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1741
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1742
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1743
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1744por CERN. Geneva“…--HTML-->These lectures will discuss the application of ads/cft techniques to condensed matter systems. After motivating this endeavor, I will review the basic features of the ads/cft correspondence that will be used. …”
Publicado 2009
Enlace del recurso
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1745por CERN. Geneva“…--HTML-->These lectures will discuss the application of ads/cft techniques to condensed matter systems. After motivating this endeavor, I will review the basic features of the ads/cft correspondence that will be used. …”
Publicado 2009
Enlace del recurso
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1746“…We calculate the gravitational corrections to the effective action of N=2 SU(2) Seiberg-Witten theory with matter using modularity, the holomorphic anomaly equation and expected behavior at the boundaries of the moduli space. …”
Enlace del recurso
Enlace del recurso
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1747por CERN. Geneva“…--HTML-->These lectures will discuss the application of ads/cft techniques to condensed matter systems. After motivating this endeavor, I will review the basic features of the ads/cft correspondence that will be used. …”
Publicado 2009
Enlace del recurso
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1748por CERN. Geneva“…--HTML-->These lectures will discuss the application of ads/cft techniques to condensed matter systems. After motivating this endeavor, I will review the basic features of the ads/cft correspondence that will be used. …”
Publicado 2009
Enlace del recurso
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1749
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1750
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1751
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1752
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1753
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1754
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1755
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1756“…We consider the singlet scalar model of dark matter and study the expected antiproton and positron signals from dark matter annihilations. …”
Enlace del recurso
info:eu-repo/semantics/article -
1757por Munoz, Carlos“…We consider the phenomenological implications of gravitino dark matter in the context of the $\mu\nu$SSM. The latter is an R-parity breaking model which provides a solution to the $\mu$-problem of the MSSM and explains the origin of neutrino masses by simply using right-handed neutrino superfields. …”
Publicado 2009
Enlace del recurso
info:eu-repo/semantics/article -
1758por Fayet, Pierre“…In a more general way, light dark matter particles are normally forbidden, unless they can annihilate sufficiently through a new interaction stronger than weak interactions (at lower energies), as induced by a light spin-1 U boson, or heavy-fermion exchanges in the case of scalar dark matter. …”
Publicado 2009
Enlace del recurso
Enlace del recurso
info:eu-repo/semantics/article -
1759
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1760“…We consider cosmologies in which a dark-energy scalar field interacts with cold dark matter. The growth of perturbations is followed beyond the linear level by means of the time-renormalization-group method, which is extended to describe a multi-component matter sector. …”
Enlace del recurso
Enlace del recurso
info:eu-repo/semantics/article