(3.1) The metric function f (r) is determined by f (r) = r2 l2 − m r + q2 r2 , Ξ2 = 1 + a l2 , (3.2) 4 and the gauge potential admits the the following form A = − q r (Ξdt − adφ)

ROT A TING CHARGED BLACK STRINGS For a four-dimensional spacetime with cylindrical or toroidal horizons, the line element can be expressed as [31–33]: ds2 = −f (r)(Ξdt − adφ)2 + r2

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Thermodynamic relation on rotating charged black strings with arbitrary cosmological constant

hep-th · 2025-07-24 · conditional · novelty 2.0

For rotating charged black strings, the Goon-Penco relation follows directly from the extended first law, making the claimed universality a thermodynamic identity.

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Thermodynamic relation on rotating charged black strings with arbitrary cosmological constant hep-th · 2025-07-24 · conditional · none · ref 3
For rotating charged black strings, the Goon-Penco relation follows directly from the extended first law, making the claimed universality a thermodynamic identity.

(3.1) The metric function f (r) is determined by f (r) = r2 l2 − m r + q2 r2 , Ξ2 = 1 + a l2 , (3.2) 4 and the gauge potential admits the the following form A = − q r (Ξdt − adφ)

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