Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Chung, D. J. H."'
Autor:
Komatsu, E., Afshordi, N., Bartolo, N., Baumann, D., Bond, J. R., Buchbinder, E. I., Byrnes, C. T., Chen, X., Chung, D. J. H., Cooray, A., Creminelli, P., Dalal, N., Dore, O., Easther, R., Frolov, A. V., Gorski, K. M., Jackson, M. G., Khoury, J., Kinney, W. H., Kofman, L., Koyama, K., Leblond, L., Lehners, J. -L., Lidsey, J. E., Liguori, M., Lim, E. A., Linde, A., Lyth, D. H., Maldacena, J., Matarrese, S., McAllister, L., McDonald, P., Mukohyama, S., Ovrut, B., Peiris, H. V., Raeth, C., Riotto, A., Rodriguez, Y., Sasaki, M., Scoccimarro, R., Seery, D., Sefusatti, E., Seljak, U., Senatore, L., Shandera, S., Shellard, E. P. S., Silverstein, E., Slosar, A., Smith, K. M., Starobinsky, A. A., Steinhardt, P. J., Takahashi, F., Tegmark, M., Tolley, A. J., Verde, L., Wandelt, B. D., Wands, D., Weinberg, S., Wyman, M., Yadav, A. P. S., Zaldarriaga, M.
A new and powerful probe of the origin and evolution of structures in the Universe has emerged and been actively developed over the last decade. In the coming decade, non-Gaussianity, i.e., the study of non-Gaussian contributions to the correlations
Externí odkaz:
http://arxiv.org/abs/0902.4759
Publikováno v:
Phys.Rev. D70 (2004) 083505
We analyze the limits on resonant particle production during inflation based upon the power spectrum of fluctuations in matter and the cosmic microwave background. We show that such a model is consistent with features observed in the matter power spe
Externí odkaz:
http://arxiv.org/abs/astro-ph/0406046
Publikováno v:
Phys.Rept.407:1-203,2005
After an introduction recalling the theoretical motivation for low energy (100 GeV to TeV scale) supersymmetry, this review describes the theory and experimental implications of the soft supersymmetry-breaking Lagrangian of the general minimal supers
Externí odkaz:
http://arxiv.org/abs/hep-ph/0312378
Publikováno v:
JCAP 0310 (2003) 012
During inflation, primordial energy density fluctuations are created from approximate de Sitter vacuum quantum fluctuations redshifted out of the horizon after which they are frozen as perturbations in the background curvature. In this paper we demon
Externí odkaz:
http://arxiv.org/abs/hep-ph/0305074
Publikováno v:
Phys.Lett. B556 (2003) 61-70
At present we know nothing about the nature of the dark energy accounting for about 70% of the energy density of the Universe. One possibility is that the dark energy is provided by an extremely light field, the quintessence, rolling down its potenti
Externí odkaz:
http://arxiv.org/abs/hep-ph/0210427
Autor:
Chung, D. J. H.
Publikováno v:
High Energy Physics - Proceedings of the Fifth Latin American Symposium; 2006, p77-98, 22p