Expected and Achievable Accuracy in Estimating Parameters of Standing Accretion Shock Instability (SASi) Fluctuations from Neutrinos and Gravitational Wave Oscillations

Faculty Mentor Name

Michele Zanolin, Cecilia Lunardini (ASU), Kei Kotake (Fukuoka, Japan)

Document Type

Presentation

Location

Jim and Linda Lee Planetarium

Start Date

5-10-2018 3:10 PM

End Date

5-10-2018 3:20 PM

Abstract

Core collapse supernovae are one of the most interesting sources of gravitational waves. When the progenitor star is particularly massive, hydrodynamic instability called standing accretion shock instability can develop and it is characterized by deterministic oscillations in the gravitational wave signal as well as in the neutrino luminosity with frequencies of 100hz. In this talk we will review current efforts to extract physical information from the SASI components of the gravitational wave and enhance the detectability of gravitational waves with such components both using laser interferometers and neutrino detectors.

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Oct 5th, 3:10 PM Oct 5th, 3:20 PM

Expected and Achievable Accuracy in Estimating Parameters of Standing Accretion Shock Instability (SASi) Fluctuations from Neutrinos and Gravitational Wave Oscillations

Jim and Linda Lee Planetarium

Core collapse supernovae are one of the most interesting sources of gravitational waves. When the progenitor star is particularly massive, hydrodynamic instability called standing accretion shock instability can develop and it is characterized by deterministic oscillations in the gravitational wave signal as well as in the neutrino luminosity with frequencies of 100hz. In this talk we will review current efforts to extract physical information from the SASI components of the gravitational wave and enhance the detectability of gravitational waves with such components both using laser interferometers and neutrino detectors.