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1by Copeland, Edmund J“... Cosmology (known also as the Pre Big Bang), we go on to include the effects of axion fields and address...”
Published 2002
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2by Easson, Damien A.“... with the Standard Big Bang (SBB) model. In the simplest example, the topology of the universe is assumed...”
Published 2001
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3“... are topological defects, remnants of inflationary-era physics that persist after the big bang. They are formed...”
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4“.... However, with homogenous initial conditions, as one might expect from certain models of inflation, pre big...”
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5“... ϕ}(z\simeq 10^{10})<0.04$ at $2σ$ level in the big-bang nucleosynthesis epoch. : 12 pages plus 5...”
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6by Lange, A. E., Ade, P. A. R., Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Coble, K., Crill, B. P., de Bernardis, P., Farese, P., Ferreira, P., Ganga, K., Giacometti, M., Hivon, E., Hristov, V. V., Iacoangeli, A., Jaffe, A. H., Martinis, L., Masi, S., Mauskopf, P. D., Melchiorri, A., Montroy, T., Netterfield, C. B., Pascale, E., Piacentini, F., Pogosyan, D., Prunet, S., Rao, S., Romeo, G., Ruhl, J. E., Scaramuzzi, F., Sforna, D.“... to, the estimates from light element abundances and big bang nucleosynthesis. When combined with large scale...”
Published 2000
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