Summer Seminar: Mauricio Bustamante and Stephan Frank

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July 5, 2016
11:30AM - 12:30PM
Location
MP 4054

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Add to Calendar 2016-07-05 11:30:00 2016-07-05 12:30:00 Summer Seminar: Mauricio Bustamante and Stephan Frank "Probing neutrino lifetime using high-energy astrophysical neutrinos"Mauricio Bustamante (Physics)In theories beyond the Standard Model, neutrinos may be unstable and decay with rates that have detectable effects. The cumulative effect of decay on a neutrino flux will be larger the longer the neutrino travel time, or baseline. Therefore, the high-energy (10 TeV -- 2 PeV) astrophysical neutrinos recently discovered by IceCube --- with estimated baselines from several megaparsecs to a few gigaparsecs --- are fertile ground to test decay. I will show how decay distorts the flavor composition of these neutrinos and the rate of neutrino-induced showers. Using these observables, existing and near-future IceCube data improve the lifetime bounds by several orders of magnitude, in the normal and inverted neutrino mass hierarchy. "Introducing Agnostic Spectral Stacking as a Powerful Method to detect and characterise Weak QSO Absorber Populations"Stephan Frank (Astronomy)We have developed a new spectral stacking method that allows for the detection and characterisation of absorber populations that are individually too weak to be detected by traditional line search methods. I will demonstrate how this technique works for the specific case of searching for signatures of NeVIII absorbers, thought to arise in warm to hot circumgalactic gas, at intermediate redshifts (z=0.7-1.2) in an ensemble of high-quality COS-spectra. MP 4054 Center for Cosmology and AstroParticle Physics (CCAPP) ccapp@osu.edu America/New_York public
Description

"Probing neutrino lifetime using high-energy astrophysical neutrinos"

Mauricio Bustamante (Physics)

In theories beyond the Standard Model, neutrinos may be unstable and decay with rates that have detectable effects. The cumulative effect of decay on a neutrino flux will be larger the longer the neutrino travel time, or baseline. Therefore, the high-energy (10 TeV -- 2 PeV) astrophysical neutrinos recently discovered by IceCube --- with estimated baselines from several megaparsecs to a few gigaparsecs --- are fertile ground to test decay. I will show how decay distorts the flavor composition of these neutrinos and the rate of neutrino-induced showers. Using these observables, existing and near-future IceCube data improve the lifetime bounds by several orders of magnitude, in the normal and inverted neutrino mass hierarchy.

 

"Introducing Agnostic Spectral Stacking as a Powerful Method to detect and characterise Weak QSO Absorber Populations"

Stephan Frank (Astronomy)

We have developed a new spectral stacking method that allows for the detection and characterisation of absorber populations that are individually too weak to be detected by traditional line search methods. I will demonstrate how this technique works for the specific case of searching for signatures of NeVIII absorbers, thought to arise in warm to hot circumgalactic gas, at intermediate redshifts (z=0.7-1.2) in an ensemble of high-quality COS-spectra.

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