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(0,4) sigma models and K3
Sarah Harrison Stanford University

The BoseHubbard model is QMAcomplete
David Gosset Institute for Quantum Computing (IQC)

Scalefree primordial cosmology
Anna Ijjas Max Planck Institute for Gravitational Physics  Albert Einstein Institute (AEI)

13/14 PSI  Standard Model Review  Lecture 1
Paul Langacker Institute for Advanced Study (IAS)
PIRSA:14010008 
13/14 PSI  Gravitational Physics Review  Lecture 1
Ruth Gregory King's College London  Department of Mathematics
PIRSA:14010027 
13/14 PSI  Standard Model Review  Lecture 2
Paul Langacker Institute for Advanced Study (IAS)
PIRSA:14010009 
13/14 PSI  Gravitational Physics Review  Lecture 2
Ruth Gregory King's College London  Department of Mathematics
PIRSA:14010028 

Introduction to Quantum Field Theory for Cosmology  Lecture 1
Achim Kempf University of Waterloo
PIRSA:14010000 
13/14 PSI  Standard Model Review  Lecture 3
Paul Langacker Institute for Advanced Study (IAS)
PIRSA:14010010