Week 01.06.2009 – 07.06.2009

Monday (01 Jun)

Numerical metrics on moduli spaces of Calabi-Yau manifolds

Regular Seminar Sergio Lukic (Imperial College)

at:
13:00 IC
room IMS seminar room
abstract:

I will explain two algorithms that compute numerically the Weil-Petersson metric on the moduli space of polarized Calabi-Yau manifolds. I will show some explicit examples. Finally, I will outline some applications of these techniques in the physics of Calabi-Yau compactifications of string theory.

Tuesday (02 Jun)

Quasi-classical quantisation of AdS4 x CP3 superstring and giant magnons

Regular Seminar Igor Shenderovich (St Petersburg)

at:
14:00 IC
room H503
abstract:

We discuss quasi-classical quantization of AdS4 x CP3 superstring using the algebraic curve techinque. We exemplify this procedure on some configurations so called giant magnons. It turns out that there are two types of configurations and they are quantizied in slightly different ways. Also we discuss testing AdS/CFT correspondence in this case.

World-sheet dualities for superspace sigma models

Regular Seminar Thomas Quella (University of Amsterdam)

at:
14:00 KCL
room 521
abstract:

Thursday (04 Jun)

Black hole microstate geometries and the information paradox

Regular Seminar Iosif Bena (Saclay)

at:
14:00 QMW
room 410 B
abstract:

Stringy modifications to spacetime structure and the CMB

Regular Seminar Subodh Patil (Humboldt University)

at:
14:00 IC
room H503
abstract:

In this talk, we will review recent work which asks the question, what, if any effects stringy modifications to geometry might have on the predictions of inflation? We couch our discussion within two well motivated frameworks-- non-commutative geometry (likely to be present during brane inflation), and modifications to mode propagation coming from a field theory representation of the stringy uncertainty principle. In the former case, we find that UV/IR mode mixing can imprint potentially observable signatures onto the CMB independent of the scale of inflation. In the latter case, we analytically compute corrections, and comment on the possibility of observing these in the fortunate circumstance that we happen to find ourselves in a weakly coupled corner of moduli space.