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The existence of dark matter is now well established by several indirect experiments. Several candidates for dark matter has also been proposed. However, the dark matter can just be like our ordinary matter in a parallel Universe with both…

High Energy Physics - Phenomenology · Physics 2014-10-28 Shreyashi Chakdar , Kirtiman Ghosh , S. Nandi

Underground laboratories host two kind of experiments at the frontier of our knowledge in Particle Physics, Astrophysics and Cosmology: the direct detection of the Dark Matter of the Universe and the search for the Neutrinoless Double Beta…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-17 Igor G. Irastorza

We construct the New Minimal Standard Model that incorporates the new discoveries of physics beyond the Minimal Standard Model (MSM): Dark Energy, non-baryonic Dark Matter, neutrino masses, as well as baryon asymmetry and cosmic inflation,…

High Energy Physics - Phenomenology · Physics 2009-09-29 Hooman Davoudiasl , Ryuichiro Kitano , Tianjun Li , Hitoshi Murayama

Astrophysical observations indicate that about 23% of the energy density of the universe is in the form of non-baryonic particles beyond the standard model of particle physics. One exciting and well motivated candidate is the lightest…

Astrophysics · Physics 2008-11-26 Richard W. Schnee

I begin by briefly reviewing the evidence for the existence of Dark Matter (DM), emphasizing that {\em many} observations, at length scales between kpc (the size of the smallest galaxies) and Gpc (the Hubble radius) can be described by the…

High Energy Physics - Phenomenology · Physics 2018-11-16 Manuel Drees

This is the third out of five chapters of the final report [1] of the Workshop on Physics at HL-LHC, and perspectives on HE-LHC [2]. It is devoted to the study of the potential, in the search for Beyond the Standard Model (BSM) physics, of…

High Energy Physics - Phenomenology · Physics 2019-08-14 X. Cid Vidal , M. D'Onofrio , P. J. Fox , R. Torre , K. A. Ulmer , A. Aboubrahim , A. Albert , J. Alimena , B. C. Allanach , C. Alpigiani , M. Altakach , S. Amoroso , J. K. Anders , J. Y. Araz , A. Arbey , P. Azzi , I. Babounikau , H. Baer , M. J. Baker , D. Barducci , V. Barger , O. Baron , L. Barranco Navarro , M. Battaglia , A. Bay , D. Bhatia , S. Biswas , D. Bloch , D. Bogavac , C. Borschensky , M. K. Bugge , D. Buttazzo , G. Cacciapaglia , L. Cadamuro , A. Calandri , D. A. Camargo , A. Canepa , L. Carminati , S. Carrá , C. A. Carrillo Montoya , A. Carvalho Antunes De Oliveira , F. L. Castillo , V. Cavaliere , D. Cavalli , C. Cecchi , A. Celis , A. Cerri , G. S. Chahal , A. Chakraborty , S. V. Chekanov , H. J. Cheng , J. T. Childers , M. Cirelli , O. Colegrove , G. Corcella , M. Corradi , M. J. Costa , R. Covarelli , N. P. Dang , A. Deandrea , S. De Curtis , H. De la Torre , L. Delle Rose , D. Del Re , A. Demela , S. Demers , R. Dermisek , A. De Santo , K. Deshpande , B. Dey , J. Donini , A. K. Duncan , V. Dutta , C. Escobar , L. Fanó , G. Ferretti , J. Fiaschi , O. Fischer , T. Flacke , E. D. Frangipane , M. Frank , G. Frattari , D. Frizzell , E. Fuchs , B. Fuks , E. Gabrielli , J. Gainer , Y. Gao , J. E. García Navarro , M. H. Genest , S. Giagu , G. F. Giudice , J. Goh , M. Gouzevitch , P. Govoni , A. Greljo , A. Grohsjean , A. Gurrola , G. Gustavino , C. Guyot , C. B. Gwilliam , S. Ha , U. Haisch , J. Haller , T. Han , D. Hayden , M. Heikinheimo , U. Heintz , C. Helsens , K. Hoepfner , J. M. Hogan , K. Huitu , P. Ilten , V. Ippolito , A. Ismail , A. M. Iyer , Sa. Jain , D. O. Jamin , L. Jeanty , T. Jezo , W. Johns , A. Kalogeropoulos , J. Karancsi , Y. Kats , H. Keller , A. Khanov , J. Kieseler , B. Kim , M. S. Kim , Y. G. Kim , M. Klasen , M. D. Klimek , R. Kogler , J. R. Komaragiri , M. Krämer , S. Kubota , A. K. Kulesza , S. Kulkarni , T. Lari , A. Ledovskoy , G. R. Lee , L. Lee , S. W. Lee , R. Leonardi , R. Les , I. M. Lewis , Q. Li , T. Li , I. T. Lim , S. H. Lim , K. Lin , Z. Liu , K. Long , M. Low , E. Lunghi , D. Madaffari , F. Mahmoudi , D. Majumder , S. Malvezzi , M. L. Mangano , E. Manoni , X. Marcano , A. Mariotti , M. Marjanovic , D. Marlow , J. Martin Camalich , P. Matorras Cuevas , M. McCullough , E. F. McDonald , J. Mejia Guisao , B. Mele , F. Meloni , I. -A. Melzer-Pellmann , C. Merlassino , A. B. Meyer , E. Michielin , A. J. Miller , L. Mittnacht , S. Mondal , S. Moretti , S. Mukhopadhyay , B. P. Nachman , K. Nam , M. Narain , M. Nardecchia , P. Nath , J. Navarro-González , A. Nisati , T. Nitta , D. L. Noel , M. M. Nojiri , J. P. Ochoa-Ricoux , H. Oide , M. L. Ojeda , S. Pagan Griso , E. Palencia Cortezon , O. Panella , P. Pani , L. Panizzi , L. Panwar , C. B. Park , J. Pazzini , K. Pedro , M. M. Perego , L. Perrozzi , B. A. Petersen , A. Pierce , G. Polesello , A. Policicchio , C. J. Potter , P. Pralavorio , M. Presilla , J. Proudfoot , F. S. Queiroz , G. Ramirez-Sanchez , D. Redigolo , A. Reimers , S. Resconi , M. Rimoldi , J. C. Rivera Vergara , T. Rizzo , C. Rogan , F. Romeo , R. Rosten , R. Ruiz , J. Ruiz-Alvarez , J. A. Sabater Iglesias , B. Safarzadeh Samani , S. Sagir , M. Saito , S. Saito , F. Sala , C. Salazar , A. Savin , R. Sawada , S. Sawant , I. Schienbein , M. Schlaffer , B. Schneider , S. C. Schuler , C. D. Sebastiani , S. Sekmen , M. Selvaggi , D. Sengupta , H. Serce , H. Serodio , L. Sestini , B. Shakya , B. Shams Es Haghi , P. Sheldon , S. Shin , F. Simonetto , L. Soffi , M. Spannowsky , J. Stupak , M. J. Sullivan , M. Sunder , Y. Takahashi , X. Tata , H. Teagle , K. Terashi , A. Tesi , A. Thamm , K. Tobioka , P. Tornambe , F. Trovato , D. Tsiakkouri , F. C. Ungaro , A. Urbano , E. Usai , N. Vanegas , L. Vaslin , C. Vázquez Sierra , I. Vivarelli , M. Vranjes Milosavljevic , H. Waltari , R. Wang , X. Wang , M. S. Weber , C. Weiland , M. Wielers , J. M. Williams , S. Willocq , D. Xu , K. Yagyu , E. Yazgan , R. Ye , H. D. Yoo , T. You , F. Yu , G. Zevi Della Porta , W. Zhang , C. Zhu , X. Zhuang , J. Zobec , J. Zupan , J. Zurita

The nature of dark matter remains a central question in particle physics, cosmology, and astrophysics. The prevailing hypothesis postulates that dark matter consists of particles that interact only weakly with Standard Model particles.…

High Energy Physics - Phenomenology · Physics 2023-12-01 Leon M. G. de la Vega , R. Ferro-Hernandez , A. García-Viltres , Eduardo Peinado , E. Vázquez-Jáuregui

In this report we summarize the many dark matter searches currently being pursued through four complementary approaches: direct detection, indirect detection, collider experiments, and astrophysical probes. The essential features of broad…

Perturbative gauge coupling unification in realistic superstring models suggests the existence of additional heavy down-type quarks, beyond the minimal supersymmetric standard model. The mass scale of the heavy down-type quarks is…

High Energy Physics - Phenomenology · Physics 2009-10-28 Sanghyeon Chang , Claudio Coriano , Alon E. Faraggi

Cosmology now provides unambiguous, quantitative evidence for new particle physics. I discuss the implications of cosmology for supersymmetry and vice versa. Topics include: motivations for supersymmetry; supersymmetry breaking; dark…

High Energy Physics - Phenomenology · Physics 2009-11-10 Jonathan L. Feng

This review briefly describes light dark matter searches performed by the BABAR experiment. Although dark matter candidates have traditionally been associated with heavy particles appearing in extensions of the Standard Model, a lighter…

High Energy Physics - Experiment · Physics 2012-06-04 B. Echenard

A hidden sector that kinetically mixes with the Minimal Supersymmetric Standard Model provides simple and well-motivated dark matter candidates that possess many of the properties of a traditional weakly interacting massive particle (WIMP).…

High Energy Physics - Phenomenology · Physics 2020-10-21 Patrick Barnes , Zachary Johnson , Aaron Pierce , Bibhushan Shakya

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

We review scenarios of physics beyond the Standard Model in which the top quark plays a special role. Models that aim at the stabilization of the weak scale are presented together with the specific phenomenology of partner states that are…

High Energy Physics - Phenomenology · Physics 2023-01-12 Roberto Franceschini

The last decade has seen unprecedented effort in dark matter model building at all mass scales coupled with the design of numerous new detection strategies. Transformative advances in quantum technologies have led to a plethora of new…

High Energy Physics - Experiment · Physics 2022-03-29 D. Antypas , A. Banerjee , C. Bartram , M. Baryakhtar , J. Betz , J. J. Bollinger , C. Boutan , D. Bowring , D. Budker , D. Carney , G. Carosi , S. Chaudhuri , S. Cheong , A. Chou , M. D. Chowdhury , R. T. Co , J. R. Crespo López-Urrutia , M. Demarteau , N. DePorzio , A. V. Derbin , T. Deshpande , M. D. Chowdhury , L. Di Luzio , A. Diaz-Morcillo , J. M. Doyle , A. Drlica-Wagner , A. Droster , N. Du , B. Döbrich , J. Eby , R. Essig , G. S. Farren , N. L. Figueroa , J. T. Fry , S. Gardner , A. A. Geraci , A. Ghalsasi , S. Ghosh , M. Giannotti , B. Gimeno , S. M. Griffin , D. Grin , D. Grin , H. Grote , J. H. Gundlach , M. Guzzetti , D. Hanneke , R. Harnik , R. Henning , V. Irsic , H. Jackson , D. F. Jackson Kimball , J. Jaeckel , M. Kagan , D. Kedar , R. Khatiwada , S. Knirck , S. Kolkowitz , T. Kovachy , S. E. Kuenstner , Z. Lasner , A. F. Leder , R. Lehnert , D. R. Leibrandt , E. Lentz , S. M. Lewis , Z. Liu , J. Manley , R. H. Maruyama , A. J. Millar , V. N. Muratova , N. Musoke , S. Nagaitsev , O. Noroozian , C. A. J. O'Hare , J. L. Ouellet , K. M. W. Pappas , E. Peik , G. Perez , A. Phipps , N. M. Rapidis , J. M. Robinson , V. H. Robles , K. K. Rogers , J. Rudolph , G. Rybka , M. Safdari , M. Safdari , M. S. Safronova , C. P. Salemi , P. O. Schmidt , T. Schumm , A. Schwartzman , J. Shu , M. Simanovskaia , J. Singh , S. Singh , M. S. Smith , W. M. Snow , Y. V. Stadnik , C. Sun , A. O. Sushkov , T. M. P. Tait , V. Takhistov , D. B. Tanner , D. J. Temples , P. G. Thirolf , J. H. Thomas , M. E. Tobar , O. Tretiak , Y. -D. Tsai , J. A. Tyson , M. Vandegar , S. Vermeulen , L. Visinelli , E. Vitagliano , Z. Wang , D. J. Wilson , L. Winslow , S. Withington , M. Wooten , J. Yang , J. Ye , B. A. Young , F. Yu , M. H. Zaheer , T. Zelevinsky , Y. Zhao , K. Zhou

Despite the fact that dark matter constitutes one of the cornerstones of the standard cosmological paradigm, its existence has so far only been inferred from astronomical observations and its microscopic nature remains elusive. Theoretical…

High Energy Physics - Phenomenology · Physics 2022-11-28 Spyros Argyropoulos , Oleg Brandt , Ulrich Haisch

The detection of the theoretically expected dark matter is central to particle physics and cosmology. Current fashionable supersymmetric models provide a natural dark matter candidate which is the lightest supersymmetric particle (LSP). The…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. D. Vergados

In this Report we discuss the four complementary searches for the identity of dark matter: direct detection experiments that look for dark matter interacting in the lab, indirect detection experiments that connect lab signals to dark matter…

Several lines of evidence suggest that some of the dark matter may be non-baryonic: the non-detection of various plausible baryonic candidates for dark matter inferred, e.g., from galaxy rotation curves and from cluster of galaxy velocity…

Astrophysics · Physics 2007-05-23 David N. Spergel

One of the most popular classes of candidates for dark matter are Weakly Interacting Massive Particles (WIMPs), i.e. particles possessing masses and couplings falling roughly within the electroweak scale. Apart from offering a natural…

High Energy Physics - Phenomenology · Physics 2011-06-21 Andreas Goudelis