2 What Can Be Learned with a Lead - Based Supernova - Neutrino Detector ?
نویسنده
چکیده
We examine the prospects for using lead as a supernova-neutrino detector by considering the spectrum of electrons produced, and the number of oneand two-neutron events. We show that the electron energy spectrum from charged-current reactions can be used to extract information about the high-temperature component of the neutrino spectrum. Some degree of electron neutrino oscillation is expected in the supernova envelope. We examine the prospects for untangling the signatures of various oscillation scenarios, including, e.g. normal or inverted hierarchies, and different values for the small mixing angle θ13.
منابع مشابه
ar X iv : h ep - p h / 02 09 26 7 v 1 2 3 Se p 20 02 What Can Be Learned with a Lead - Based Supernova - Neutrino Detector ?
We examine the prospects for using lead as a supernova-neutrino detector by considering the spectrum of electrons produced, and the number of oneand two-neutron events. We show that the electron energy spectrum from charged-current reactions can be used to extract information about the high-temperature component of the neutrino spectrum. Some degree of electron neutrino oscillation is expected ...
متن کاملLANNDD - A Massive Liquid Argon Detector for Proton Decay, Supernova and Solar Neutrino Studies and a Neutrino Factory Detector
We describe a possible Liquid Argon Neutrino and Nucleon Decay Detector (LANNDD) that consists of a 70 kT magnetized liquid Argon tracking detector. The detector is being designed for the Carlsbad Underground Laboratory. The major scientific goals are: 1) Search for μ + ν + → K p to 10 years lifetime 2) Detection of large numbers of solar neutrino events and supernova events 3) Study of atmosph...
متن کاملar X iv : a st ro - p h / 03 08 23 9 v 2 1 8 A ug 2 00 3 Neutrino signatures of the supernova - gamma ray burst relationship
We calculate the TeV-PeV neutrino fluxes of gamma-ray bursts associated with supernovae, based on the observed association between GRB 030329 and supernova SN 2003dh. The neutrino spectral flux distributions can test for possible delays between the supernova and the gamma-ray burst events down to much shorter timescales than what can be resolved with photons. As an illustrative example, we calc...
متن کاملar X iv : a st ro - p h / 03 08 23 9 v 1 1 3 A ug 2 00 3 Neutrino signatures of the supernova - gamma ray burst relationship
We calculate the TeV-PeV neutrino fluxes of gamma-ray bursts associated with supernovae, based on the observed association between GRB 030329 and supernova SN 2003dh. The neutrino spectral flux distributions can test for possible delays between the supernova and the gamma-ray burst events down to much shorter timescales than what can be resolved with photons. As an illustrative example, we calc...
متن کاملar X iv : a st ro - p h / 03 08 23 9 v 3 1 4 O ct 2 00 3 Neutrino signatures of the supernova - gamma ray burst relationship
We calculate the TeV-PeV neutrino fluxes of gamma-ray bursts associated with supernovae, based on the observed association between GRB 030329 and supernova SN 2003dh. The neutrino spectral flux distributions can test for possible delays between the supernova and the gamma-ray burst events down to much shorter timescales than what can be resolved with photons. As an illustrative example, we calc...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2008