Materias dentro de su búsqueda.
Materias dentro de su búsqueda.
Filosofía
16
Estudio y enseñanza
15
Inglés
14
Física
10
Química
10
Lenguaje y lenguas
9
Aspectos sociales
8
Materia
8
Historia
7
Traducción e interpretación
7
Arquitectura
6
Mente y cuerpo
6
Propiedades de la materia
6
Matemáticas
5
Novela inglesa
5
Retórica
5
Ciencia
4
Ciencia política
4
Conciencia (Psicología)
4
Constitución de la materia
4
Ecología
4
Estilo
4
Estudiantes universitarios
4
Mecánica
4
Teoría del conocimiento
4
Adquisición de segundo lenguaje
3
Aspectos económicos
3
Ciencias sociales
3
Conversación
3
Diseño
3
-
5461por Singh, A“…This model eliminates singularities in the existing Big Bang model of the universe, predicts effects of gravity on the observed mass evolution, dark matter/energy, and accelerated expansion of the universe. …”
Publicado 2004
Enlace del recurso
-
5462“…(Shortened) Weakly Interacting Massive Particles are often said to be the best Dark Matter candidates. Studies have shown however that rather large Dark Matter-photon or Dark Matter-baryon interactions could be allowed by cosmology. …”
Enlace del recurso
Enlace del recurso
-
5463
-
5464
-
5465
-
5466
-
5467
-
5468
-
5469por Koch, H, Backenstoss, Gerhard, Bamberger, A, Bergström, I, Bounin, P, Bunaciu, T, Egger, J, Hultberg, S, Lynen, U, Ritter, H G, Schwitter, A“…They depend on the basic interaction between a K/sup -/ and a nucleon and on the nuclear matter distribution at the surface of the nucleus. …”
Publicado 1972
Enlace del recurso
-
5470“…We propose and examine a new set of benchmark supersymmetric scenarios, some of which have non-universal Higgs scalar masses (NUHM) and others have gravitino dark matter (GDM). The scalar masses in these models are either considerably larger or smaller than the narrow range allowed for the same gaugino mass m_{1/2} in the constrained MSSM (CMSSM) with universal scalar masses m_0 and neutralino dark matter. …”
Enlace del recurso
Enlace del recurso
-
5471“…It is, therefore, quite promising in the present scenario that the supersymmetric dark matter is discovered before the LHC, assuming that the dark matter is the lightest supersymmetric particle.…”
Enlace del recurso
Enlace del recurso
-
5472
-
5473
-
5474por Viel, Matteo, Lesgourgues, Julien, Haehnelt, Martin G., Matarrese, Sabino, Riotto, Antonio“…We present constraints on the mass of Warm Dark Matter (WDM) particles from a combined analysis of the matter power spectrum inferred from the SDSS (Sloan Digital Sky Survey) Lyman-alpha flux power spectrum at 2.2<z<4.2, cosmic microwave background data and the galaxy power spectrum. …”
Publicado 2006
Enlace del recurso
Enlace del recurso
-
5475
-
5476
-
5477“…We investigate the measurement of supersymmetric particle masses at the LHC in gravitino dark matter (GDM) scenarios where the next-to-lightest supersymmetric partner (NLSP) is the lighter scalar tau, or stau, and is stable on the scale of a detector. …”
Enlace del recurso
Enlace del recurso
-
5478
-
5479por Picozza, P., Galper, A.M., Castellini, G., Adriani, O., Altamura, F., Ambriola, M., Barbarino, G.C., Basili, A., Bazilevskaja, G.A., Bencardino, R., Boezio, M., Bogomolov, E.A., Bonechi, L., Bongi, M., Bongiorno, L., Bonvicini, V., Cafagna, F., Campana, D., Carlson, P., Casolino, M., De Marzo, C., De Pascale, M.P., De Rosa, G., Fedele, D., Hofverberg, P., Koldashov, S.V., Krutkov, S.Yu., Kvashnin, A.N., Lund, J., Lundquist, J., Maksumov, O., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V.V., Minori, M., Misin, S., Mocchiutti, E., Morselli, A., Nikonov, N.N., Orsi, S., Osteria, G., Papini, P., Pearce, M., Ricci, M., Ricciarini, S.B., Runtso, M.F., Russo, S., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Taddei, E., Vacchi, A., Vannuccini, E., Voronov, S.A., Yurkin, Y.T., Zampa, G., Zampa, N., Zverev, V.G.Enlace del recurso
Publicado 2006
Enlace del recurso
-
5480“…We study the possible positron/electron excesses within the multi-component leptonically decaying dark matter (DM) scenario by fitting the most recent AMS-02 data on the positron fraction and total e+ + e− flux. …”
Enlace del recurso
Enlace del recurso