Quantum Gravity Unit Guest Seminar: Tensionless strings and Compactification

Visitor seminar hosted by Quantum Gravity Unit

Speaker: Dr. Priyadarshini Pandit, Indian Institute of Technology Kanpur

Title: Tensionless Strings and Compactification

Electromagnetism from Spacetime Algebra

A physics lecture for borderline-physicists.
Title: Electromagnetism from Spacetime Algebra.
Speaker: Yasha Neiman.

Planets in bullet-time: inside Ne(wt)o(n)'s apple

A physics lecture for non-physicists.
Title: Planets in bullet-time: inside Newton's apple.
Speaker: Yasha Neiman.

Kite and Triangle diagrams through Symmetries of Feynman Integrals

Visitor seminar hosted by Quantum Gravity Unit
Speaker: Dr. Subhajit Mazumdar,Center for Theoretical Physics, Seoul National University
Title: Kite and Triangle diagrams through Symmetries of Feynman Integrals

QG group meeting: self-dual GR in de Sitter space (Yasha Neiman)

QG group meeting.
Speaker: Yasha Neiman.
Title: "Self-dual GR in de Sitter space".

Gravity, the Improbability Engine

A physics lecture for non-physicists.
Title: Gravity, the Improbability Engine.
Speaker: Yasha Neiman.

Why is the sky blue?

A physics lecture for non-physicists.
Title: Why is the sky blue?
Speaker: Yasha Neiman.

"BRST formalism of Weyl conformal gravity in Weyl geometry" Prof. Ichiro Oda, University of the Ryukyus

Quantum Gravity Unit visitor seminar.
Speaker: Prof. Ichiro Oda, University of the Ryukyus
Title: BRST formalism of Weyl conformal gravity in Weyl geometry

"BMS algebra from Virasoro algebras", Dr. Hisayoshi Muraki, IBS Center for Geometry and Physics

Visitor Seminar hosted by Quantum Gravity Unit
Speaker: Dr. Hisayoshi Muraki, IBS Center for Geometry and Physics
Title: "BMS algebra from Virasoro algebras"

Quantum Informational Analogue Models of Black Holes: What Happens After Half Evaporation?, Dr. Marco Michel, Ben-Gurion University of the Negev

Quantum Gravity Unit visitor seminar.
Speaker: Dr. Marco Michel, Ben-Gurion University of the Negev .
Title: Quantum Informational Analogue Models of Black Holes: What Happens After Half Evaporation?