Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2011-07-04
Physics Letters B 703 (2011) 627-632
Physics
High Energy Physics
High Energy Physics - Theory
18 pages, acknowledgments included, some concepts clarified, typos corrected, journal reference included
Scientific paper
10.1016/j.physletb.2011.08.052
We have studied the Hawking radiation corresponding to the NS5 and Little String Theory (LST) black hole models using two semi-classical methods: the complex path method and a gravitational anomaly. After summarizing some known concepts about the thermodynamics of these theories, we have computed the emission rates for the two black hole models. The temperature calculated from, e.g. the well-known surface gravity expression, is shown to be identical to that obtained from both the computation of the gravitational anomaly and the complex path method. Moreover, the two semi-classical methods show that NS5 exhibits non-thermal behavior that contrasts with the thermal behavior of LST. We remark that energy conservation is the key factor leading to a non-thermal profile for NS5. In contrast, LST keeps a thermal profile even when energy conservation is considered because temperature in this model does not depend on energy.
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