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If a component of the dark matter has dissipative interactions, it could collapse to form a thin dark disk in our Galaxy that is coplanar with the baryonic disk. It has been suggested that dark disks could explain a variety of observed…

星系天体物理 · 物理学 2018-09-03 Katelin Schutz , Tongyan Lin , Benjamin R. Safdi , Chih-Liang Wu

Dark matter, one of the important portion of the universe, could affect the visible matter in neutron stars. An important physical feature of dark matter is due to the spin of dark matter particles. Here, applying the piecewise polytropic…

高能物理 - 唯象学 · 物理学 2018-04-19 Zeinab Rezaei

Dark matter, proposed decades ago as a speculative component of the universe, is now known to be the vital ingredient in the cosmos, eight times more abundant than ordinary matter, one quarter of the total energy density and the component…

天体物理学 · 物理学 2009-09-15 Jeremiah P. Ostriker , Paul J. Steinhardt

We analyze a cosmological model featuring an interaction between dark energy and dark matter in light of the measurements of the Cosmic Microwave Background released by three independent experiments: the most recent data by the Planck…

宇宙学与河外天体物理 · 物理学 2023-07-13 Yuejia Zhai , William Giarè , Carsten van de Bruck , Eleonora Di Valentino , Olga Mena , Rafael C. Nunes

Phenomena currently attributed to Dark Matter (DM) and Dark Energy (DE) are merely a result of the interplay between gravitational energy density, caused by the contraction of space by matter, and space dilation, caused by the energy…

天体物理学 · 物理学 2008-10-23 Shlomo Barak , Elia M. Leibowitz

If multiple thermal weakly interacting massive particle (WIMP) dark matter candidates exist, then their capture and annihilation dynamics inside a massive stars such as Sun could change from conventional method of study. With a simple…

高能物理 - 唯象学 · 物理学 2023-04-25 Amit Dutta Banik

The nature of the dark matter in the halo of our Galaxy is still largely unknown. The microlensing events found so far towards the Large Magellanic Cloud suggest that at most about 20% of the halo dark matter is in the form of MACHOs…

高能物理 - 唯象学 · 物理学 2017-08-23 Philippe Jetzer

Our standard model of the Universe predicts the distribution of dark matter to $1\%$ at the scales needed for upcoming experiments, yet our predictions for how the luminous matter -- which has interactions besides gravity -- is distributed…

高能物理 - 理论 · 物理学 2025-03-03 Nora Elisa Chisari

We revisit the question of whether the observed periodicity of comet impacts on Earth is consistent with Solar oscillation about the Galactic midplane and spiral arm crossings, here in the context of dissipative dark matter models. Consider…

地球与行星天体物理 · 物理学 2017-03-01 Eric David Kramer , Michael Rowan

Although various pieces of indirect evidence about the nature of dark matter have been collected, its direct detection has eluded experimental searches despite extensive effort. If the mass of dark matter is below 1 MeV, it is essentially…

量子物理 · 物理学 2013-12-16 C. Jess Riedel

Astronomical and cosmological observations of the past 80 years build solid evidence that atomic matter makes up only a small fraction of the matter in the universe. The dominant fraction does not interact with electromagnetic radiation,…

宇宙学与河外天体物理 · 物理学 2015-05-27 Wolfgang Rau

We investigate phenomenological interactions between dark matter and dark energy and constrain these models by employing the most recent cosmological data including the cosmic microwave background radiation anisotropies from Planck 2015,…

宇宙学与河外天体物理 · 物理学 2017-01-25 André A. Costa , Xiao-Dong Xu , Bin Wang , E. Abdalla

We look at our since long studied model for dark matter as being pearls of a speculated new vacuum containing highly compressed ordinary matter, with so much ordinary in it that the content of ordinary matter in the dark matter pearls…

高能物理 - 唯象学 · 物理学 2026-02-10 Colin D. Froggatt , Holger Bech Nielsen

Microlensed double-image quasars have sent a consistent message that the baryonic dark matter consists of a population of free-roaming planet mass objects, as summarized previously. These were previously predicted to have formed at the time…

天体物理学 · 物理学 2016-11-03 Rudolph E. Schild

The properties of a neutron star are studied in the presence of dark matter. We have considered a relatively light Weakly Interacting Massive Particle (WIMP) as a dark matter candidate with properties suggested by the results of the…

核理论 · 物理学 2020-08-26 Abdul Quddus , Grigorios Panotopoulos , Bharat Kumar , Shakeb Ahmad , S. K. Patra

Melanoma is a type of skin cancer with the most rapidly increasing incidence. Early detection of melanoma using dermoscopy images significantly increases patients' survival rate. However, accurately classifying skin lesions by eye,…

计算机视觉与模式识别 · 计算机科学 2019-02-14 Xiaoxiao Li , Junyan Wu , Eric Z. Chen , Hongda Jiang

Multiple astrophysical and cosmological observations show that the majority of the matter in the universe is non-luminous. It is not made of known particles, and it is called dark matter. This is one of the few pieces of concrete…

高能物理 - 实验 · 物理学 2020-01-01 Oliver Buchmueller , Caterina Doglioni , Lian-Tao Wang

Exotic dark matter together with dark energy or cosmological constant seem to dominate in the Universe. An even higher density of such matter seems to be gravitationally trapped in our Galaxy. The nature of dark matter can be unveiled only,…

核理论 · 物理学 2009-09-29 J. D. Vergados

A series of dynamical anomalies in the orbits of distant trans-Neptunian objects points to a new celestial body (usually named Planet Nine) in the solar system. In this draft, we point out that a mirror planet captured from the outer solar…

地球与行星天体物理 · 物理学 2022-10-11 Pei Wang , Yu Chen Tang , Lei Zu , Yuan Yuan Chen , Lei Feng

The detection of dark matter is central to particle physics and cosmology. Current fashionable supersymmetric models provide a dark matter candidate, the lightest supersymmetric particle (LSP). When combined with fairly well understood…

天体物理学 · 物理学 2007-05-23 J. D. Vergados