Black hole dynamics and information preservation

What happens to the information embodied in an exhausted star as it collapses into a black hole? Where in space is it preserved? how is it physically instantiated? How is it transduced into outgoing radiation? We will address those issues as we analyze the impact of QFT on the dynamics of a black hole. The analysis also shows why large BHs are cold and why electrically charged BHs are quick to shed their electric charge. The analysis further points to small, though potentially relevant quantum and statistical fluctuations inside a BH. An open question remains: how does the emerging picture of a BH interior, due to QFT effects, change the stress tensor, if at all, and what is its impact, if any, on the metric tensor inside the BH.

You will receive zoom access info by Meetup message and/or email (if I have your email) shortly after you RSVP to this event, provided you do so by noon on 7/12/20.

Cheers,

Moshe Rozenblit PhD