Factorable
发表于 2025-3-25 03:59:26
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Tincture
发表于 2025-3-25 10:05:13
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FID
发表于 2025-3-25 12:39:02
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美色花钱
发表于 2025-3-25 18:51:04
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Tdd526
发表于 2025-3-25 23:14:31
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photopsia
发表于 2025-3-26 02:51:12
Gravitational Waves and the Cosmic Neutrino Background,nd the evolution of the universe. Unfortunately, the weakly interacting nature of neutrinos combined with the low temperature of the background today, makes the prospect for detection near impossible in the foreseeable future. Despite this, the dynamics of the C.B could have had significant effects
吹气
发表于 2025-3-26 05:09:13
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Infect
发表于 2025-3-26 08:53:33
Harald Schoen,Siegfried Schumann Any such extensions normally have many phenomenological implications, which can allow for the utilisation of a variety of tools to constrain the models. As of yet, none of these extensions have been accepted because they either are ruled out by experimental searches or current experiments are not s
AGOG
发表于 2025-3-26 14:26:03
Charlotte Kellermann,Hans Rattinger scalar field which acts as the inflaton, whose domination of the early universe’s energy density, and traversal of its almost flat potential, leads to the exponential expansion. In this chapter we explore a new class of natural inflation mechanisms which exhibit scale invariance via the dilaton, an
minaret
发表于 2025-3-26 19:29:28
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