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2781
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2782“…We find that over a large range of parameter space, a light neutralino can supply the correct relic abundance of dark matter either through resonant s-channel triplet scalar funnels or well tempering of the Bino with the triplet fermions. …”
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2783
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2784“…Supersymmetry is the best motivated and most thoroughly formulated and investigated model of New Physics which predicts a light Higgs boson and can explain dark matter. This paper discusses how the study of the Higgs boson connects with the search for supersymmetry and for dark matter at the LHC and at a future $e^+e^-$ collider and with dedicated underground dark matter experiments.…”
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2785
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2786por Crivellin, Andreas, Hoferichter, Martin, Procura, Massimiliano, Tunstall, Lewis C.“…In these proceedings we review the interplay between LHC searches for dark matter and direct detection experiments. For this purpose we consider two prime examples: the effective field theory (EFT) approach and the minimal supersymmetric standard model (MSSM). …”
Publicado 2015
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2787por Pinna, Deborah“…A search for dark matter produced in association with a top quark pair is presented. …”
Publicado 2015
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2788“…Recently, we have derived a novel and compact expression for how perturbations in the matter fields of the cosmological fluid can lead to deviations from the standard Friedmann equations. …”
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2789por Maire, Antonin“…Phase diagram (temperature, net baryon density) of QCD matter, ranging from regular nuclear matter to Quark-Gluon Plasma.…”
Publicado 2015
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2790
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2791por Blas, Diego, Floerchinger, Stefan, Garny, Mathias, Tetradis, Nikolaos, Wiedemann, Urs Achim“…Two-loop calculations of the matter power spectrum in the viscous theory lead to excellent agreement with $N$-body simulations up to scales $k=0.2 \, h/$Mpc. …”
Publicado 2015
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2792por Bagnaschi, E.A., Buchmueller, O., Cavanaugh, R., Citron, M., De Roeck, A., Dolan, M.J., Ellis, J.R., Flächer, H., Heinemeyer, S., Isidori, G., Malik, S., Martínez Santos, D., Olive, K.A., Sakurai, K., de Vries, K.J., Weiglein, G.“…Different mechanisms operate in various regions of the MSSM parameter space to bring the relic density of the lightest neutralino, neutralino_1, assumed here to be the LSP and thus the Dark Matter (DM) particle, into the range allowed by astrophysics and cosmology. …”
Publicado 2015
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Enlace del recurso
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2793“…Stringent limits on the interactions between dark matter (DM) and the standard model can be set by studying how initial-state or final-state particles recoil against missing transverse energy (MET). …”
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Enlace del recurso
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2794
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2795por De Cosa, Annapaola“…The CMS and ATLAS collaborations searched for Dark Matter (DM) particles directly produced in pair. The searches are performed using the full LHC Run-I dataset recorded with the CMS and ATLAS detectors in proton-proton collisions at a center-of-mass energy of 8 TeV. …”
Publicado 2015
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2796por de Cosa, Annapaola“…The CMS and ATLAS collaborations searched for Dark Matter (DM) particles directly produced in pair. The searches are performed using the full LHC Run-I dataset recorded with the CMS and ATLAS detectors in proton-proton collisions at a center-of-mass energy of 8 TeV. …”
Publicado 2015
Enlace del recurso
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2797
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2798
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2799
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2800