November 2017

Wednesday, November 1, 2017

1:30pm

- 3:00pm

Friday, November 3, 2017

12:30pm

- 2:00pm

As our astrophysical understanding of dark matter reaches smaller scales, what deviations from standard astrophysical models of dark matter could we hope to search for?

Wednesday, November 8, 2017

1:30pm

- 3:00pm

I will briefly review the motivation for the existence of new physics in the neutrino sector and I will describe a few different ways of looking for such new physics.

Wednesday, November 15, 2017

1:30pm

- 3:00pm

Cascade decays are prevalent in high energy physics, and are, in particular, a hallmark of many new physics models. The masses of particles in the decay chain can be measured using kinematic

Friday, November 17, 2017

12:30pm

- 2:00pm

Wednesday, November 29, 2017

1:30pm

- 3:00pm

Current all-orders proofs of factorization of hard processes

are made by extracting the leading power behavior of Feynman graphs,

i.e., by extracting asymptotics strictly order-by-order in perturbation

are made by extracting the leading power behavior of Feynman graphs,

i.e., by extracting asymptotics strictly order-by-order in perturbation

November 2017

Wednesday, November 1, 2017

1:30pm

- 3:00pm

Friday, November 3, 2017

12:30pm

- 2:00pm

As our astrophysical understanding of dark matter reaches smaller scales, what deviations from standard astrophysical models of dark matter could we hope to search for?

Wednesday, November 8, 2017

1:30pm

- 3:00pm

I will briefly review the motivation for the existence of new physics in the neutrino sector and I will describe a few different ways of looking for such new physics.

Wednesday, November 15, 2017

1:30pm

- 3:00pm

Cascade decays are prevalent in high energy physics, and are, in particular, a hallmark of many new physics models. The masses of particles in the decay chain can be measured using kinematic

Friday, November 17, 2017

12:30pm

- 2:00pm

Wednesday, November 29, 2017

1:30pm

- 3:00pm

Current all-orders proofs of factorization of hard processes

are made by extracting the leading power behavior of Feynman graphs,

i.e., by extracting asymptotics strictly order-by-order in perturbation

are made by extracting the leading power behavior of Feynman graphs,

i.e., by extracting asymptotics strictly order-by-order in perturbation