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Physics & Astronomy Colloquium

Physics and Astronomy Colloquium: Neutrinos from Nuclear Reactors: Searches and Surprises

Nuclear reactors are very bright sources of neutrinos. The radioactive fission products are neutron rich, and beta decay back to the valley of stability while emitting (electron anti-)neutrinos along the way. This was how the neutrino was discovered, and how we verified that neutrino oscillations explained the Solar Neutrino Problem. More recently, the Daya Bay Reactor Neutrino Experiment discovered a new mode of neutrino oscillation, and the PROSPECT experiment is being planned to search for "sterile" neutrinos.



This talk will first review the basics of neutrinos, their detection, neutrino oscillations, and nuclear reactors as neutrino sources. We'll then take a tour of recent results and next steps, including some surprises in what we've learned about the reactor neutrino source itself.

 

Refreshments will be served in CP 179 at 3:15 PM

Date:
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Location:
CP155

Colloquium: The many facets of strongly coupled QFT: from QCD to Cosmology

Abstract: Quantum Field Theory is a universal language to describe a multitude of physical phenomena from elementary particle and condensed matter physics. Often apparent complexity of the described phenomena is attributed to strong coupling in the underlying QFT. Accordingly, understanding strongly-coupled dynamics became a universal theoretical challenge relevant for many areas of contemporary physics. Remarkably, the past decade was characterized by an accelerated development of several original approaches to this problem, leading to a plethora of new results. In my talk I will focus on several non-pertubative methods, most notably holographic correspondence, and describe recent progress and hot research topics. Refreshments will be served in CP 179 at 3:15 PM

Date:
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The Universe as a Detector: What can we learn about fundamental physics from Cosmology?

 

 

Dr. Harsh Mathur Case Western Reserve University The imprint of primordial gravitational radiation on the cosmic microwave background polarization, if observed, is considered smoking gun proof of inflation. I will discuss how such an observation can not only provide information about the Universe in the epoch of inflation but also constrain theories of grand unification. In the second part of the talk I will discuss tests of gravity on scales ranging from the tabletop to the cosmological scale. Such tests may shed light on physics beyond the standard model.

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