Lecture 11: Global Gaussian Fluctuations for the Heights

2021 ◽  
pp. 86-93
2007 ◽  
Vol 10 (1) ◽  
pp. 21-27 ◽  
Author(s):  
Baruch Meerson ◽  
Manuel Díez-Minguito ◽  
Thomas Schwager ◽  
Thorsten Pöschel

2021 ◽  
Vol 3 (2) ◽  
Author(s):  
A. M. Bilen ◽  
B. Georgeot ◽  
O. Giraud ◽  
G. Lemarié ◽  
I. García-Mata

2018 ◽  
Vol 27 (14) ◽  
pp. 1846005 ◽  
Author(s):  
Tom Banks ◽  
W. Fischler

This essay outlines the Holographic Spacetime (HST) theory of cosmology and its relation to conventional theories of inflation. The predictions of the theory are compatible with observations, and one must hope for data on primordial gravitational waves or non-Gaussian fluctuations to distinguish it from conventional models. The model predicts an early era of structure formation, prior to the Big Bang. Understanding the fate of those structures requires complicated simulations that have not yet been done. The result of those calculations might falsify the model, or might provide a very economical framework for explaining dark matter and the generation of the baryon asymmetry.


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