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3961por Laner Ogilvy, Christian“…Many theories predict candidates to the dark matter particles that are light enough to be produced at the LHC. …”
Publicado 2017
Enlace del recurso
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3962
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3963“…We study electroweak scale Dark Matter (DM) whose interactions with baryonic matter are mediated by a heavy anomalous Z′. …”
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3964por Narrias Villar, Daniel Isaac“…Several theories beyond the standard model predict new particles decaying resonantly into dibosons or coupling to dark matter particles. Jet substructure and boson tagging techniques play a crucial role in searches for dark matter and diboson resonances in boosted topologies with hadronic final states. …”
Publicado 2017
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3965por Wang, Rui“…Dark matter can be sought in complementary experiments: direct detection, indirect detection and colliders all contribute to a comprehensive set of searches for weakly interacting massive particles (WIMPs). …”
Publicado 2017
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3966“…We provide a Mathematica package, DirectDM, that takes as input the Wilson coefficients of the relativistic effective theory describing the interactions of dark matter with quarks, gluons and photons, and matches it onto an effective theory describing the interactions of dark matter with neutrons and protons. …”
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3967“…We study this effect for the double disk dark matter (DDDM) scenario, where a fraction of the dark matter is dissipative and settles into a thin disk. …”
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3968por Mukherjee, Maitreyee, Basu, Sumit, Chatterjee, Arghya, Chatterjee, Sandeep, Adhya, Souvik Priyam, Thakur, Sanchari, Nayak, Tapan K.“…We present the first estimates of isothermal compressibility ( kT ) of hadronic matter formed in relativistic nuclear collisions ( sNN=7.7 GeV to 2.76 TeV) using experimentally observed quantities. kT is related to the fluctuation in particle multiplicity, temperature, and volume of the system formed in the collisions. …”
Publicado 2017
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3969por Schioppa, Marco“…The ATLAS, CMS and LHCb collaborations searched for Dark Matter (DM) in events with long-lived particles. Many theories of physics beyond the Standard Model predict the existence of stable, neutral, weakly-interacting and massive particles that are putative Dark Matter candidates. …”
Publicado 2017
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3970por Alexeev, Boris V“…Non-Local Astrophysics: Dark Matter, Dark Energy and Physical Vacuum highlights the most significant features of non-local theory, a highly effective tool for solving many physical problems in areas where classical local theory runs into difficulties. …”
Publicado 2017
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3971por Pinna, Deborah“…The evidence of the existence of dark matter is provided by astrophysical observationsat different scales. …”
Publicado 2017
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3972por Fan, Tian-You“…The book systematically introduces the mathematical models and solutions of generalized hydrodynamics of soft-matter quasicrystals (SMQ). It provides methods for solving the initial-boundary value problems in these systems. …”
Publicado 2017
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3973“…In many of these cases, there are interesting prospects for discovering dark matter particles in Higgs or Z decays, as well as dark matter particles weighing ≳100 GeV. …”
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3974“…Combining this measurement with the existence of two-solar-mass stars, we generate a generic family of neutron-star-matter equations of state (EOSs) that interpolate between state-of-the-art theoretical results at low and high baryon density. …”
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3975
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3976“…A new dedicated experimental program is needed to test this mass range of primordial dark matter.…”
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3977“…The observation of an absorption feature in the 21-cm spectrum at redshift z≈17 implies bounds on dark-matter (DM) annihilations for a broad range of masses, given that significant heating of the intergalactic medium would have erased such a feature. …”
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3978
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3979“…We construct models with minimal field content that can simultaneously explain the muon g − 2 anomaly and give the correct dark matter relic abundance. These models fall into two general classes, whether or not the new fields couple to the Higgs. …”
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Enlace del recurso
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3980