microscopic entropy of black rings trobada de nadal 2004 a ecm s1s1 s2s2 david mateos
TRANSCRIPT
Microscopic Entropy of Black RingsMicroscopic Entropy of Black RingsTrobada de Nadal 2004 a ECMTrobada de Nadal 2004 a ECM
S1
S2
David MateosDavid Mateos
•Microscopic Entropy of the Black Ring [hep-th/0411187] M. Cyrier, M. Guica, D.M. & A. Strominger
•A Supersymmetric Black Ring [hep-th/0407065] H. Elvang, R. Emparan, D.M. & H. Reall
•Supersymmetric Black Rings and 3-charge Supertubes [hep-th/0408120] H. Elvang, R. Emparan, D.M. & H. Reall
•Supertubes [hep-th/0103030] D.M. & P. Townsend
•Supergravity Supertubes [hep-th/0106012] R. Emparan, D.M. & P. Townsend
•Tachyons, Supertubes and Brane/anti-Brane Systems [hep-th/0112054] D.M., S. Ng & P. Townsend
•Supercurves [hep-th/0204062] D.M., S. Ng & P. Townsend
Black Ring = Asymptotically Flat, Stationary Black Hole Solution in 5D with Horizon Topology S1 £ S2
S1
S2
£ flat directions = Black Supertube
Why are Supersymmetric BRs interesting?
• Establish stability and non-uniqueness in susy sector
(In 4D ! S2, in 5D ! Emparan & Reall)
• Implication for microscopic entropy calculation
! Not only counting BPS states with same charges is not enough,
it is also not right.
• Provide ideal arena to study these issues because:
susy + know microscopic constituents + stability mechanism
• Expose how little we know about gravitational physics in D>4
2-charge Supertubes: Worldvolume Description D.M. & Townsend
Supersymmetric Brane Expansion in Flat Space by Angular Momentum
F1
D0
E
B
P
Tubular D2/F1/D0 Bound State
1/4-SUSY preserved
QF1 and QD0 dissolved as fluxesJ generated as integrated PoyntingE = QF1 + QD0
Arbitrary Cross-section C in E8:(and charge densities)
TS-Dualizing = `Helical’ String with Left-moving wave on it
No net D2-brane charge but dipole qD2 » nD2
J
¼-SUSY
C
P
J
2-charge Supertubes: Supergravity Description Emparan, D.M. & Townsend
No net D2 charge, but D2 dipole (and higher) moments:
Easily understood ~ D2/anti-D2 pair:
x
3-charge Supertubes and Supersymmetric Black Rings:Supergravity Description
Elvang, Emparan, D.M. & ReallBena & WarnerGauntlett & Gutowski
T34 Lift
First, lift 2-charge supertube to M-theory:
Ring solution with regular horizon ! 3 charges
Best microscopic description ! M-theory
T6 E4 = E2 (r, £ E2 (, )
r
R
£ time = 5D black ring metric
With 3 charges, each pair expands:
r
R
New feature: J 0
7 parameters: R, Qi , qi
5 conserved charges: Qi , J and J
Infinite violation of uniqueness
Choosing Qi, qi and J as independent parameters:
Black String Limit
Send R ! 1 keeping Qi / R and qi fixed
Important: J ! P 0 but J ! 0 !
Black string solution of Bena
S2
12
M23456
M5
E B
E £ B = 0
12
M23456
M5
E B
E £ B / Q1 q1 + Q2 q2 + Q3 q3 – q1 q2 q3
Suggests J is Poynting-generated by SUGRA fields J » s T0 » s E £ B
Components of D=11 SUGRA F4
Worldvolume 3-charge Supertubes
Elvang, Emparan, D.M. & Reall
First step: F1/D4/D0 bound state with D2/D6/NS5 dipoles Bena & Kraus
Gibbons & PapadopoulosGauntlett, Lambert & West
Problematic in openstring description
Circumvented in M-theory:
Single M5-brane =
Holomorphic 2-surface in T6
7
Turning on H induces M2 charge and allows arbitrary C
C
In summary: Captures 3 dipoles, J = 0
Microscopic Entropy Counting
Single M5-brane =
Holomorphic 2-surface in T6 S1 R1,3
4D black hole
Maldacena, Strominger & Witten; Vafa
(0,4) CFT with cleft= 6q1q2q3 and left-moving momentum p
p’ = p + M2-induced shift
M-theory on T6 £ S1 £ R1,3
Microscopic Entropy Counting Cyrier, Guica, D.M. & Strominger
Single M5-brane =
Holomorphic 2-surface in T6 S1 in R1,4
5D black ring
(0,4) CFT with cleft= 6q1q2q3 and left-moving momentum p = J
Counts states with J=0 !!!
M-theory on T6 £ R1,4
One conclusion:
Microscopic constituents of Susy Black Rings
= Supertubes
One open question:
Microscopic versus macroscopic descriptions?
or
J ?
3-charge Supertubes D1/D5/P System Elvang, Emparan, D.M & ReallBena & Kraus
Same CFT describes Black Hole and Black Ring
Decoupling limit: ’ ! 0 , r /’ fixed, etc.
RG
>