Titlebook: Quantum Cosmology - The Supersymmetric Perspective - Vol. 2; Advanced Topic Paulo Vargas Moniz Book 2010 Springer-Verlag Berlin Heidelberg

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袖章

Connections and Loops Within SQCed upon Bianchi models described . with connections [20,21]. Further motivation will surely arise from recent developments in . [22–43], inheriting some of the main features and principles from . [44–66]. In this chapter, we explain . the outlook is so promising in this area.

beta-carotene

faction

Book 2010 promote continuity. The idea for this book took about 10 years to materialize, and it is the author’s hope that its content will constitute the beginning of further explorations beyond current horizons. More speci cally, this book appeals to the reader to engage upon and persevere with a journey, m

脫離

輕率看法

More Obstacles and Results: From QC to SQCear the end of this volume, the reader will hopefully agree that SQC constitutes a vaster, more adequate, and more elegant perspective for the very early universe. With this in mind, we have in this volume discussed further essential elements from either QC or SUSY/SUGRA, with a view to obtaining a more realistic SQC.

知識分子

Introduction in) a superstring theory? Why should the very early universe be explored in that manner? Are there enticing and interesting research problems left to solve? How relevant would it be to address and solve them?

男生如果明白

‘Observational’ Quantum Cosmologyhe boundaries of our knowledge, i.e., . exactly constitutes these limits? What are the best directions to move in, and in particular, what predictions or (falsifiable) tests for the universe can be made using quantum cosmology?

Intuitive

Additional SUSY and SUGRA Issuesare SUSY breaking (see Sects. 3.1 and 3.2) [1–9] and supersymmetric quantum mechanics (SQM) (see Sect. 3.3) [10–70]. Neither of them has been much investigated in SQC, although the latter feature could be associated with the SQC approach introduced in Chap. 6 of Vol. I.

DALLY

Further Explorations in SQC , = 1 SUGRAhat this uses the reduction of canonical quantum . = 1 SUGRA in four spacetime dimensions (see Sects. 4.1 and 4.2 of Vol. I) to a cosmological minisuperspace, with the essential feature that . momenta are represented by differential operators of the canonical conjugate variables [5–7].