[Theory-seminars] FW: Physics Colloquium for Friday, September 18, "Particle vortex statistics and phases of dense matter" - Srimoyee Sen

Mary Fox mfox at jlab.org
Mon Sep 14 18:22:18 EDT 2020



From: Wilkinson, Ellie V <evwilk at wm.edu>
Sent: Monday, September 14, 2020 9:23 AM
To: physics2017 at physics.wm.edu
Cc: undergrads2017 at physics.wm.edu
Subject: [EXTERNAL] Physics Colloquium for Friday, September 18, "Particle vortex statistics and phases of dense matter" - Srimoyee Sen

[A person posing for the camera  Description automatically generated]Physics Colloquium                                                Srimoyee Sen [Host: C. Monahan]
Friday, September 18, 2020                                     Iowa State University
4:00 PM                                                                   "Particle vortex statistics and the phases of dense matter"

Zoom Link:    https://cwm.zoom.us/j/97377816824<https://urldefense.proofpoint.com/v2/url?u=https-3A__cwm.zoom.us_j_97377816824&d=DwMFAg&c=CJqEzB1piLOyyvZjb8YUQw&r=NXc6ETf15Ad2OT-P0W4YLg&m=85ZnIt97TtTeWdC-YSV9NggAJyibvbP-7TOo7DjvPco&s=AfU7jIgw_zVfGKi53F9eaGOIVuTJU6mI8fPJ9tNXeRI&e=>



Abstract:
Neutron stars are extremely dense objects where atomic nuclei dissolve to produce extended soup of nucleons/baryons. Recent observation of neutron star mergers through gravitational waves has given rise to vigorous research activity in this area. In order to make progress in understanding neutron stars, it is of utmost importance to understand the properties of such dense matter as well as accurately model its equation of state. In this talk I discuss the various patterns of organizations expected to arise in dense baryonic matter and how modern developments in topological phase transitions in condensed matter systems combined with perturbative techniques in quantum chromodynamics, the theory of strong interactions, can inform our knowledge in this regard.

Cheers,
Ellie Wilkinson
William & Mary Physics
Administrative Coordinator

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