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arXiv:0806.0028 · Physical Review B

Quantum spherical spin glass with random short-range interactions

Pedro Castro Menezes, Alba Theumann

Published Aug 25, 2008• 5 citations
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Abstract

In the present paper we analyze the critical properties of a quantum spherical spin-glass model with short-range random interactions. Since the model allows for rigorous detailed calculations, we can show how the effective partition function calculated with the help of the replica method for the spin-glass fluctuating fields ${Q}_{\ensuremath{\alpha}\ensuremath{\gamma}}(\stackrel{P\vec}{k}{\ensuremath{\omega}}_{1}{\ensuremath{\omega}}_{2})$ separates into a mean-field contribution for ${Q}_{\ensuremath{\alpha}\ensuremath{\alpha}}(0;\ensuremath{\omega};\ensuremath{-}\ensuremath{\omega})$ and a strictly short-range partition function for the fields ${Q}_{\ensuremath{\alpha}\ensuremath{\ne}\ensuremath{\gamma}}(\stackrel{P\vec}{k}{\ensuremath{\omega}}_{1}{\ensuremath{\omega}}_{2})$. Here $\ensuremath{\alpha},\ensuremath{\gamma}=1,\dots{},n$ are replica indices. The mean-field part ${W}_{\text{MF}}$ coincides with previous results. The short-range part ${W}_{\text{SR}}$ describes a phase transition in a ${Q}^{3}$-field theory, where the fluctuating fields depend on a space variable $\stackrel{P\vec}{r}$ and times ${\ensuremath{\tau}}_{1}$ and ${\ensuremath{\tau}}_{2}$. This we analyze using the renormalization group with dimensional regularization and minimal subtraction of dimensional poles. By generalizing standard field theory methods to our particular situation, we can identify the critical dimensionality as ${d}_{c}=5$ at very low temperatures due to the dimensionality shift ${D}_{c}={d}_{c}+1=6$. We then perform an ${ϵ}^{\ensuremath{'}}$ expansion to order one loop to calculate the critical exponents by solving the renormalization-group equations.

DOI
10.1103/physrevb.78.054444

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In the present paper we analyze the critical properties of a quantum spherical spin-glass model with short-range random interactions. Since the model allows for rigorous detailed calculations, we can show how the effective partition function calculated with the help of the replica method for the spin-glass fluctuating fields {Q}_{\ensuremath{\alpha}\ensuremath{\gamma}}(\stackrel{P\vec}{k}{\ensuremath{\omega}}_{1}{\ensuremath{\omega}}_{2}) separates into a mean-field contribution for Q\ensuremathα\ensuremathα(0;\ensuremathω;\ensuremath−\ensuremathω){Q}_{\ensuremath{\alpha}\ensuremath{\alpha}}(0;\ensuremath{\omega};\ensuremath{-}\ensuremath{\omega})Q\ensuremathα\ensuremathα​(0;\ensuremathω;\ensuremath−\ensuremathω) and a strictly short-range partition function for the fields {Q}_{\ensuremath{\alpha}\ensuremath{\ne}\ensuremath{\gamma}}(\stackrel{P\vec}{k}{\ensuremath{\omega}}_{1}{\ensuremath{\omega}}_{2}). Here \ensuremathα,\ensuremathγ=1,…,n\ensuremath{\alpha},\ensuremath{\gamma}=1,\dots{},n\ensuremathα,\ensuremathγ=1,…,n are replica indices. The mean-field part WMF{W}_{\text{MF}}WMF​ coincides with previous results. The short-range part WSR{W}_{\text{SR}}WSR​ describes a phase transition in a Q3{Q}^{3}Q3-field theory, where the fluctuating fields depend on a space variable \stackrel{P\vec}{r} and times \ensuremathτ1{\ensuremath{\tau}}_{1}\ensuremathτ1​ and \ensuremathτ2{\ensuremath{\tau}}_{2}\ensuremathτ2​. This we analyze using the renormalization group with dimensional regularization and minimal subtraction of dimensional poles. By generalizing standard field theory methods to our particular situation, we can identify the critical dimensionality as dc=5{d}_{c}=5dc​=5 at very low temperatures due to the dimensionality shift Dc=dc+1=6{D}_{c}={d}_{c}+1=6Dc​=dc​+1=6. We then perform an ϵ\ensuremath′{ϵ}^{\ensuremath{'}}ϵ\ensuremath′ expansion to order one loop to calculate the critical exponents by solving the renormalization-group equations.
We analyze the critical properties of a quantum spherical spin-glass model with random inverse power-law interactions ${r}^{\ensuremath{-}(d+\ensuremath{\sigma})}$. It was shown in a previous publication that the effective partition function calculated with help of the replica method for the spin-glass fluctuating fields ${Q}_{\ensuremath{\alpha}\ensuremath{\gamma}}(\stackrel{P\vec}{k},{\ensuremath{\omega}}_{1},{\ensuremath{\omega}}_{2})$ separates into a mean-field contribution for the ${Q}_{\ensuremath{\alpha}\ensuremath{\alpha}}(0,\ensuremath{\omega},\ensuremath{-}\ensuremath{\omega})$ and a strictly long-range partition function for the fields ${Q}_{\ensuremath{\alpha}\ensuremath{\ne}\ensuremath{\gamma}}(\stackrel{P\vec}{k},{\ensuremath{\omega}}_{1},{\ensuremath{\omega}}_{2})$. Here $\ensuremath{\alpha},\ensuremath{\gamma}=1,\dots{},n$ are replica indices. The long-range part WLR{W}_{\text{LR}}WLR​ describes a phase transition in a Q3{Q}^{3}Q3-field theory that we analyze using the renormalization group with dimensional regularization and minimal subtraction of dimensional poles. By generalizing standard field theory methods to our particular situation, we can identify the upper critical dimensionality as ${d}_{c}=\frac{5\ensuremath{\sigma}}{2}$ at very low temperatures due to the dimensionality shift ${D}_{c}={d}_{c}+\frac{\ensuremath{\sigma}}{2}=3\ensuremath{\sigma}$. We then perform an ${ϵ}^{\ensuremath{'}}={d}_{c}\ensuremath{-}d$ expansion to order one loop to calculate the critical exponents by solving the renormalization-group equations.
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