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Ising Cosmology
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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
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Cited by 1 Pith paper
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Energy momentum tensor correlators in $\phi^4$ theory II: The spin-two sector
A four-loop calculation shows the energy-momentum tensor charge C_T separates into a fixed-point value plus corrections proportional to the beta function.
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