Ising Cosmology

Abstract

Using arguments from holography we propose that the deviation of the cosmological spectral index $n_S$ of scalar fluctuations from unity may be controlled almost entirely by the critical exponent $\eta$ of the $d=3$ Ising model

arXiv comment10 pages, 1 figure, version accepted for publication

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Cited by in corpus (1)

• Thermal effects in Ising Cosmology