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Related papers: Mirror matter-type dark matter

200 papers

The phenomenological implications of the eleven dimensional limit of $M$-theory (strongly coupled $E_8\times E_8$) are investigated. In particular we calculate the supersymmetric particle spectrum subject to constraints of correct…

High Energy Physics - Phenomenology · Physics 2014-11-17 D. Bailin , G. V. Kraniotis , A. Love

Asymmetric dark matter models are based on the hypothesis that the present-day abundance of dark matter has the same origin as the abundance of ordinary or visible matter: an asymmetry in the number densities of particles and antiparticles.…

High Energy Physics - Phenomenology · Physics 2013-08-02 Kalliopi Petraki , Raymond R. Volkas

The fundamental nature of dark matter is entirely unknown. A compelling candidate is Twin Higgs mirror matter, invisible hidden-sector cousins of the Standard Model particles and forces. This predicts mirror neutron stars made entirely of…

High Energy Astrophysical Phenomena · Physics 2023-05-12 Maurício Hippert , Jack Setford , Hung Tan , David Curtin , Jacquelyn Noronha-Hostler , Nicolas Yunes

Well known scaling laws among the structural properties of the dark and the luminous matter in disc systems are too complex to be arisen by two inert components that just share the same gravitational field. This brings us to critically…

Astrophysics of Galaxies · Physics 2020-03-10 Paolo Salucci , Nicola Turini

The cold dark matter model successfully explains both the emergence and evolution of cosmic structures on large scales and, when we include a cosmological constant, the properties of the homogeneous and isotropic Universe. However, the cold…

Cosmology and Nongalactic Astrophysics · Physics 2020-08-04 Ivan de Martino , Sankha S. Chakrabarty , Valentina Cesare , Arianna Gallo , Luisa Ostorero , Antonaldo Diaferio

These lecture notes aim to provide an introduction to dark matter from the perspective of astrophysics/cosmology. We start with a rapid overview of cosmology, including the evolution of the Universe, its thermal history and structure…

High Energy Physics - Phenomenology · Physics 2022-01-26 Anne M. Green

The emerging cosmological picture is of a spatially flat universe composed predominantly of three components: ordinary baryons ($\Omega_B \approx 0.05$), non-baryonic dark matter ($\Omega_{Dark} \approx 0.22$) and dark energy…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. Foot , R. R. Volkas

I give a review of the development of the concept of dark matter. The dark matter story passed through several stages from a minor observational puzzle to a major challenge for theory of elementary particles. Modern data suggest that dark…

Cosmology and Nongalactic Astrophysics · Physics 2018-03-14 J. Einasto

In this article we address the mystery of dark matter. We expound the various evidences, astrophysical and cosmological, leading to hypothesize the existence of an invisible form of matter, whose attempts at detecting it have so far all…

General Relativity and Quantum Cosmology · Physics 2024-10-15 Sergio Luigi Cacciatori , Vittorio Gorini , Federico Re

The nature of dark matter is one of the open problems of the Standard Model of particle physics. Despite the great experimental efforts, we have not yet found a positive signal of its interactions with ordinary matter. One possible…

High Energy Physics - Phenomenology · Physics 2019-04-09 M. Blennow , E. Fernández-Martínez , A. Olivares-Del Campo , S. Pascoli , S. Rosauro-Alcaraz , A. V. Titov

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…

High Energy Physics - Phenomenology · Physics 2017-08-23 Philippe Jetzer

It has been revealed using microlensing that a considerable part, possibly more than half, of the dark matter in the halo of our Galaxy consists of objects with a mass spectrum ranging from 0.05 to 0.8 of the solar mass. What is the nature…

Astrophysics · Physics 2007-05-23 A. V. Gurevich , K. P. Zybin , V. A. Sirota

It has been argued that the observed core density profile of galaxies is inconsistent with having a dark matter particle that is collisionless and alternative dark matter candidates which are self interacting may explain observations…

High Energy Physics - Phenomenology · Physics 2009-11-07 R. N. Mohapatra , S. Nussinov , V. L. Teplitz

The problems of simple elementary weakly interacting massive particles (WIMPs) appeal to extend the physical basis for nonbaryonic dark matter. Such extension involves more sophisticated dark matter candidates from physics beyond the…

High Energy Physics - Phenomenology · Physics 2019-04-30 Vitaly Beylin , Maxim Yu. Khlopov , Vladimir Kuksa , Nikolay Volchanskiy

Many independent high-resolution simulations of structure formation in cold dark matter models show that galactic halos should have singular core profiles. This is in stark contrast with observations of both low- and high-surface brightness…

Astrophysics · Physics 2007-05-23 Steen Hannestad

We present new fast numerical simulations of cosmic microwave background and large scale structure in the case in which the cosmological dark matter is made entirely or partly of mirror matter. We consider scalar adiabatic primordial…

Cosmology and Nongalactic Astrophysics · Physics 2014-01-24 Paolo Ciarcelluti , Quentin Wallemacq

Rotation curve measurements provided the first strong indication that a significant fraction of matter in the Universe is non-baryonic. Since then, a tremendous amount of progress has been made on both the theoretical and experimental…

High Energy Physics - Phenomenology · Physics 2016-12-21 Mariangela Lisanti

Dark matter in the universe seems to be one of the most important puzzles science has to face in this moment. In this essay we point out that dark matter could be a spin-0 fundamental interaction of Nature rather than a simple particle.…

Astrophysics · Physics 2010-12-09 T. Matos , L. A. Urena-Lopez

These lectures are intended to provide a brief pedagogical review of dark matter for the newcomer to the subject. We begin with a discussion of the astrophysical evidence for dark matter. The standard weakly-interacting massive particle…

Cosmology and Nongalactic Astrophysics · Physics 2009-07-14 Guido D'Amico , Marc Kamionkowski , Kris Sigurdson

I give a review of the development of the concept of dark matter. The dark matter story passed through several stages from a minor observational puzzle to a major challenge for theory of elementary particles. Modern data suggest that dark…

Cosmology and Nongalactic Astrophysics · Physics 2013-08-13 Jaan Einasto