Cardy formula

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Template:Short description In physics, the Cardy formula gives the entropy of a two-dimensional conformal field theory (CFT). In recent years, this formula has been especially useful in the calculation of the entropy of BTZ black holes and in checking the AdS/CFT correspondence and the holographic principle.

Using results by J. L. Cardy,[1] the following entropy formula can be derived:

S=2πc6(L0c24).

Here c is the central charge, L0=ER is the product of the total energy and radius of the system, and the shift of c/24 is related to the Casimir effect. These data emerge from the Virasoro algebra of this CFT. The proof of the above formula relies on modular invariance of a Euclidean CFT on the torus.

The Cardy formula is usually understood as counting the number of states of energy Δ=L0+L¯0 of a CFT quantized on a circle. To be precise, the microcanonical entropy (that is to say, the logarithm of the number of states in a shell of width δ1) is given by

Sδ(Δ)=2πcΔ3+O(lnΔ)

in the limit Δ. This formula can be turned into a rigorous bound.[2]

In 2000, E. Verlinde extended this to certain strongly-coupled (n+1)-dimensional CFTs.[3] The resulting Cardy–Verlinde formula was obtained by studying a radiation-dominated universe with the Friedmann–Lemaître–Robertson–Walker metric

ds2=dt2+R2(t)Ωn2

where R is the radius of a n-dimensional sphere at time t. The radiation is represented by a (n+1)-dimensional CFT. The entropy of that CFT is then given by the formula

S=2πRnEc(2EEc),

where Ec is the Casimir effect, and E the total energy. The above reduced formula gives the maximal entropy

SSmax=2πREn,

when Ec=E, which is the Bekenstein bound. The Cardy–Verlinde formula was later shown by Kutasov and Larsen[4] to be invalid for weakly interacting CFTs. In fact, since the entropy of higher dimensional (meaning n>1) CFTs is dependent on exactly marginal couplings, it is believed that a Cardy formula for the entropy is not achievable when n>1.

See also

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