We discuss the decay of axion walls bounded by strings and present numerical simulations of the decay process. In these simulations, the decay happens immediately, in a time scale of order the light travel time, and the average energy of the radiated axions is (wa) -~ 7ma for v~,/rna ~-500. (w~) is
Axions from string decay
โ Scribed by C. Hagmann; S. Chang; P. Sikivie
- Publisher
- Elsevier Science
- Year
- 1999
- Tongue
- English
- Weight
- 422 KB
- Volume
- 72
- Category
- Article
- ISSN
- 0920-5632
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โฆ Synopsis
We have studied numerically the evolution and decay of axion strings. These global defects decay mainly by axion emission and thus contribute to the cosmological axion energy density. The relative importance of this source relative to misalignment production of axions depends on the spectrum. Radiation spectra for various string loop configurations are presented. They support the contention that the string decay contribution is of the same order of magnitude as the contribution from misalignment.
๐ SIMILAR VOLUMES
When the amount of the axion emitted from the axionic string and the a~ionic domain wall is evaluated, the number density of the source string should be necessarily determined. Although it is the simplest assumption that the axionic string obeys the scaling distribution similar to the cosmic gauged
## Abstract We discuss exclusive decays of large spin mesons into mesons in models of large __N__^__c__^ quenched QCD at strong coupling using string theory. The rate of the processes are calculated by studying the splitting of a macroscopic string on the relevant dual gravity backgrounds. We study