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相关论文: A quest for weak objects and for invisible stars

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Exploring dark matter via observations of extreme astrophysical environments -- defined here as heavy compact objects such as white dwarfs, neutron stars, and black holes, as well as supernovae and compact object merger events -- has been a…

There is now abundant evidence for the presence of large quantities of unseen matter surrounding normal galaxies, including our own$^{1,2}$. The nature of this `dark matter' is unknown, except that it cannot be made of normal stars, dust,…

The nature of the dark matter in the Universe is one of the outstanding questions in astrophysics. In this talk, I address possible stellar baryonic contributions to the 50-90% of our Galaxy that is made of unknown dark matter. First I show…

天体物理学 · 物理学 2007-05-23 Katherine Freese , Brian Fields , David Graff

The nature of the dark matter of the Universe is yet unknown and most likely is connected with new physics. The search for its composition is under way through direct and indirect detection. Fundamental physical aspects such as energy…

高能物理 - 唯象学 · 物理学 2009-11-07 Ivone F. M. Albuquerque , Jodi Lamoureux , George F. Smoot

The ground state of matter may be strange quark matter (SQM), not hadronic matter. A whole sequence of SQM objects, ranging from strange quark stars and strange quark dwarfs to strange quark planets, can stably exist according to this SQM…

太阳与恒星天体物理 · 物理学 2022-07-04 Abdusattar Kurban , Yong-Feng Huang , Jin-Jun Geng , Hong-Shi Zong

MAssive Compact Halo Objects such as brown dwarfs, Jupiters, and black holes are prime candidates to comprise the dark halo of our galaxy. Paczynski noted that objects (dubbed MACHOs) with masses in the range $10^{-6}M_\odot < M \simlt 100…

天体物理学 · 物理学 2009-10-22 D. P. Bennett

In the past four decades a new type of astronomy has emerged, where instead of looking up into the sky "telescopes" are buried miles underground or deep under water or ice and search not for photons (that is, light), but rather for…

天体物理学 · 物理学 2008-11-26 E. Waxman

Over the past several years, there has been enormous interest in massive neutron stars and white dwarfs due to either their direct or indirect evidence. The recent detection of gravitational wave event GW190814 has confirmed the existence…

高能天体物理现象 · 物理学 2022-11-23 Banibrata Mukhopadhyay , Mukul Bhattacharya

I summarize here and discuss the results of presently operating neutrino telescopes in searching for a signal of dark matter weakly interacting massive particles (WIMPs).

高能物理 - 唯象学 · 物理学 2007-05-23 O. V. Suvorova

There is abundant evidence that the mass of the Universe is dominated by dark matter of unknown form. The MACHO project is one of several teams searching for the dark matter around our Galaxy in the form of Massive Compact Halo Objects…

天体物理学 · 物理学 2008-11-26 Will Sutherland

The Milky Way Galaxy contains a large, spherical component which is believed to harbor a substantial amount of unseen matter. Recent observations indirectly suggest that as much as half of this ``dark matter'' may be in the form of old,…

天体物理学 · 物理学 2009-10-12 B. R. Oppenheimer , N. C. Hambly , A. P. Digby , S. T. Hodgkin , D. Saumon

We present mid-infrared photometry of 124 white dwarf stars with Spitzer Space Telescope. Objects were observed simultaneously at 4.5 and 8.0um with sensitivities better than 1 mJy. This data can be used to test models of white dwarf…

Dark matter is one of the most important open problems in particle physics and cosmology. Weakly interacting massive particles (WIMPs) appear as an appealing solution, providing the right relic density with a cross-section at the…

高能物理 - 唯象学 · 物理学 2021-10-04 C. Siqueira , Guilherme N. Fortes , Aion Viana , Farinaldo Queiroz

Several dark matter models allow for the intriguing possibility of exotic compact object formation. These objects might have unique characteristics that set them apart from their baryonic counterparts. Furthermore, gravitational wave…

高能天体物理现象 · 物理学 2022-06-29 Michael Ryan , David Radice

White dwarfs and neutron stars are stellar objects with masses comparable to that of our sun. However, as the endpoint stages of stellar evolution, these objects do not sustain any thermonuclear burning and therefore can no longer support…

天体物理学 · 物理学 2007-05-23 Shmuel Balberg , Stuart L. Shapiro

The masses of compact objects like white dwarfs, neutron stars and black holes are fundamental to astrophysics, but very difficult to measure. We present the results of an analysis of subluminous B (sdB) stars in close binary systems with…

天体物理学 · 物理学 2008-04-09 S. Geier , C. Karl , H. Edelmann , U. Heber , R. Napiwotzki

The masses of compact objects like white dwarfs, neutron stars and black holes are fundamental to astrophysics, but very difficult to measure. We present the results of an analysis of subluminous B (sdB) stars in close binary systems with…

天体物理学 · 物理学 2008-11-26 S. Geier , C. Karl , H. Edelmann , U. Heber , R. Napiwotzki

The quest to understand the nature dark matter is one of the most relevant ones in Particle Physics nowadays, since it constitutes most of the matter of the Universe and it is still unknown what it is made of. In order to answer to this…

高能天体物理现象 · 物理学 2016-10-04 J. D. Zornoza

Recent detection of gravitational wave from nine black hole merger events and one neutron star merger event by LIGO and VIRGO shed a new light in the field of astrophysics. On the other hand, in the past decade, a few super-Chandrasekhar…

高能天体物理现象 · 物理学 2020-01-08 Surajit Kalita , Banibrata Mukhopadhyay

The cold dark matter of the Universe may be comprised of very light and very weakly interacting particles, so-called WISPs. Two prominent examples are hidden photons and axion-like particles. In this note we propose a new technique to…

高能物理 - 唯象学 · 物理学 2015-06-12 Dieter Horns , Joerg Jaeckel , Axel Lindner , Andrei Lobanov , Javier Redondo , Andreas Ringwald