<p>We construct an asymptotically flat T-fold representative of a four-dimensional dyonic black-hole charge orbit in doubled type-IIB theory. Starting from the F1-P-NS5-KKM toroidal seed, an integral parabolic T-duality monodromy is imposed on an active doubled three-torus. The non-geometric data enter only through this global patching: the Reissner–Nordstrom-type term is sourced by conserved four-dimensional electric and magnetic field strengths in the doubled Kaluza–Klein/winding local system, not by an internal algebraic <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(Q\)</EquationSource> <EquationSource Format="MATHML"><math> <mi>Q</mi> </math></EquationSource> </InlineEquation>-flux alone. Exact duality preserves the local equations, the BPS index and the <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(O(6,6)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>O</mi> <mo stretchy="false">(</mo> <mn>6</mn> <mo>,</mo> <mn>6</mn> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation>-invariant of the NS–NS/<InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(N=4\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>N</mi> <mo>=</mo> <mn>4</mn> </mrow> </math></EquationSource> </InlineEquation> charge sublattice governing the entropy. The minimal Einstein–Maxwell dilaton slice contains a running scalar branch and an equal-charge Reissner–Nordstrom limit; the extremal near-horizon region is locally <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(\textrm{AdS}_2\times S^2\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mtext>AdS</mtext> <mn>2</mn> </msub> <mo>×</mo> <msup> <mi>S</mi> <mn>2</mn> </msup> </mrow> </math></EquationSource> </InlineEquation>, with the compact factor globally T-duality patched.</p>

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A T-fold black hole in doubled type IIB

  • Mir Faizal,
  • Arshid Shabir

摘要

We construct an asymptotically flat T-fold representative of a four-dimensional dyonic black-hole charge orbit in doubled type-IIB theory. Starting from the F1-P-NS5-KKM toroidal seed, an integral parabolic T-duality monodromy is imposed on an active doubled three-torus. The non-geometric data enter only through this global patching: the Reissner–Nordstrom-type term is sourced by conserved four-dimensional electric and magnetic field strengths in the doubled Kaluza–Klein/winding local system, not by an internal algebraic \(Q\) Q -flux alone. Exact duality preserves the local equations, the BPS index and the \(O(6,6)\) O ( 6 , 6 ) -invariant of the NS–NS/ \(N=4\) N = 4 charge sublattice governing the entropy. The minimal Einstein–Maxwell dilaton slice contains a running scalar branch and an equal-charge Reissner–Nordstrom limit; the extremal near-horizon region is locally \(\textrm{AdS}_2\times S^2\) AdS 2 × S 2 , with the compact factor globally T-duality patched.