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Recent observations have discovered star formation activities in the extreme outer regions of disk galaxies. However it remains unclear what physical mechanisms are responsible for triggering star formation in such low-density gaseous…

天体物理学 · 物理学 2009-11-13 Kenji Bekki , Masashi Chiba

We reply to criticisms by Desch et al. (2021) regarding our Scientific Reports paper, "Breakup of a long-period comet as the origin of the dinosaur extinction." The background impact rates of main-belt asteroids and long-period comets have…

地球与行星天体物理 · 物理学 2021-05-26 Amir Siraj , Abraham Loeb

The physical processes defining the dynamics of disk galaxies are still poorly understood. Hundreds of articles have appeared in the literature over the last decades without arriving at an understanding within a consistent gravitational…

星系天体物理 · 物理学 2020-05-26 Klaus Wilhelm , Bhola N. Dwivedi

We analyze 11 years of Fermi-LAT data corresponding to the sky regions of 7 dwarf irregular (dIrr) galaxies. DIrrs are dark matter (DM) dominated systems, proposed as interesting targets for the indirect search of DM with gamma rays. The…

宇宙学与河外天体物理 · 物理学 2022-11-28 V. Gammaldi , J. Pérez-Romero , J. Coronado-Blázquez , M. Di Mauro , E. V. Karukes , M. A. Sánchez-Conde , P. Salucci

Within the standard cosmological scenario the Universe is found to be filled by obscure components (dark matter and dark energy) for ~95% of its energy budget. In particular, almost all the matter content in the Universe is given by dark…

宇宙学与河外天体物理 · 物理学 2015-06-04 Crescenzo Tortora , Philippe Jetzer , Nicola R. Napolitano

In this review, I discuss just three aspects of the stability and evolution of galactic discs. (1) I first review our understanding of the bar instability and how it can be controlled. Disc galaxies in which the orbital speed does not…

天体物理学 · 物理学 2007-05-23 J. A. Sellwood

Dark Matter (DM) being the vital ingredient in the cosmos, still remains a mystery. Standard assumption is that the collisionless cold dark matter (CCDM) particles are represented by some weakly interacting fundamental fields which can not…

天体物理学 · 物理学 2009-11-11 Ariel Zhitnitsky

The proposal of a galactic population of intermediate mass black holes (IMBHs), forming dark matter (DM) ``mini-spikes'' around them, has received considerable attention in recent years. In fact, leading in some scenarios to large…

宇宙学与河外天体物理 · 物理学 2010-04-15 Torsten Bringmann , Julien Lavalle , Pierre Salati

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…

高能物理 - 唯象学 · 物理学 2015-03-10 Jonathan H. Davis

The Oort cloud is usually thought of as a collection of icy comets inhabiting the outer reaches of the Solar system, but this picture is incomplete. We use simulations of the formation of the Oort cloud to show that ~4% of the small bodies…

地球与行星天体物理 · 物理学 2015-06-23 Andrew Shannon , Alan P. Jackson , Dimitri Veras , Mark Wyatt

The search for a particle dark matter signal in terms of radiation produced by dark matter annihilation or decay has to cope with the extreme faintness of the predicted signal and the presence of masking astrophysical backgrounds. It has…

宇宙学与河外天体物理 · 物理学 2022-11-11 S. Arcari , E. Pinetti , N. Fornengo

Stationary, axisymmetric, dust sourced solutions of Einstein's equations have been proposed as fully general relativistic models for disc galaxies. These models introduce a novel physical element, i.e., a non-negligible dragging vortex…

广义相对论与量子宇宙学 · 物理学 2024-10-17 Federico Re , Marco Galoppo

We continue our exploration of whether the flyby anomalies can be explained by scattering of spacecraft nucleons from dark matter gravitationally bound to the earth, with the addition of data from five new flybys to that from the original…

地球与行星天体物理 · 物理学 2015-06-03 Stephen L. Adler

The dark matter hypothesis, which is not called into question here, explains why typical rotation curves of spiral galaxies do not follow a Keplerian profile. It is however not sufficient in itself to explain why the whole matter…

星系天体物理 · 物理学 2019-06-13 Vincent Deledicque

We propose a novel mechanism to explain the positron excesses, which are observed by satellite-based telescopes including PAMELA and AMS-02, in dark matter (DM) scenarios. The novelty behind the proposal is that it makes direct use of DM…

高能物理 - 唯象学 · 物理学 2018-05-09 Doojin Kim , Jong-Chul Park , Seodong Shin

We show that a Magellanic Cloud origin for the warp of the Milky Way can explain most quantitative features of the outer HI layer recently identified by Levine, Blitz & Heiles (2005). We construct a model similar to that of Weinberg (1998)…

天体物理学 · 物理学 2009-11-11 Martin D. Weinberg , Leo Blitz

In a recent paper (arXiv:1106.4546), we introduced "dynamical dark matter," a new framework for dark-matter physics, and outlined its underlying theoretical principles and phenomenological possibilities. Unlike most traditional approaches…

高能物理 - 唯象学 · 物理学 2013-05-30 Keith R. Dienes , Brooks Thomas

We present the first detailed analysis of the effects of dissipative dark matter on stellar streams. As a concrete example, we generate a cosmological hydrodynamic zoom-in simulation of a Milky Way-mass galaxy, assuming that the dark matter…

We study eccentric equatorial orbits of a stellar-mass black hole around an intermediate-mass slowly rotating Kerr black hole in the presence of gravitational radiation and a dark matter halo. The stellar-mass companion will inspiral…

广义相对论与量子宇宙学 · 物理学 2025-05-13 Darkhan Shadykul , Hrishikesh Chakrabarty , Daniele Malafarina

We propose that the cloud moving on a highly eccentric orbit near the central black hole in our Galaxy, reported by Gillessen et al., is formed by a photoevaporation wind originating in a disk around a star that is tidally perturbed and…

星系天体物理 · 物理学 2015-06-04 Jordi Miralda-Escude