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We use a combined 1.2 Ms of $NuSTAR$ observations of M31 to search for X-ray lines from sterile neutrino dark matter decay. For the first time in a $NuSTAR$ analysis, we consistently take into account the signal contribution from both the…

High Energy Astrophysical Phenomena · Physics 2019-04-24 Kenny C. Y. Ng , Brandon M. Roach , Kerstin Perez , John F. Beacom , Shunsaku Horiuchi , Roman Krivonos , Daniel R. Wik

We analyze two dedicated NuSTAR observations with exposure ${\sim}190$ ks located ${\sim}10^\circ$ from the Galactic plane, one above and the other below, to search for x-ray lines from the radiative decay of sterile-neutrino dark matter.…

High Energy Astrophysical Phenomena · Physics 2020-05-11 Brandon M. Roach , Kenny C. Y. Ng , Kerstin Perez , John F. Beacom , Shunsaku Horiuchi , Roman Krivonos , Daniel R. Wik

We present two complementary NuSTAR x-ray searches for keV-scale dark matter decaying to mono-energetic photons in the Milky Way halo. In the first, we utilize the known intensity pattern of unfocused stray light across the detector planes…

Using tremendous photon statistics gained with the stray light aperture of the NuSTAR telescope over 11 years of operation, we set strong limits on the emission of close to monochromatic photons from the radiative decays of putative dark…

High Energy Physics - Phenomenology · Physics 2024-12-30 R. A. Krivonos , V. V. Barinov , A. A. Mukhin , D. S. Gorbunov

We present the results of the search for decaying dark matter with particle mass in the 6-40 keV range with NuSTAR deep observations of COSMOS and ECDFS empty sky fields. We show that main contribution to the decaying dark matter signal…

High Energy Astrophysical Phenomena · Physics 2016-12-07 Andrii Neronov , Denys Malyshev , Dominique Eckert

A sterile neutrino of ~keV mass is a well motivated dark matter candidate. Its decay generates an X-ray line that offers a unique target for X-ray telescopes. For the first time, we use the Gamma-ray Burst Monitor (GBM) onboard the Fermi…

Cosmology and Nongalactic Astrophysics · Physics 2015-08-07 Kenny C. Y. Ng , Shunsaku Horiuchi , Jennifer M. Gaskins , Miles Smith , Robert Preece

We calculate the most stringent constraints up to date on the parameter space for sterile neutrino warm dark matter models possessing a radiative decay channel into X-rays. These constraints arise from the X-ray flux observations from the…

Astrophysics of Galaxies · Physics 2018-10-16 R. Yunis , C. R. Argüelles , N. E. Mavromatos , A. Moliné , A. Krut , J. A. Rueda , R. Ruffini

Line emission from dark matter is well motivated for some candidates e.g. sterile neutrinos. We present the first search for dark matter line emission in the 3-80keV range in a pointed observation of the Bullet Cluster with NuSTAR. We do…

For the first time, we use the Gamma-ray Burst Monitor (GBM) on-board the Fermi satellite to search for sterile neutrino decay lines in the energy range 10-25 keV corresponding to sterile neutrino mass range 20-50 keV. This energy range has…

High Energy Astrophysical Phenomena · Physics 2015-02-12 Shunsaku Horiuchi , Kenny C. Y. Ng , Jennifer M. Gaskins , Miles Smith , Robert Preece

Sterile neutrinos with masses in the keV range are well-motivated extensions to the Standard Model that could explain the observed neutrino masses while also making up the dark matter (DM) of the Universe. If sterile neutrinos are DM then…

Cosmology and Nongalactic Astrophysics · Physics 2021-08-04 Joshua W. Foster , Marius Kongsore , Christopher Dessert , Yujin Park , Nicholas L. Rodd , Kyle Cranmer , Benjamin R. Safdi

Sterile neutrinos are attractive dark matter candidates. Their parameter space of mass and mixing angle has not yet been fully tested despite intensive efforts that exploit their gravitational clustering properties and radiative decays. We…

Astrophysics · Physics 2008-11-26 Hasan Yuksel , John F. Beacom , Casey R. Watson

Sterile neutrinos may be one of the best Warm Dark Matter candidates we have today. Both lower and upper bounds on the mass of the sterile neutrino come from astronomical observations. We show that the proper inclusion of the neutrino…

Astrophysics · Physics 2008-11-26 Steen H. Hansen , Julien Lesgourgues , Sergio Pastor , Joseph Silk

Space-based instruments provide new and, in some cases, unique opportunities to search for dark matter. In particular, if dark matter comprises sterile neutrinos, the x ray detection of their decay line is the most promising strategy for…

Astrophysics · Physics 2008-11-26 Alexander Kusenko

We use the Chandra unresolved X-ray emission spectrum from a 12'-28' (2.8-6.4 kpc) annular region of the Andromeda galaxy to constrain the radiative decay of sterile neutrino warm dark matter. By excising the most baryon-dominated, central…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Casey R. Watson , Zhiyuan Li , Nicholas K. Polley

Warm dark matter (WDM) might more easily account for small scale clustering measurements than the heavier particles typically invoked in Lambda cold dark matter (LCDM) cosmologies. In this paper, we consider a Lambda WDM cosmology in which…

Astrophysics · Physics 2009-11-11 Casey R. Watson , John F. Beacom , Hasan Yuksel , Terry P. Walker

It is possible that the strongest interactions between dark matter and the Standard Model occur via the neutrino sector. Unlike gamma rays and charged particles, neutrinos provide a unique avenue to probe for astrophysical sources of dark…

High Energy Physics - Phenomenology · Physics 2023-11-07 Carlos A. Argüelles , Diyaselis Delgado , Avi Friedlander , Ali Kheirandish , Ibrahim Safa , Aaron C. Vincent , Henry White

We perform an exhaustive scan of the allowed resonant production regime for sterile neutrino dark matter in order to improve constraints for dark matter structures which arise from the non-thermal sterile neutrino energy spectra.…

High Energy Physics - Phenomenology · Physics 2017-05-03 John F. Cherry , Shunsaku Horiuchi

We report the results of a search for an emission line from radiatively decaying dark matter in the Chandra X-ray Observatory spectrum of the ultra-faint dwarf spheroidal galaxy Willman 1. 99% confidence line flux upper limits over the…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Michael Loewenstein , Alexander Kusenko

Recently an unidentified emission line at 3.55 keV has been detected in X-ray spectra of clusters of galaxies. The line has been discussed as a possible decay signature of 7.1 keV sterile neutrinos, which have been proposed as a dark matter…

High Energy Astrophysical Phenomena · Physics 2019-05-29 F. Hofmann , C. Wegg

We report new constraints on the velocity-independent annihilation cross section $\langle \sigma v \rangle$ of keV-scale dark matter particles based on 11 years of observations with the NuSTAR X-ray telescope. Using the unfocused stray…

High Energy Astrophysical Phenomena · Physics 2025-12-30 E. I. Zakharov , V. V. Barinov , D. S. Gorbunov , R. A. Krivonos , A. A. Mukhin
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