May 2020

Friday, May 1, 2020

12:30pm

- 1:30pm

Zoom meeting

I will discuss new insights into the structure of the nucleon obtained through first-principles lattice QCD calculations.

Wednesday, May 6, 2020

1:30pm

- 2:30pm

zoom

Quantum field theory (QFT) works remarkably well for making theoretical predictions in collider scattering experiments.

Friday, May 8, 2020

12:30pm

- 1:30pm

Zoom

Neutrinos are copiously produced at the LHC, but no LHC neutrino has ever been detected. FASERv, a recently approved subdetector of FASER, is designed to detect such collider neutrinos for the first time and study their properties.

Wednesday, May 13, 2020

1:30pm

- 2:30pm

Zoom

Light dark matter (DM) is difficult to detect in traditional nuclear recoil searches due to the small amount of energy transferred in DM-nucleus scattering.

Friday, May 15, 2020

12:30pm

- 1:30pm

Zoom

Core-collapse supernovae originate from the gravitational collapse of massive stars. These explosions are the birthplace of neutron stars, the site of element synthesis, and the source of copious quantities of neutrinos.

Wednesday, May 20, 2020

1:30pm

- 2:30pm

zoom

Eff

Friday, May 22, 2020

12:30pm

- 1:30pm

zoom

Sterile neutrinos with masses around a few keV have been postulated to be viable dark matter candidates.

Wednesday, May 27, 2020

1:30pm

- 2:30pm

Zoom

In this talk, I will review a framework for finding the conservative potential of compact binary systems using scattering amplitudes and effective field theory.

Friday, May 29, 2020

12:30pm

- 1:30pm

Zoom

I will describe a new method to compute and constrain the possible shapes of primordial correlation functions from inflation.

May 2020

Friday, May 1, 2020

12:30pm

- 1:30pm

Zoom meeting

I will discuss new insights into the structure of the nucleon obtained through first-principles lattice QCD calculations.

Wednesday, May 6, 2020

1:30pm

- 2:30pm

zoom

Quantum field theory (QFT) works remarkably well for making theoretical predictions in collider scattering experiments.

Friday, May 8, 2020

12:30pm

- 1:30pm

Zoom

Neutrinos are copiously produced at the LHC, but no LHC neutrino has ever been detected. FASERv, a recently approved subdetector of FASER, is designed to detect such collider neutrinos for the first time and study their properties.

Wednesday, May 13, 2020

1:30pm

- 2:30pm

Zoom

Light dark matter (DM) is difficult to detect in traditional nuclear recoil searches due to the small amount of energy transferred in DM-nucleus scattering.

Friday, May 15, 2020

12:30pm

- 1:30pm

Zoom

Core-collapse supernovae originate from the gravitational collapse of massive stars. These explosions are the birthplace of neutron stars, the site of element synthesis, and the source of copious quantities of neutrinos.

Wednesday, May 20, 2020

1:30pm

- 2:30pm

zoom

Eff

Friday, May 22, 2020

12:30pm

- 1:30pm

zoom

Sterile neutrinos with masses around a few keV have been postulated to be viable dark matter candidates.

Wednesday, May 27, 2020

1:30pm

- 2:30pm

Zoom

In this talk, I will review a framework for finding the conservative potential of compact binary systems using scattering amplitudes and effective field theory.

Friday, May 29, 2020

12:30pm

- 1:30pm

Zoom

I will describe a new method to compute and constrain the possible shapes of primordial correlation functions from inflation.