Black Holes and Applied Holography
from
Monday, 12 November 2012 (10:00)
to
Friday, 16 November 2012 (16:30)
Monday, 12 November 2012
10:30
Registration
Registration
10:30 - 11:00
Room: Aud. C
11:00
A1
-
Gordon Semenoff
A1
Gordon Semenoff
11:00 - 11:50
Room: Aud. A
11:50
Coffee break
Coffee break
11:50 - 12:10
Room: Aud. C
12:10
A1
-
Gordon Semenoff
A1
Gordon Semenoff
12:10 - 13:00
Room: Aud. A
13:00
Lunch break
Lunch break
13:00 - 14:30
Room: Canteen
14:30
B1
-
Ben Craps
B1
Ben Craps
14:30 - 15:20
Room: Aud. A
15:20
Coffee break
Coffee break
15:20 - 15:40
Room: Aud. C
15:40
B1
-
Ben Craps
B1
Ben Craps
15:40 - 16:30
Room: Aud. A
Tuesday, 13 November 2012
10:00
B2
-
Ben Craps
B2
Ben Craps
10:00 - 10:50
Room: Aud. A
10:50
Coffee break
Coffee break
10:50 - 11:10
Room: Aud. C
11:10
B2
-
Ben Craps
B2
Ben Craps
11:10 - 12:00
Room: Aud. A
12:00
Coffee break
Coffee break
12:00 - 12:20
Room: Aud. C
12:20
C1
-
Jan de Boer
C1
Jan de Boer
12:20 - 13:10
Room: Aud. A
13:10
Lunch break
Lunch break
13:10 - 14:30
Room: Canteen
14:30
C1
-
Jan de Boer
C1
Jan de Boer
14:30 - 15:20
Room: Aud. A
15:20
Coffee break
Coffee break
15:20 - 15:40
Room: Aud. C
15:40
Exercises (B)
-
Ben Craps
Exercises (B)
Ben Craps
15:40 - 17:00
Room: Aud. D
19:00
Dinner at Spiseloppen
Dinner at Spiseloppen
19:00 - 21:30
Wednesday, 14 November 2012
10:00
Tour of NBI
-
Felicity Pors
(
Niels Bohr Archive
)
Tour of NBI
Felicity Pors
(
Niels Bohr Archive
)
10:00 - 11:00
Room: Reception
11:00
B3
-
Ben Craps
B3
Ben Craps
11:00 - 11:50
Room: Aud. A
11:50
Coffee break
Coffee break
11:50 - 12:10
Room: Aud. C
12:10
B3
-
Ben Craps
B3
Ben Craps
12:10 - 13:00
Room: Aud. A
13:00
Lunch
Lunch
13:00 - 14:20
Room: Canteen
14:20
C2
-
Jan de Boer
C2
Jan de Boer
14:20 - 15:10
Room: Aud. A
15:10
Coffee break
Coffee break
15:10 - 15:30
Room: Aud. C
15:30
C2
-
Jan de Boer
C2
Jan de Boer
15:30 - 16:20
Room: Aud. A
16:20
Coffee break
Coffee break
16:20 - 16:40
Room: Aud. C
16:40
Exercises (C)
-
Jan de Boer
Exercises (C)
Jan de Boer
16:40 - 18:00
Room: Aud. D
Thursday, 15 November 2012
10:00
C3
-
Jan de Boer
C3
Jan de Boer
10:00 - 10:50
Room: Aud. A
10:50
Coffee break
Coffee break
10:50 - 11:10
Room: Aud. C
11:10
C3
-
Jan de Boer
C3
Jan de Boer
11:10 - 12:00
Room: Aud. A
12:00
Coffee break
Coffee break
12:00 - 12:20
Room: Aud. C
12:20
A2
-
Gordon Semenoff
A2
Gordon Semenoff
12:20 - 13:10
Room: Aud. A
13:10
Lunch
Lunch
13:10 - 14:30
Room: Canteen
14:30
A2
-
Gordon Semenoff
A2
Gordon Semenoff
14:30 - 15:20
Room: Aud. A
15:20
Coffee break
Coffee break
15:20 - 15:40
Room: Aud. C
15:40
Exercises (A)
-
Gordon Semenoff
Exercises (A)
Gordon Semenoff
15:40 - 17:00
Room: Aud. D
Friday, 16 November 2012
10:00
Seminar, Quantum Fluctuations in Cosmology
-
Viatcheslav Mukhanov
Seminar, Quantum Fluctuations in Cosmology
Viatcheslav Mukhanov
10:00 - 11:00
Room: Aud. A
11:00
Coffee break
Coffee break
11:00 - 11:15
Room: Aud. C
11:15
A3
-
Gordon Semenoff
A3
Gordon Semenoff
11:15 - 12:05
Room: Aud. A
12:05
Coffee break
Coffee break
12:05 - 12:20
Room: Aud. C
12:20
A3
-
Gordon Semenoff
A3
Gordon Semenoff
12:20 - 13:10
Room: Aud. A
13:10
Lunch
Lunch
13:10 - 14:20
Room: Canteen
14:20
Examples of non-AdS Holography
-
Jelle Hartong
Examples of non-AdS Holography
(<font color="#990011">Series A:</font> <b><font color="#0066FF">Introduction to AdS/CFT </font></b> (Gordon Semenoff))
Jelle Hartong
14:20 - 15:10
Room: Aud. D
Mini introductory course on holography for space-times that are no longer asymptotically AdS but instead for example conformally AdS, Lifshitz or Schroedinger. Such cases are interesting for potential applications to condensed matter theory, black hole physics (Kerr/CFT, subtracted geometry) and for generalizing our notions of holography.
15:10
Coffee break
Coffee break
15:10 - 15:30
Room: Aud. C
15:30
Examples of non-AdS Holography
-
Jelle Hartong
Examples of non-AdS Holography
Jelle Hartong
15:30 - 16:20
Room: Aud. D
Mini introductory course on holography for space-times that are no longer asymptotically AdS but instead for example conformally AdS, Lifshitz or Schroedinger. Such cases are interesting for potential applications to condensed matter theory, black hole physics (Kerr/CFT, subtracted geometry) and for generalizing our notions of holography.