Titlebook: Cosmology and String Theory; Hora?iu N?stase Book 2019 Springer Nature Switzerland AG 2019 String Theory in Cosmology.string inflation.ekp

壁畫

https://doi.org/10.1007/978-3-322-81113-4dy of the basics of cosmology in a non-relativistic (non-general relativity) setting. Of course, the Universe is expanding, and the proper description of that is in general relativity, but we will see that with a simple non-relativistic analysis, supplemented with a few nontrivial points, we can go

Munificent

Constitution

,M?glichkeiten der Zieldeterminierung,lus cold dark matter). Dark Matter is what the name suggests, matter that is dark, i.e., non-luminous. That is, matter that we cannot detect from emitted light. I will presentthe evidences, then review the possible candidates for dark matter, and finish describing the .CDM model.

舊石器時(shí)代

音的強(qiáng)弱

,M?glichkeiten der Umfelddeterminierung, constant. We will see that we can quantify the condition into what is known as “slow-roll inflation”. We will not address other types of inflation in this book, though we will explain what they can be.

多產(chǎn)魚

野蠻

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無所不知

,M?glichkeiten der Umfelddeterminierung,ory of local supersymmetry. In practice, we will use a bit of both definitions to find it. Before that however, we need to define what supersymmetry is. After that, we will count degrees of freedom, in order to see what supergravity models we can have. After defining the vielbein-spin connection for

爭吵加

,M?glichkeiten der Umfelddeterminierung,raviton, described by the metric . (which can be written as .), except for the coupling to fermions, which is written in terms of .. -gravitino(s)., one for each supersymmetry.Indeed, each supersymmetry . takes us from the graviton to a different gravitino, .. -other fields: scalars ., vectors ., sp