Journal
PHYSICAL REVIEW LETTERS
Volume 117, Issue 20, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.117.201601
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Funding
- John Templeton Foundation [48222]
- DOE [DE-SC0009924, DE-SC0011687]
- Padua University [CPDA144437]
- STFC [ST/L000415/1]
- JSPS KAKENHI Grant [16H03979]
- CEA Enhanced Eurotalents Fellowship
- Science and Technology Facilities Council [ST/L000415/1] Funding Source: researchfish
- Grants-in-Aid for Scientific Research [16H03979] Funding Source: KAKEN
- STFC [ST/L000415/1] Funding Source: UKRI
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We construct the first family of horizonless supergravity solutions that have the same mass, charges, and angular momenta as general supersymmetric rotating D1-D5-P black holes in five dimensions. This family includes solutions with arbitrarily small angular momenta, deep within the regime of quantum numbers and couplings for which a large classical black hole exists. These geometries are well approximated by the black-hole solution, and in particular exhibit the same near-horizon throat. Deep in this throat, the black-hole singularity is resolved into a smooth cap. We also identify the holographically dual states in the N = (4; 4) D1-D5 orbifold conformal field theory (CFT). Our solutions are among the states counted by the CFT elliptic genus, and provide examples of smooth microstate geometries within the ensemble of supersymmetric black-hole microstates.
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