Since the first detection of a gravitational wave event of the
merger of two neutron stars in 2017, two more detections in the
neutron star mass range have been announced. The first one,
GW190425, involved an unusually massive neutron star, the...
The future interior of black holes in AdS/CFT can be described
in terms of a quantum circuit. We investigate boundary quantities
detecting properties of this quantum circuit. We discuss relations
between operator size, quantum complexity, and the...
Many space and astrophysical plasmas, such as the solar wind,
radiatively inefficient accretion flows onto black holes, and the
intracluster medium of galaxy clusters (ICM), are hot and dilute,
which makes them weakly collisional or even...
This is a continuation of a series of talks I have given in
recent years reporting on work with Jan Manschot, et. al.
There will be some repetition, and some updates and new
results. (See below for some relevant links.)
Manschot and I have...
This is a continuation of a series of talks I have given in
recent years reporting on work with Jan Manschot, et. al.
There will be some repetition, and some updates and new
results. (See below for some relevant links.)
Manschot and I have...
Abstract: This is a continuation of a series of talks I have
given in recent years reporting on work with Jan Manschot, et.
al.
There will be some repetition, and some updates and new
results. (See below for some relevant links.)
Manschot and I...
The clustered nature of star formation leaves a long-term
imprint on galaxies, stars, and planets. At young ages, stellar
clustering subdivides galaxies into individual building blocks
undergoing vigorous, feedback-driven life cycles that vary
with...
I will discuss ongoing work about a string theoretic
perspective on the 2d Bethe/Gauge correspondence of
Nekrasov-Shatashvili. In this work, we focus on gl(M|N) spin
chains. We show that the two sides of the correspondence, the
integrable spin chain...
We present spherically symmetric solutions to Einstein’s
equations, which are equivalent to canonical Schwarzschild and
Reissner-Nordstrom black holes on the exterior, but with singular
(Planck-density) shells at their respective event and inner...
