Axiverse and Black Hole
Autor: | Kodama, Hideo, Yoshino, Hirotaka |
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Rok vydání: | 2011 |
Předmět: | |
Druh dokumentu: | Working Paper |
DOI: | 10.1142/S2010194512004199 |
Popis: | String theory/M-theory generally predicts that axionic fields with a broad mass spectrum extending below 10^{-10}eV are produced after compactification to four dimensions. These axions/fields provoke a rich variety of cosmophysical phenomena on different scales depending on their masses and provide us new windows to probe the ultimate theory. In this article, after overviewing this axiverse idea, I take up the black hole instability as the most fascinating one among such axionic phenomena and explain its physical mechanism and astrophysical predictions. Comment: References added; 32 pages, 24 figures. Based on the lecture at the 2011 Shanghai Asia-Pacific School and Workshop on Gravitation |
Databáze: | arXiv |
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