String Cosmology 2009
DOI: 10.1002/9783527628063.ch1
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Introduction to Cosmology and String Theory

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Cited by 2 publications
(11 citation statements)
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“…Which mesons condense first in D3/Dp systems depends on the details of the system. 4 The general lesson from these D3/Dp systems is that the p-wave superfluid phase transition appears to be vector meson condensation, which is in line with our weak-coupling intuition.…”
Section: Field Theory Descriptionsupporting
confidence: 58%
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“…Which mesons condense first in D3/Dp systems depends on the details of the system. 4 The general lesson from these D3/Dp systems is that the p-wave superfluid phase transition appears to be vector meson condensation, which is in line with our weak-coupling intuition.…”
Section: Field Theory Descriptionsupporting
confidence: 58%
“…Any closed string that wrap the null circle is massless, hence when T = 0 and we compactify x − the supergravity approximation becomes unreliable [182]. As emphasized in [182], if the spacetime has momentum in the x − direction then the x − circle is no longer 4 Supersymmetric Sch5 solutions do exist [187,188], obtained by using different directions of the S 5 (besides the Hopf fiber) in the TsT transformation, which are very similar in form to the solution above. We leave a thorough analysis of probe branes in those backgrounds for the future.…”
Section: The Null Melvin Twistmentioning
confidence: 99%
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