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Related papers: Dark Matter Astrophysics

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The identification of a solution to the dark matter problem has many arrows to its bow: if dark matter is a new elementary particle, both laboratory experiments and astrophysics can bring relevant and complementary pieces of information,…

High Energy Astrophysical Phenomena · Physics 2017-01-17 N. Fornengo

In these lectures we first concentrate on the cosmological problems which, hopefully, have to do with the new physics to be probed at the LHC: the nature and origin of dark matter and generation of matter-antimatter asymmetry. We give…

Cosmology and Nongalactic Astrophysics · Physics 2015-04-15 V. A. Rubakov

We study a superweakly interacting dark matter particle motivated by minimal walking technicolor theories. Our WIMP is a mixture of a sterile state and a state with the charges of a standard model fourth family neutrino. We show that the…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 Kimmo Kainulainen , Kimmo Tuominen , Jussi Virkajarvi

An ever-increasing body of evidence suggests that weakly interacting massive particles (WIMPs) constitute the bulk of the matter in the Universe. Experimental data, dimensional analysis and Standard Model particle physics are sufficient to…

High Energy Physics - Phenomenology · Physics 2007-05-23 F. Halzen

Weakly interacting massive particles (WIMPs) can be gravitationally captured by the Sun and trapped in its core. The annihilation of those WIMPs into Standard Model particles produces a spectrum of neutrinos whose energy distribution is…

High Energy Astrophysical Phenomena · Physics 2019-09-20 Carlos A. Argüelles , Ali Kheirandish , Jeffrey Lazar , Qinrui Liu

Cold dark matter may be made of superweakly-interacting massive particles, superWIMPs, that naturally inherit the desired relic density from late decays of metastable WIMPs. Well-motivated examples are weak-scale gravitinos in supergravity…

High Energy Physics - Phenomenology · Physics 2008-11-26 Jonathan L. Feng , Arvind Rajaraman , Fumihiro Takayama

Introduction to the meaning of dark matter and a few historical gestures. What it is? By what the dark matter is formed? Experimental phenomenon evidences and relative explanation under the point of view of the physics of the elementary…

Astrophysics · Physics 2007-05-23 Azzurra Auteri

Particles weakly interacting with ordinary matter, with an associated mass of the order of an atomic nucleus (WIMPs), are plausible candidates for Dark Matter. The direct detection of an elastic collision of a target nuclei induced by one…

Instrumentation and Methods for Astrophysics · Physics 2016-08-01 C. Couturier , O. Guillaudin , F. Naraghi , Q. Riffard , D. Santos , N. Sauzet , P. Colas , E. Ferrer Ribas , I. Giomataris , J. Busto , D. Fouchez , C. Tao , N. Zhou

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…

Cosmology and Nongalactic Astrophysics · Physics 2020-08-28 Paolo Salucci , Nicola Turini , Chiara Di Paolo

Despite significant experimental sensitivity to point-like, weakly interacting particles at the electroweak mass scale, dark matter has not been found yet. This could hint at a more complex dark sector with multiple states or composite dark…

High Energy Physics - Phenomenology · Physics 2023-01-02 Juri Smirnov

One of the great mysteries of contemporary science is dark matter, an exotic substance of unknown nature that, in theory, makes up about 27\% of the total mass-energy density of the universe, and which does not appear to emit, absorb, or…

Physics Education · Physics 2024-06-25 Jorge Pinochet

(Shortened) Weakly Interacting Massive Particles are often said to be the best Dark Matter candidates. Studies have shown however that rather large Dark Matter-photon or Dark Matter-baryon interactions could be allowed by cosmology. Here we…

Astrophysics · Physics 2009-11-10 Celine Boehm , Richard Schaeffer

Dark matter may be composed of superWIMPs, superweakly-interacting massive particles produced in the late decays of other particles. We focus here on the well-motivated supersymmetric example of gravitino LSPs. Gravitino superWIMPs share…

High Energy Physics - Phenomenology · Physics 2007-05-23 Jonathan L. Feng , Arvind Rajaraman , Bryan T. Smith , Shufang Su , Fumihiro Takayama

Astrophysical observations currently provide the only robust, empirical measurements of dark matter. In the coming decade, astrophysical observations will guide other experimental efforts, while simultaneously probing unique regions of dark…

Cosmology and Nongalactic Astrophysics · Physics 2019-03-12 Keith Bechtol , Alex Drlica-Wagner , Kevork N. Abazajian , Muntazir Abidi , Susmita Adhikari , Yacine Ali-Haïmoud , James Annis , Behzad Ansarinejad , Robert Armstrong , Jacobo Asorey , Carlo Baccigalupi , Arka Banerjee , Nilanjan Banik , Charles Bennett , Florian Beutler , Simeon Bird , Simon Birrer , Rahul Biswas , Andrea Biviano , Jonathan Blazek , Kimberly K. Boddy , Ana Bonaca , Julian Borrill , Sownak Bose , Jo Bovy , Brenda Frye , Alyson M. Brooks , Matthew R. Buckley , Elizabeth Buckley-Geer , Esra Bulbul , Patricia R. Burchat , Cliff Burgess , Francesca Calore , Regina Caputo , Emanuele Castorina , Chihway Chang , George Chapline , Eric Charles , Xingang Chen , Douglas Clowe , Johann Cohen-Tanugi , Johan Comparat , Rupert A. C. Croft , Alessandro Cuoco , Francis-Yan Cyr-Racine , Guido D'Amico , Tamara M Davis , William A. Dawson , Axel de la Macorra , Eleonora Di Valentino , Ana Díaz Rivero , Seth Digel , Scott Dodelson , Olivier Doré , Cora Dvorkin , Christopher Eckner , John Ellison , Denis Erkal , Arya Farahi , Christopher D. Fassnacht , Pedro G. Ferreira , Brenna Flaugher , Simon Foreman , Oliver Friedrich , Joshua Frieman , Juan García-Bellido , Eric Gawiser , Martina Gerbino , Maurizio Giannotti , Mandeep S. S. Gill , Vera Gluscevic , Nathan Golovich , Satya Gontcho A Gontcho , Alma X. González-Morales , Daniel Grin , Daniel Gruen , Andrew P. Hearin , David Hendel , Yashar D. Hezaveh , Christopher M. Hirata , Renee Hložek , Shunsaku Horiuchi , Bhuvnesh Jain , M. James Jee , Tesla E. Jeltema , Marc Kamionkowski , Manoj Kaplinghat , Ryan E. Keeley , Charles R. Keeton , Rishi Khatri , Sergey E. Koposov , Savvas M. Koushiappas , Ely D. Kovetz , Ofer Lahav , Casey Lam , Chien-Hsiu Lee , Ting S. Li , Michele Liguori , Tongyan Lin , Mariangela Lisanti , Marilena LoVerde , Jessica R. Lu , Rachel Mandelbaum , Yao-Yuan Mao , Samuel D. McDermott , Mitch McNanna , Michael Medford , P. Daniel Meerburg , Manuel Meyer , Mehrdad Mirbabayi , Siddharth Mishra-Sharma , Moniez Marc , Surhud More , John Moustakas , Julian B. Muñoz , Simona Murgia , Adam D. Myers , Ethan O. Nadler , Lina Necib , Laura Newburgh , Jeffrey A. Newman , Brian Nord , Erfan Nourbakhsh , Eric Nuss , Paul O'Connor , Andrew B. Pace , Hamsa Padmanabhan , Antonella Palmese , Hiranya V. Peiris , Annika H. G. Peter , Francesco Piacentni , Francesco Piacentini , Andrés Plazas , Daniel A. Polin , Abhishek Prakash , Chanda Prescod-Weinstein , Justin I. Read , Steven Ritz , Brant E. Robertson , Benjamin Rose , Rogerio Rosenfeld , Graziano Rossi , Lado Samushia , Javier Sánchez , Miguel A. Sánchez-Conde , Emmanuel Schaan , Neelima Sehgal , Leonardo Senatore , Hee-Jong Seo , Arman Shafieloo , Huanyuan Shan , Nora Shipp , Joshua D. Simon , Sara Simon , Tracy R. Slatyer , Anže Slosar , Srivatsan Sridhar , Albert Stebbins , Oscar Straniero , Louis E. Strigari , Tim M. P. Tait , Erik Tollerud , M. A. Troxel , J. Anthony Tyson , Cora Uhlemann , L. Arturo Urenña-López , Aprajita Verma , Ricardo Vilalta , Christopher W. Walter , Mei-Yu Wang , Scott Watson , Risa H. Wechsler , David Wittman , Weishuang Xu , Brian Yanny , Sam Young , Hai-Bo Yu , Gabrijela Zaharijas , Andrew R. Zentner , Joe Zuntz

We put constraints on asymmetric dark matter candidates with spin-dependent interactions based on the simple existence of white dwarfs and neutron stars in globular clusters. For a wide range of the parameters (WIMP mass and WIMP-nucleon…

High Energy Astrophysical Phenomena · Physics 2011-04-22 Chris Kouvaris , Peter Tinyakov

Since the daring intuition by Fritz Zwicky in 1933 about the existence of dark matter in the Universe, in spite of the extensive investigations pursued over a very long lapse of time, the nature of this matter and of its (other than…

High Energy Physics - Phenomenology · Physics 2019-10-30 Alessandro Bottino

There is plenty of evidence that most matter in the Universe is dark (non-luminous). Particle physics offers several possible explanations. In this talk I focus on cold dark matter; the most promising candidates are then axions and the…

High Energy Physics - Phenomenology · Physics 2008-02-03 Manuel Drees

These lectures have been given to particle physicists, mostly experimentalists and very briefly and at a pedestrian level review the problems of dark matter. The content of the lectures is the following: 1. Introduction. 2. Cosmological…

Astrophysics · Physics 2015-06-24 A. D. Dolgov

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…

High Energy Physics - Phenomenology · Physics 2015-06-12 Dieter Horns , Joerg Jaeckel , Axel Lindner , Andrei Lobanov , Javier Redondo , Andreas Ringwald

Astrophysics gives evidence for the existence of Dark Matter and puts constraints on its nature. The Cold Dark Matter model has become "standard" cosmology combined with a cosmological constant. There are indications that "Cold" Dark Matter…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Charling Tao
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