Following the collision of two compact objects, an accretion
disk forms and from it matter is ejected that sources the
universe's heavy elements and that is observable as a kilonova. The
amount of ejecta, the types of elements that form, and the...
Collisionless shocks are ubiquitously in the Universe and are
held responsible for the production of non-thermal particles and
high-energy radiation. Without particle collisions, theoretical
works show that microscopic instabilities are able to...
Next-generation Large-Scale Structure (LSS) and Cosmic Microwave
Background (CMB) surveys will provide us with unprecedented levels
of precision in the final constraints on our cosmological model.
However, the computational challenges posed by these...
Studying turbulence is an integral component of understanding
plasma behavior from fusion devices to interstellar space. While
much work has been done studying turbulence in laboratory fusion
settings, less has been attempted in the laboratory for...
Abstract 1: I will discuss gravitational waves (GWs)
induced by a heavy spectator field that starts to oscillate during
inflation. During the oscillation of the spectator field, its
effective mass can also oscillate in some potentials. This
mass...
The meeting will be a hybrid presentation of in person, for
Princeton University affiliates
(net ID holders) and Invited Speakers,
and a Zoom presentation for all NON PU affiliates.
Registration is required for everyone to receive the Zoom link
and...
