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Omega Centauri, the largest known globular cluster in the Milky Way, is believed to be the remains of a dwarf galaxy's core. Giving its potential abundance of dark matter (DM), it is an attractive target for investigating the nature of this…

高能天体物理现象 · 物理学 2024-07-03 Guan-Sen Wang , Zhan-Fang Chen , Lei Zu , Hao Gong , Lei Feng , Yi-Zhong Fan

The Galactic Center region is expected to host the largest density of Dark Matter (DM) particles within the Milky Way. Then a relatively large gamma-ray signal would be expected from the possible DM particles annihilation (or decay). We are…

高能天体物理现象 · 物理学 2019-08-14 Vincenzo Vitale , Aldo Morselli

Recent gamma-ray and radio studies have obtained some stringent constraints on annihilating dark matter properties. However, only a few studies have focussed on using X-ray data to constrain annihilating dark matter. In this article, we…

星系天体物理 · 物理学 2022-08-15 Man Ho Chan , Chak Man Lee

As a well-motivated dark matter candidate, axions can be detected through the axion-photon resonant conversion in the magnetospheres of magnetic white dwarf stars or neutron stars. In this work, we utilize Omega Centauri, which is the…

高能天体物理现象 · 物理学 2021-11-24 Jin-Wei Wang , Xiao-Jun Bi , Peng-Fei Yin

We focus on two aspects of Omega Cen that are rather uncharacteristic of globular clusters: its metallicity distribution and its orbit. We use (1) a Washington (M-T_2,M)_o color-magnitude diagram containing 130,000 stars, (2) DDO51…

天体物理学 · 物理学 2007-05-23 S. R. Majewski , R. J. Patterson , D. I. Dinescu , W. Y. Johnson , J. C. Ostheimer , W. E. Kunkel , C. Palma

Dark matter is the dominant form of matter in the universe, but its nature is unknown. It is plausibly an elementary particle, perhaps the lightest supersymmetric partner of known particle species. In this case, annihilation of dark matter…

Recent observational studies of $\gamma$-ray emission from massive globular clusters (GCs) have revealed possible evidence of dark matter (DM) annihilation within GCs. It is, however, still controversial whether the emission comes from DM…

星系天体物理 · 物理学 2020-05-20 Henriette Wirth , Kenji Bekki , Kohei Hayashi

The center of the Milky Way is one of the most interesting regions of the $\gamma$-ray sky because of the potential for indirect dark matter (DM) detection. It is also complicated due to the many sources and uncertainties associated with…

高能物理 - 唯象学 · 物理学 2014-10-10 German A. Gomez-Vargas

Clusters of galaxies are the largest gravitationally-bound systems in the Universe. Their dynamics are dominated by dark matter (DM), which makes them among the best targets for indirect DM searches. We analyze 12 years of data collected by…

高能天体物理现象 · 物理学 2023-05-03 Mattia Di Mauro , Judit Pérez-Romero , Miguel A. Sánchez-Conde , Nicolao Fornengo

Dark matter (DM) constitutes around a 25% of the Universe, while baryons only a 4%. DM can be reasonably assumed to be made of particles, and many theories (Super-symmetry, Universal Extra Dimensions, etc.) predict Weakly Interacting…

高能天体物理现象 · 物理学 2022-03-02 A. Morselli , B. Canadas , V. Vitale

We explore two possible scenarios to explain the observed gamma-ray emission associated with the atypical globular cluster Omega-Centauri: emission from millisecond pulsars (MSP) and dark matter (DM) annihilation. In the first case the…

Omega Centauri is the most massive globular cluster of the Milky Way, and possesses many peculiar properties. In particular, the cluster contains distinct multiple stellar populations, with a large spread in metallicity and different…

星系天体物理 · 物理学 2019-02-27 Rodrigo Ibata , Michele Bellazzini , Khyati Malhan , Nicolas Martin , Paolo Bianchini

The most massive and complex globular clusters in the Galaxy are thought to have originated as the nuclear cores of now tidally disrupted dwarf galaxies, but the connection between globular clusters and dwarf galaxies is tenuous with the…

太阳与恒星天体物理 · 物理学 2020-05-13 Christian I. Johnson , Andrea K. Dupree , Mario Mateo , John I. Bailey , Edward W. Olszewski , Matthew G. Walker

Dark matter (DM) is one of the major components in the Universe. However, at present its existence is still only inferred through indirect astronomical observations. DM particles can annihilate or decay, producing final-state Standard Model…

高能天体物理现象 · 物理学 2023-09-19 Francesco Gabriele Saturni , Michele Doro , Aldo Morselli , Gonzalo Rodríguez-Fernández

The presence of dark matter (DM) is suggested by a wealth of astrophysical and cosmological measurements. However, its underlying nature is yet unknown. Among the most promising candidates are weakly interacting massive particles (WIMPs):…

高能天体物理现象 · 物理学 2021-08-25 A. Montanari , E. Moulin , D. Malyshev

The most massive globular cluster in the Milky Way, omega Centauri, is thought to be the remaining core of a disrupted dwarf galaxy, as expected within the model of hierarchical merging. It contains several stellar populations having…

星系天体物理 · 物理学 2015-05-14 Jae-Woo Lee , Young-Woon Kang , Jina Lee , Young-Wook Lee

Dark matter is thought to make up most of the matter density of the Universe, yet its true nature remains uncertain. Among dark matter theories, Weakly Interacting Massive Particles (WIMPs) are a prominent candidate for dark matter because…

高能天体物理现象 · 物理学 2023-09-20 Micael Andrade , Aion Viana

The dwarf spheroidal satellite galaxies of the Milky Way are some of the most dark-matter-dominated objects known. Due to their proximity, high dark matter content, and lack of astrophysical backgrounds, dwarf spheroidal galaxies are widely…

高能天体物理现象 · 物理学 2019-08-14 Matthew Wood , Brandon Anderson , Alex Drlica-Wagner , Johann Cohen-Tanugi , Jan Conrad

Dark Matter (DM) is an elusive form of matter which has been postulated to explain astronomical observations through its gravitational effects on stars and galaxies, gravitational lensing of light around these, and through its imprint on…

高能物理 - 唯象学 · 物理学 2016-06-07 James Bateman , Ian McHardy , Alexander Merle , Tim R. Morris , Hendrik Ulbricht

Over the past few decades, a consensus picture has emerged in which roughly a quarter of the universe consists of dark matter. I begin with a review of the observational evidence for the existence of dark matter: rotation curves of…

宇宙学与河外天体物理 · 物理学 2017-05-31 Katherine Freese
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