007-05-23 Penny D. Sackett

Recent N-body simulations indicate that a thick disc of dark matter, co-rotating with the stellar disc, forms in a galactic halo after a merger at a redshift $z<2$. The existence of such a dark disc component in the Milky Way could affect…

Astrophysics of Galaxies · Physics 2014-11-20 Fu-Sin Ling

We make preliminary estimates to assess whether the recently reported flyby anomaly can be attributed to dark matter interactions. We consider both elastic and exothermic inelastic scattering from dark matter constituents; for isotropic…

Astrophysics · Physics 2009-01-16 Stephen L. Adler

Advances in high angular resolution astronomy make it conceivable that black hole dark matter could be detected via angular deviation effects. Assuming the dark matter in the galaxy is made of solar mass black holes, there is a non-trivial…

Cosmology and Nongalactic Astrophysics · Physics 2021-03-08 Leo Stodolsky

A recent study conducted using CALIFA survey data (Lee et al, 2019b) has found that the orbital motions of neighbor galaxies are coherent with the spin direction of a target galaxy on scales of many Megaparsecs. We study this so called…

Cosmology and Nongalactic Astrophysics · Physics 2022-08-24 Yigon Kim , Rory Smith , Jihye Shin

Galactic halos are of great importance for our understanding of both the dark matter nature and primordial non-Gaussianity in the perturbation spectrum, a powerful discriminant of the physical mechanisms that generated the cosmological…

In this paper we study the effect of the channeling of ions recoiling from collisions with weakly interacting massive particles (WIMPs) in single crystal detectors. In particular we investigate the possibility that channeling may give rise…

Instrumentation and Methods for Astrophysics · Physics 2015-05-19 Richard J. Creswick , Shmuel Nussinov , Frank T. Avignone

Directional detection of dark matter is the next generation experiment, which is expected to have better back ground rejection efficiency than conventional direct search. Another intriguing possibility of the experiment by means of the…

High Energy Physics - Phenomenology · Physics 2014-12-16 Keiko I. Nagao

Halometry---mapping out the spectrum, location, and kinematics of nonluminous structures inside the Galactic halo---can be realized via variable weak gravitational lensing of the apparent motions of stars and other luminous background…

Cosmology and Nongalactic Astrophysics · Physics 2018-08-08 Ken Van Tilburg , Anna-Maria Taki , Neal Weiner