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相关论文: $G$ Objects and primordial black holes

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We consider the possibility that the weakly interacting massive particles produced from the evaporation of primordial black hole can explain both the relic density of dark matter and the baryon asymmetry of the Universe, through their…

高能物理 - 唯象学 · 物理学 2024-02-22 Ki-Young Choi , Jongkuk Kim , Erdenebulgan Lkhagvadorj

In 2011, we discovered a compact gas cloud ("G2") with roughly three Earth masses that is falling on a near-radial orbit toward the massive black hole in the Galactic Center. The orbit is well constrained and pericenter passage is predicted…

In the mass range of 1e15 g up to 1e26 g, primordial black holes (PBHs) as a possible contribution to the dark matter are still unexplored. In this contribution, we investigate the possibility of an electromagnetic signal from PBH…

宇宙学与河外天体物理 · 物理学 2009-05-20 Julia K. Becker , Marek A. Abramowicz , Peter L. Biermann

Primordial black holes (PBHs), if they exist, may collide with and be captured by neutron stars. We adopt a relativistic point-mass approximation to study this capture, the subsequent confinement of the PBH of mass $m$ inside the neutron…

广义相对论与量子宇宙学 · 物理学 2024-06-26 Thomas W. Baumgarte , Stuart L. Shapiro

In this paper, we show that in the vicinity of certain astronomical bodies, e.g., a Neutron Star, a Black Hole, there exist significant enhancements of Dark Matter's density and current, due to its interaction with the gravitational field…

高能物理 - 唯象学 · 物理学 2018-08-07 H. B. Tran Tan , V. V. Flambaum , J. C. Berengut

Despite intensive searches, the only pulsar within 0.1 pc of the central black hole in our Galaxy, Sgr A*, is a radio-loud magnetar. Since magnetars are rare among the Galactic neutron star population, and a large number of massive stars…

高能天体物理现象 · 物理学 2016-04-06 Dimitrios Giannios , Duncan R. Lorimer

In this small review we present the actual state the knowledge about weighting black holes. Black holes can be found in stellar binary systems in our Galaxy and in other nearby galaxies, in globular clusters, which we can see in our and…

高能天体物理现象 · 物理学 2009-10-05 B. Czerny , M. Nikolajuk

We investigate the effects of dark matter annihilation on objects with masses close to the sub-stellar limit, finding that the minimum mass for stable hydrogen burning is larger than the $\sim0.075 M_\odot $ value predicted in the Standard…

高能物理 - 唯象学 · 物理学 2025-09-09 Djuna Croon , Jeremy Sakstein , Juri Smirnov , Jack Streeter

Primordial black holes (PBHs) from the early Universe constitute an attractive dark matter candidate. First detections of black hole-neutron star (BH-NS) candidate gravitational wave events by the LIGO/Virgo collaboration, GW200105 and…

宇宙学与河外天体物理 · 物理学 2022-05-24 Misao Sasaki , Volodymyr Takhistov , Valeri Vardanyan , Ying-li Zhang

Primordial black holes (PBHs) could provide the dark matter but a variety of constraints restrict the possible mass windows to $10^{16} - 10^{17}$g, $10^{20} - 10^{24}$g and $10 - 10^3M_{\odot}$. The last possibility is of special interest…

宇宙学与河外天体物理 · 物理学 2020-01-08 Bernard Carr

The Galactic Center (GC) is potentially hosting the largest indirect signal from particle dark matter (DM), which in many well-motivated models would produce gamma rays as their final states. However, this region has often been dismissed…

高能物理 - 唯象学 · 物理学 2025-11-06 Silvia Manconi , Christopher Eckner , Francesca Calore , Fiorenza Donato

We argue that the hypothesis of the gravitational repulsion between matter and antimatter can be tested at the Ice Cube, a neutrino telescope, recently constructed at the South Pole. If there is such a gravitational repulsion, the…

广义相对论与量子宇宙学 · 物理学 2011-07-13 Dragan Slavkov Hajdukovic

It is often assumed that the strong gravitational field of a super-massive black hole disrupts an adjacent molecular cloud preventing classical star formation in the deep potential well of the black hole. Yet, young stars have been observed…

星系天体物理 · 物理学 2016-08-10 B. Jalali , F. I. Pelupessy , A. Eckart , S. Portegies Zwart , N. Sabha , A. Borkar , J. Moultaka , K. Mužić , L. Moser

In this proceedings, we study the possible gravitational impact of primordial black holes (PBHs) or dark matter (DM) clumps on GNSS satellite orbits and gravimeter measurements. It provides a preliminary step to the future exhaustive…

宇宙学与河外天体物理 · 物理学 2023-12-25 Bruno Bertrand , Michal Cuadrat-Grzybowski , Pascale Defraigne , Michel Van Camp , Sébastien Clesse

The Center of our Galaxy is a peculiar region where a number of crucial astrophysical phenomena take place, from star formation to SN explosions and accretion onto a massive black hole. The quest for a massive black hole in the Galactic…

天体物理学 · 物理学 2007-05-23 A. Goldwurm

We present a novel model-independent generic mechanism for primordial black hole formation within the context of non-singular matter bouncing cosmology. In particular, considering a short duration transition from the matter contracting…

广义相对论与量子宇宙学 · 物理学 2024-06-21 Theodoros Papanikolaou , Shreya Banerjee , Yi-Fu Cai , Salvatore Capozziello , Emmanuel N. Saridakis

Formation and disruption of dark-matter cusps are reviewed. Accumulation of baryons at the center of a halo can displace the dark matter, converting singular density cusps into low-density cores. The displaced mass can be of order 10 M_b…

天体物理学 · 物理学 2007-05-23 David Merritt , Milos Milosavljevic

We investigate a possibility of primordial black hole (PBH) formation with a hierarchical mass spectrum in multiple phases of inflation. As an example, we find that one can simultaneously realize a mass spectrum which has recently attracted…

宇宙学与河外天体物理 · 物理学 2019-08-13 Yuichiro Tada , Shuichiro Yokoyama

It has long been suspected that Active Galactic Nuclei are powered by accretion of matter onto massive black holes and this belief implies their presence in the nuclei of most nearby galaxies as "relics" of past activity. Just a few years…

天体物理学 · 物理学 2007-05-23 Alessandro Marconi

The accumulation of certain types of dark matter particles in neutron star cores due to accretion over long timescales can lead to the formation of a mini black hole. In this scenario, the neutron star is destabilized and implodes to form a…

广义相对论与量子宇宙学 · 物理学 2023-05-09 Divya Singh , Anuradha Gupta , Emanuele Berti , Sanjay Reddy , B. S. Sathyaprakash
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