Language：English   Publishing type：Research paper (scientific journal)   Publisher：SciPost Foundation  

We quantize the D1-D5-P microstate geometries known as superstrata directly in supergravity. We use Rychkov's consistency condition [hep-th/0512053] which was derived for the D1-D5 system
for superstrata, this condition turns out to be strong enough to fix the symplectic form uniquely. For the (1, 0, n) superstrata, we further confirm this quantization by a bona-fide explicit computation of the symplectic form using the semiclassical covariant quantization method in supergravity. We use the resulting quantizations to count the known supergravity superstrata states, finding agreement with previous countings that the number of these states grows parametrically smaller than those of the corresponding black hole.

DOI： 10.21468/SciPostPhys.10.1.018

Open Access

Web of Science

Scopus

Language：English   Publishing type：Research paper (scientific journal)   Publisher：Springer Science and Business Media Deutschland GmbH  

We study the random geometry approach to the TT¯ deformation of 2d conformal field theory developed by Cardy and discuss its realization in a gravity dual. In this representation, the gravity dual of the TT¯ deformation becomes a straightforward translation of the field theory language. Namely, the dual geometry is an ensemble of AdS3 spaces or BTZ black holes, without a finite cutoff, but instead with randomly fluctuating boundary diffeomorphisms. This reflects an increase in degrees of freedom in the renormalization group flow to the UV by the irrelevant TT¯ operator. We streamline the method of computation and calculate the energy spectrum and the thermal free energy in a manner that can be directly translated into the gravity dual language. We further generalize this approach to correlation functions and reproduce the all-order result with universal logarithmic corrections computed by Cardy in a different method. In contrast to earlier proposals, this version of the gravity dual of the TT¯ deformation works not only for the energy spectrum and the thermal free energy but also for correlation functions.

DOI： 10.1007/JHEP11(2020)108

Open Access

Web of Science

Scopus

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

We give a survey of the present status of the microstate geometries called
superstrata. Superstrata are smooth, horizonless solutions of six-dimensional
supergravity that represent some of the microstates of the D1-D5-P black hole
in string theory. They are the most general microstate geometries of that sort
whose CFT dual states are identified. After reviewing relevant features of the
dual CFT, we discuss the construction of superstratum solutions in
supergravity, based on the linear structure of the BPS equations. We also
review some of recent work on generalizations of superstrata and physical
properties of superstrata. Although the number of superstrata constructed so
far is not enough to account for the black-hole entropy, they give us valuable
insights into the microscopic physics of black holes.

DOI： 10.1007/s10714-020-02698-8

Web of Science

Scopus

arXiv

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

We count the number of regular supersymmetric solutions in supergravity,
called superstrata, that represent non-linear completion of linear fluctuations
around empty AdS_3 x S^3. These solutions carry the same charges as the D1-D5-P
black hole and represent its microstates. We estimate the entropy using
thermodynamic approximation and find that it is parametrically smaller than the
area-entropy of the D1-D5-P black hole. Therefore, these superstrata based on
AdS_3 x S^3 are not typical microstates of the black hole. What are missing in
the superstrata based on AdS_3 x S^3 are higher and fractional modes in the
dual CFT language. We speculate on what kind of other configurations to look at
as possible realization of those modes in gravity picture, such as superstrata
based on other geometries, as well as other brane configurations.

DOI： 10.1007/JHEP10(2019)017

Open Access

Web of Science

Scopus

arXiv

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

We construct a new class of smooth horizonless microstate geometries of the
supersymmetric D1-D5-P black hole in type IIB supergravity. We first work in
the AdS$_3 \times S^3$ decoupling limit and use the fermionic symmetries of the
theory to generate new momentum carrying perturbations in the bulk that have an
explicit CFT dual description. We then use the supergravity equations to
calculate the backreaction of these perturbations and find the full non-linear
solutions both in the asymptotically AdS and asymptotically flat case. These
new geometries have a simpler structure than the previously known superstrata
solutions.

DOI： 10.1007/JHEP03(2019)095

Open Access

Web of Science

Scopus

arXiv

Language：English   Publishing type：Research paper (scientific journal)  

We construct an infinite family of smooth asymptotically-flat supergravity
solutions that have the same charges and angular momenta as general
supersymmetric D1-D5-P black holes, but have no horizon. These solutions
resemble the corresponding black hole to arbitrary accuracy outside of the
horizon: they have asymptotically flat regions, AdS_3 x S^3 throats and
very-near-horizon AdS_2 throats, which however end in a smooth cap rather than
an event horizon. The angular momenta of the solutions are general, and in
particular can take arbitrarily small values. Upon taking the AdS_3 x S^3
decoupling limit, we identify the holographically-dual CFT states.

DOI： 10.1007/JHEP02(2018)014

arXiv

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

A supertube is a supersymmetric configuration in string theory which occurs
when a pair of branes spontaneously polarizes and generates a new dipole charge
extended along a closed curve. The dipole charge of a codimension-2 supertube
is characterized by the U-duality monodromy as one goes around the supertube.
For multiple codimension-2 supertubes, their monodromies do not commute in
general. In this paper, we construct a supersymmetric solution of
five-dimensional supergravity that describes two supertubes with such
non-Abelian monodromies, in a certain perturbative expansion. In supergravity,
the monodromies are realized as the multi-valuedness of the scalar fields,
while in higher dimensions they correspond to non-geometric duality twists of
the internal space. The supertubes in our solution carry NS5 and 5$_2^2$ dipole
charges and exhibit the same monodromy structure as the SU(2) Seiberg-Witten
geometry. The perturbative solution has $\mathrm{AdS}_2\times S^2$ asymptotics
and vanishing four-dimensional angular momentum. We argue that this solution
represents a microstate of four-dimensional black holes with a finite horizon
and that it provides a clue for the gravity realization of a pure-Higgs branch
state in the dual quiver quantum mechanics.

DOI： 10.1007/JHEP12(2017)103

arXiv

Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1103/PhysRevLett.117.201601

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： http://dx.doi.org/10.1007/JHEP03(2012)084

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1007/JHEP03(2012)094

Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1103/PhysRevLett.106.191601

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1007/JHEP10(2011)116

Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1103/PhysRevD.84.026010

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1103/PhysRevLett.104.251603

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1088/1126-6708/2009/07/094

Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1016/j.nuclphysb.2007.08.010

Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1088/1126-6708/2008/10/102

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1016/j.nuclphysb.2008.05.005

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1103/PhysRevD.77.044044

Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1088/1126-6708/2007/04/017

Authorship：Lead author   Language：Japanese   Publishing type：Research paper (scientific journal)  

Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1103/PhysRevLett.96.071601

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1088/1126-6708/2005/08/100

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1088/0264-9381/22/22/010

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1016/j.nuclphysb.2003.12.030

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1016/j.nuclphysb.2004.07.015

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1088/1126-6708/2003/04/052

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1088/1126-6708/2003/05/059

Authorship：Lead author   Language：English   Publishing type：Research paper (scientific journal)  

DOI： 10.1088/1126-6708/2002/06/034

Language：English   Publishing type：Research paper (scientific journal)  

DOI： https://doi.org/10.1103/PhysRevD.66.106001

Event date： 2021.6

Language：Japanese   Presentation type：Oral presentation (invited, special)  

Venue：Osaka University (Zoom)  

Event date： 2011.6

Language：Japanese   Presentation type：Oral presentation (general)  

Country：Japan  

Event date： 2011.3

Language：Japanese   Presentation type：Oral presentation (invited, special)  

Country：Japan  

Event date： 2011.2

Language：English   Presentation type：Oral presentation (general)  

Country：Japan  

Event date： 2011.2

Language：Japanese   Presentation type：Oral presentation (invited, special)  

Country：Japan  

Event date： 2010.6

Language：English   Presentation type：Oral presentation (general)  

Country：Japan  

Event date： 2009.12

Language：Japanese   Presentation type：Oral presentation (invited, special)  

Country：Japan  

Event date： 2009.10

Language：Japanese   Presentation type：Oral presentation (invited, special)  

Country：Japan  

Event date： 2009.7

Language：English   Presentation type：Oral presentation (general)  

Country：Japan  

Event date： 2009.6

Language：English   Presentation type：Oral presentation (invited, special)  

Country：Japan  

Event date： 2008.8

Language：English   Presentation type：Oral presentation (general)  

Country：Japan  

Event date： 2006.12

Language：English   Presentation type：Oral presentation (invited, special)  

Country：Japan  

Event date： 2006.4

Language：English   Presentation type：Oral presentation (general)  

Country：Japan  

Event date： 2005.12

Language：English   Presentation type：Oral presentation (general)  

Country：Japan