Quantum Phase Transitions

نویسنده

  • Subir Sachdev
چکیده

whereM is a real, symmetric, positive-definite matrix (i.e. all eigenvalues are positive). This identity can be easily established by changing variables of integration to a basis in which M is diagonal. We will use this identity to compute the free energy density F , defined by Z = exp(−V F ) where V is the volume of spacetime. In the paramagnetic phase, r > 0, the perturbative expansion for F takes the form F = C1 + C2u + O(u) + . . ., while in the magnetically ordered phase, r < 0, it takes the form F = C3/u+C4 +O(u). Obtain expressions for C1−4. Assume we have normalized the Dφα in Z to absorb the factor of 1/ √ π in (2).

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تاریخ انتشار 1999