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Dark matter is the name assigned to one of the most important contemporary challenges that fundamental physics research is facing. In recent years, the hypothesis that dark matter might be "light" is gaining interest. Following this idea,…

High Energy Physics - Phenomenology · Physics 2022-01-10 P. Achenbach , L. Doria , M. Battaglieri

Dark matter is among the most important open problems in both astrophysics and particle physics. We review the status of art of dark matter search at theoretical and experimental level discussing also alternative hypotheses.

Cosmology and Nongalactic Astrophysics · Physics 2011-11-09 S. Capozziello , L. Consiglio , M. De Laurentis , G. De Rosa , C. Di Donato

In this article, I summarize and discuss the body of evidence which has accumulated in favor of dark matter in the form of approximately 10 GeV particles. This evidence includes the spectrum and angular distribution of gamma rays from the…

Cosmology and Nongalactic Astrophysics · Physics 2012-01-09 Dan Hooper

It is well known that dark matter density measurements, indirect and direct detection experiments, importantly complement the LHC in setting strong constraints on new physics scenarios. Yet, dark matter searches are subject to limitations…

High Energy Physics - Phenomenology · Physics 2017-10-11 G. Robbins , F. Mahmoudi , A. Arbey , M. Boudaud

Indirect dark matter searches are briefly reviewed. Current experimental data from satellites and Cherenkov telescopes searching for antimatter and gamma rays in galactic and extragalactic regions, are compared with predictions from…

High Energy Physics - Phenomenology · Physics 2012-03-06 Carlos Munoz

Direct searches for Dark Matter are experiment dedicated to the observation of the energetic recoiling ions produced by the scattering of WIMP particles from our galactic halo on terrestrial targets. The status and prospects of some…

High Energy Astrophysical Phenomena · Physics 2009-06-24 J. Gascon

Monochromatic gamma-ray signals constitute a potential smoking gun signature for annihilating or decaying dark matter particles that could relatively easily be distinguished from astrophysical or instrumental backgrounds. We provide an…

High Energy Physics - Phenomenology · Physics 2024-07-24 S. Abe , J. Abhir , A. Abhishek , F. Acero , A. Acharyya , R. Adam , A. Aguasca-Cabot , I. Agudo , A. Aguirre-Santaella , J. Alfaro , R. Alfaro , N. Alvarez-Crespo , R. Alves Batista , J. -P. Amans , E. Amato , G. Ambrosi , L. Angel , C. Aramo , C. Arcaro , T. T. H. Arnesen , L. Arrabito , K. Asano , Y. Ascasibar , J. Aschersleben , H. Ashkar , M. Backes , A. Baktash , C. Balazs , M. Balbo , A. Baquero Larriva , V. Barbosa Martins , U. Barres de Almeida , J. A. Barrio , I. Batković , R. Batzofin , J. Baxter , J. Becerra González , G. Beck , W. Benbow , D. Berge , E. Bernardini , J. Bernete , K. Bernlöhr , A. Berti , B. Bertucci , P. Bhattacharjee , S. Bhattacharyya , C. Bigongiari , A. Biland , E. Bissaldi , J. Biteau , O. Blanch , J. Blazek , F. Bocchino , C. Boisson , J. Bolmont , G. Bonnoli , A. Bonollo , P. Bordas , Z. Bosnjak , E. Bottacini , M. Böttcher , T. Bringmann , E. Bronzini , R. Brose , A. M. Brown , G. Brunelli , A. Bulgarelli , T. Bulik , I. Burelli , L. Burmistrov , M. Burton , M. Buscemi , T. Bylund , J. Cailleux , A. Campoy-Ordaz , B. K. Cantlay , G. Capasso , A. Caproni , R. Capuzzo-Dolcetta , P. Caraveo , S. Caroff , A. Carosi , R. Carosi , E. Carquin , M. -S. Carrasco , F. Cassol , L. Castaldini , N. Castrejon , A. J. Castro-Tirado , D. Cerasole , M. Cerruti , P. M. Chadwick , S. Chaty , A. W. Chen , M. Chernyakova , A. Chiavassa , J. Chudoba , L. Chytka , G. M. Cicciari , A. Cifuentes , C. H. Coimbra Araujo , M. Colapietro , V. Conforti , F. Conte , J. L. Contreras , A. Costa , H. Costantini , G. Cotter , P. Cristofari , O. Cuevas , Z. Curtis-Ginsberg , G. D'Amico , F. D'Ammando , S. Dai , M. Dalchenko , F. Dazzi , A. De Angelis , M. de Bony de Lavergne , V. De Caprio , E. M. de Gouveia Dal Pino , B. De Lotto , M. De Lucia , R. de Menezes , M. de Naurois , V. de Souza , L. del Peral , M. V. del Valle , A. G. Delgado Giler , J. Delgado Mengual , C. Delgado , M. Dell'aiera , D. della Volpe , D. Depaoli , T. Di Girolamo , A. Di Piano , F. Di Pierro , R. Di Tria , L. Di Venere , C. Díaz , S. Diebold , A. Dinesh , J. Djuvsland , R. M. Dominik , D. Dominis Prester , A. Donini , D. Dorner , J. Dörner , M. Doro , J. -L. Dournaux , C. Duangchan , C. Dubos , L. Ducci , V. V. Dwarkadas , J. Ebr , C. Eckner , K. Egberts , S. Einecke , D. Elsässer , G. Emery , M. Errando , C. Escanuela , P. Escarate , M. Escobar Godoy , J. Escudero , P. Esposito , S. Ettori , D. Falceta-Goncalves , E. Fedorova , S. Fegan , Q. Feng , G. Ferrand , F. Ferrarotto , E. Fiandrini , A. Fiasson , M. Filipovic , V. Fioretti , M. Fiori , L. Foffano , L. Font Guiteras , G. Fontaine , S. Fröse , Y. Fukazawa , Y. Fukui , A. Furniss , G. Galanti , G. Galaz , C. Galelli , S. Gallozzi , V. Gammaldi , M. Garczarczyk , C. Gasbarra , D. Gasparrini , A. Ghalumyan , F. Gianotti , M. Giarrusso , J. G. Giesbrecht Formiga Paiva , N. Giglietto , F. Giordano , R. Giuffrida , J. -F. Glicenstein , J. Glombitza , P. Goldoni , J. M. González , M. M. González , J. Goulart Coelho , T. Gradetzke , J. Granot , D. Grasso , R. Grau , L. Gréaux , D. Green , J. G. Green , G. Grolleron , L. M. V. Guedes , O. Gueta , J. Hackfeld , D. Hadasch , P. Hamal , W. Hanlon , S. Hara , V. M. Harvey , T. Hassan , K. Hayashi , B. Heß , L. Heckmann , M. Heller , S. Hernández Cadena , O. Hervet , J. Hinton , N. Hiroshima , B. Hnatyk , R. Hnatyk , W. Hofmann , J. Holder , D. Horan , P. Horvath , T. Hovatta , M. Hrabovsky , D. Hrupec , M. Iarlori , T. Inada , F. Incardona , S. Inoue , Y. Inoue , F. Iocco , M. Iori , K. Ishio , M. Jamrozy , P. Janecek , F. Jankowsky , P. Jean , J. Jimenez Quiles , W. Jin , C. Juramy-Gilles , J. Jurysek , M. Kagaya , O. Kalekin , V. Karas , H. Katagiri , J. Kataoka , S. Kaufmann , D. Kazanas , D. Kerszberg , D. B. Kieda , T. Kleiner , G. Kluge , Y. Kobayashi , K. Kohri , N. Komin , P. Kornecki , K. Kosack , G. Kowal , H. Kubo , J. Kushida , A. La Barbera , N. La Palombara , M. Láinez , A. Lamastra , J. Lapington , P. Laporte , S. Lazarević , J. Lazendic-Galloway , M. Lemoine-Goumard , J. -P. Lenain , F. Leone , E. Leonora , G. Leto , E. Lindfors , M. Linhoff , I. Liodakis , A. Lipniacka , S. Lombardi , F. Longo , R. López-Coto , M. López-Moya , A. López-Oramas , S. Loporchio , J. Lozano Bahilo , P. L. Luque-Escamilla , O. Macias , P. Majumdar , M. Mallamaci , D. Malyshev , D. Mandat , G. Manicò , M. Mariotti , I. Márquez , P. Marquez , G. Marsella , J. Martí , G. A. Martínez , M. Martínez , O. Martinez , C. Marty , A. Mas-Aguilar , M. Mastropietro , D. Mazin , S. Menchiari , E. Mestre , J. -L. Meunier , D. M. -A. Meyer , M. Meyer , D. Miceli , M. Miceli , M. Michailidis , J. Michałowski , T. Miener , J. M. Miranda , A. Mitchell , M. Mizote , T. Mizuno , R. Moderski , M. Molero , C. Molfese , E. Molina , T. Montaruli , A. Moralejo , D. Morcuende , A. Morselli , E. Moulin , V. Moya Zamanillo , K. Munari , T. Murach , A. Muraczewski , H. 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Zhang , V. I. Zhdanov , K. Ziętara , M. Živec , J. Zuriaga-Puig

The detection of exotic cosmic rays due to pair annihilation of dark matter particles in the Milky Way halo is a viable techniques to search for supersymmetric dark matter candidates. The study of the spectrum of gamma-rays, antiprotons and…

The Fermi Gamma-Ray Space Telescope, successfully launched on June 11th, 2008, is the next generation satellite experiment for high-energy gamma-ray astronomy. The main instrument, the Fermi Large Area Telescope (LAT), with a wide field of…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Christine Meurer

The presence of dark matter in the universe is nowadays supported by a substantial set of astronomical and cosmological observations. A large amount of dark matter is expected in the Galactic Center (GC) region. Thanks also to its…

High Energy Astrophysical Phenomena · Physics 2016-09-22 V. Lefranc , E. Moulin

Gamma-ray observations of Milky Way dwarf galaxies have been used to place stringent constraints on the dark matter's annihilation cross section. In this paper, we evaluate the sensitivity of the proposed Advanced Particle-astrophysics…

High Energy Astrophysical Phenomena · Physics 2023-08-31 Fei Xu , Dan Hooper

Direct dark matter detection experiments search for rare signals induced by hypothetical, galactic dark matter particles in low-background detectors operated deep underground. I will briefly review the direct detection principles, the…

Instrumentation and Methods for Astrophysics · Physics 2025-12-30 Laura Baudis

We provide a status report on our search for dark matter in our Galaxy in the form of massive compact halo objects (or Machos), using gravitational microlensing of background stars. This search uses a very large format CCD camera on the…

Many results from astrophysical observations point to a 27% contribution of non-baryonic dark matter to the mass-energy budget of the universe. Although still elusive, strongly motivated candidates in form of weakly interacting massive…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Matthieu Kieffer , Knut Dundas Mora , Jan Conrad , Christian Farnier , A. Jacholkowska , Johannes Veh , Aion Viana

Dark matter (DM) is largely believed to be the dominant component of the matter content of the Universe. Astronomical measurements can be utilized to search for Standard Model (SM) annihilation or decay products of DM, complementing direct…

High Energy Astrophysical Phenomena · Physics 2021-08-16 Chiara Giuri

In this work we derive the first theoretical prediction of the cross-correlation signal between the unresolved gamma-ray background and the 21-cm line originated by the spin-flip transition of neutral hydrogen atoms, by taking as benchmark…

Cosmology and Nongalactic Astrophysics · Physics 2020-05-20 Elena Pinetti

For some time, the Draco dwarf spheroidal galaxy has garnered interest as a possible source for the indirect detection of dark matter. Its large mass-to-light ratio and relative proximity to the Earth provide favorable conditions for the…

There is currently vast evidence for Dark Matter (DM) from astronomical observations. However, in spite of tremendous efforts by large experimental groups, there is no confirmed direct detection of the dark matter in our galaxy. Recent…

Instrumentation and Methods for Astrophysics · Physics 2014-11-20 Juan Estrada

In this review statistical issues appearing in astrophysical searches for particle dark matter, i.e. indirect detection (dark matter annihilating into standard model particles) or direct detection (dark matter particles scattering in deep…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-22 Jan Conrad

In this thesis, I study the expected direct and indirect detection signals of dark matter. More precisely, I study three aspects of dark matter; I use hydrodynamic simulations to extract properties of weakly interacting dark matter that are…

High Energy Physics - Phenomenology · Physics 2017-06-06 Lina Necib