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  1. 4961
    “…We show that warm dark matter keV fermions (`inos') can be responsible for both core and halo galactic structure, in agreement with current astrophysical/cosmological constraints. We identify the inos with sterile right-handed neutrinos. …”
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    Enlace del recurso
    The role of self-interacting right-handed neutrinos in galactic structure
  2. 4962
    “…We highlight in particular direct dark matter detection experiments (which are sensitive to neutrino magnetic moments because of the predicted modifications to the solar neutrino scattering rate), stellar cooling, and cosmological constraints.…”
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    The Neutrino Magnetic Moment Portal
  3. 4963
    por Bartolo, N, Matarrese, S, Riotto, Antonio
    Publicado 2005
    “…We calculate the full second-order radiation transfer function for Cosmic Microwave Background anisotropies on large angular scales in a flat universe filled with matter and cosmological constant. It includes (i) the second-order generalization of the Sachs-Wolfe effect, and of (ii) both the early and late Integrated Sachs-Wolfe effects, (iii) the contribution of the second-order tensor modes, and is valid for a generic set of initial conditions specifying the level of primordial non-Gaussianity.…”
    Enlace del recurso
    Enlace del recurso
    The Full Second-Order Radiation Transfer Function for Large-Scale CMB Anisotropies
  4. 4964
    por Giovannini, Massimo
    Publicado 2006
    “…Large-scale magnetic fields can affect scalar cosmological perturbations whose evolution is described in the conformally Newtonian gauge and within the tight coupling approximation. …”
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    Enlace del recurso
    Transfer matrices for magnetized CMB anisotropies
  5. 4965
    “…We analyze the properties of dark matter halos in the cold-plus-warm dark matter cosmologies (CWDM). We study their dependence on the fraction and velocity dispersion of the warm particle, keeping the free-streaming scale fixed. …”
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    Enlace del recurso
    The inner structure of haloes in Cold+Warm dark matter models
  6. 4966
    por Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Battaner, E., Benabed, K., Benoit-Levy, A., Bernard, J.P., Bersanelli, M., Bielewicz, P., Bond, J.R., Borrill, J., Bouchet, F.R., Burigana, C., Butler, R.C., Calabrese, E., Chamballu, A., Chiang, H.C., Christensen, P.R., Clements, D.L., Colombo, L.P.L., Couchot, F., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Diego, J.M., Dole, H., Dore, O., Dupac, X., Ensslin, T.A., Eriksen, H.K., Fabre, O., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Galeotta, S., Galli, S., Ganga, K., Giard, M., Gonzalez-Nuevo, J., Gorski, K.M., Gregorio, A., Gruppuso, A., Hansen, F.K., Hanson, D., Harrison, D.L., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huffenberger, K.M., Jaffe, A.H., Jones, W.C., Keihanen, E., Keskitalo, R., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lamarre, J.M., Lasenby, A., Lawrence, C.R., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P.B., Linden-Vornle, M., Lopez-Caniego, M., Lubin, P.M., Macias-Perez, J.F., Mandolesi, N., Maris, M., Martin, P.G., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Mazzotta, P., Meinhold, P.R., Melchiorri, A., Mendes, L., Menegoni, E., Mennella, A., Migliaccio, M., Miville-Deschenes, M.A., Moneti, A., Montier, L., Morgante, G., Moss, A., Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Norgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., Oxborrow, C.A., Pagano, L., Pajot, F., Paoletti, D., Pasian, F., Patanchon, G., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Pratt, G.W., Prunet, S., Rachen, J.P., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Ristorcelli, I., Rocha, G., Roudier, G., Rusholme, B., Sandri, M., Savini, G., Scott, D., Spencer, L.D., Stolyarov, V., Sudiwala, R., Sutton, D., Suur-Uski, A.S., Sygnet, J.F., Tauber, J.A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Uzan, J.P., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L.A., Yvon, D., Zacchei, A., Zonca, A.
    Publicado 2014
    “…We examine in detail the degeneracies between fundamental constants and the cosmological parameters, in order to compare the limits obtained from Planck and WMAP and to determine the constraining power gained by including other cosmological probes. …”
    Enlace del recurso
    Enlace del recurso
    Planck intermediate results. XXIV. Constraints on variation of fundamental constants
  7. 4967
    “…We train this emulator with more than 200,000 measurements, spanning a broad cosmological parameter space that includes massive neutrinos and dynamical dark energy. …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    Accelerating Large-Scale-Structure data analyses by emulating Boltzmann solvers and Lagrangian Perturbation Theory
  8. 4968
    por Mazure, Alain, Basa, Stéphane
    Publicado 2009
    “…In this book, cosmologists Dr Alain Mazure and Dr Stéphane Basa throw light on the assemblage of facts, hypotheses and cosmological conclusions and show how these ‘beacons’ illuminate their immediate surroundings and allow us to study the vast cosmos, like searchlights revealing the matter comprising our universe.…”
    Enlace del recurso
    Exploding superstars: understanding supernovae and gamma-ray bursts
  9. 4969
    por Schmelling, Michael
    Publicado 2005
    “…Cosmological arguments suggest that physics beyond the Standard Model, so-called New Physics, is needed to explain the matter-antimatter asymmetry of the universe by providing extra sources of CP-violation. …”
    Enlace del recurso
    Sensitivity to New Physics in the B-Sector
  10. 4970
    por Alloin, Danielle, Gieren, Wolfgang
    Publicado 2003
    “…A sufficient accuracy is required both for a precise determination of the cosmological parameters and also in order to achieve a better understanding of physical processes in extragalactic systems. …”
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    Enlace del recurso
    Stellar candles for the extragalactic distance scale
  11. 4971
    por von Berlepsch, Regina
    Publicado 2011
    “…<br /> The result is a systematic overview of the latest astronomical and cosmological research.<br />…”
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    Deciphering the universe through spectroscopy
  12. 4972
    “…Combined with the COBE measurement and the high redshift supernovae data we obtain new constraints on the fractional matter density and the cosmological constant.…”
    Enlace del recurso
    Enlace del recurso
    A measurement of $\Omega$ from the North American test flight of BOOMERANG
  13. 4973
    por Bertin, V, Nezri, E, Orloff, J
    Publicado 2002
    “…Only models with neutralino annihilation into gauge bosons can satisfy cosmological constraints and current neutrino indirect detection sensitivities. …”
    Enlace del recurso
    Enlace del recurso
    Neutrino Indirect Detection of Neutralino Dark Matter in the CMSSM
  14. 4974
    por Barbieri, Riccardo
    Publicado 1981
    “…Topics dealt with are: new thresholds beyond the mass of the Higgs boson, and associated violation of lepton and baryon number; chirality and anomaly constraints; a prediction for the top quark mass and the value of the light quark mass scale; heavy fermions and cosmological baryon production at temperatures near 1 TeV. (13 refs).…”
    Enlace del recurso
    New physical thresholds above M/sub W/
  15. 4975
    por Schmelling, M
    Publicado 2005
    “…Cosmological arguments suggest that physics beyond the Standard Model, so-called New Physics, is needed to explain the matter-antimatter asymmetry of the universe by providing extra sources of CP-violation. …”
    Enlace del recurso
    Sensitivity to New Physics in the B-Sector
  16. 4976
    por Bodeker, Dietrich
    Publicado 2006
    “…The high temperature damping rate is always smaller than the Hubble rate, so that thermal effects are not sufficient for solving the cosmological moduli problem.…”
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    Enlace del recurso
    Moduli decay in the hot early Universe
  17. 4977
    “…We illustrate how recently improved low-redshift cosmological measurements can tighten constraints on neutrino properties. …”
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    Enlace del recurso
    Robust Neutrino Constraints by Combining Low Redshift Observations with the CMB
  18. 4978
    “…The light neutrino mixing angles observable via oscillation effects are related to the heavy conjugate (right-handed) neutrino mass matrix, which also plays a key role in cosmological baryogenesis. The ratios of neutrino and charged lepton decay modes in baryon decay may also be related to neutrino oscillation parameters. …”
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    Enlace del recurso
    Flipped angles and phases: a systematic study
  19. 4979
    “…We work out the predictions for all sparticle and Higgs masses and discuss the prospects for their detection at the Tevatron, LEPI,II, and HERA. We find that the cosmological neutralino relic density is always within current expectations (\ie, $\Omega_\chi h^2_0\lsim0.9$). …”
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    Enlace del recurso
    Towards a unified string supergravity model
  20. 4980
    “…Utilising non-perturbative lattice simulations, we demonstrate here that the symmetry does get restored at a certain temperature T_c, both for a 3+1 and a 4+1 dimensional world (the latter with a finite cutoff). To avoid a cosmological domain wall problem, such models would thus be allowed only if the reheating temperature after inflation is below T_c. …”
    Enlace del recurso
    Enlace del recurso
    Finite temperature Z(N) phase transition with Kaluza-Klein gauge fields
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