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Simulating the Supernova Neutrinosphere with Heavy Ion Collisions

Registration closed 24/03/2014.

Secretariat

Ines Campo
+39 0461 314721
Monday, 7 April, 2014 - 09:00 to Friday, 11 April, 2014 - 17:00
Abstract: 

The aim of the workshop is to explore reproducing supernova neutrinosphere conditions in the laboratory using heavy ion collisions with radioactive beams. Much of the "action" in core collapse supernovae happens near the neutrinosphere. This surface of last scattering is a warm low-­density gas of neutron rich matter. By studying this gas, its composition, correlations, and equation of state in the laboratory, one will be able to make better predictions for supernova neutrino spectra and nucleosynthesis. The workshop will involve heavy ion experimentalists and theorists, many-body theorists, astrophysicists, and neutrino physicists.

Registration period: 
03 Feb 2014 to 23 Mar 2014

Organizers

C. Horowitz Indiana University
J. Natowitz Texas A&M University
L. Roberts Caltech
H. Wolter University of Munich

Attendees

Last nameFirst nameInstitutionCountry of Institution
BarbuiMarinaCycoltron Institute, TAMUTexas, USA
BlaschkeDavidUniversity of WroclawPoland
bonaseraaldoINFN &Cycl inst. Texas A&MItalia
BonnetEricGANILFrance
ChbihiAbdelouahadGANILFrance
FischerTobiasInstitute of Theoretical Physics, University of WroclawPoland
FrohlichCarlaNorth Carolina State UniversityUSA
GaitanosTheodorosInstitut für Theoretische Physik IGermany
HagelKrisCyclotron Institute, Texas A & M UniversityUnited States
HempelMatthiasBasel UniversitySwitzerland
HorowitzCharlesIndiana UniversityUnited States
LentzEricUniversity of Tennessee, KnoxvilleUSA
LiQingfengSchool of Science, Huzhou Teachers CollegeZhejiang Province, P.R. China
LynchWilliamMichigan State UniversityUSA
Martinez-PinedoGabrielTU DarmstadtGermany
McLaughlinGailNorth Carolina State UniversityUSA
MuellerBernhardMonash UniversityAustralia
MukherjeeAbhishekECT*Italy
MurphyJeremiahDepartment of Physics, Florida State UniversityUnited States of America
NapolitaniPaoloInstitut de Physique Nucléaire d'Orsay (IPN)France
NatowitzJosephTexas A&M UniversityUS
O'ConnorEvanCanadian Institute of Theoretical AstrophysicsCanada
OnoAkiraTohoku UniversityJapan
PasquaAntonioUniversity of TriesteItaly
RadutaAdrianaIFIN-HHRomania
reddysanjayInstitute for Nuclear Theory, Uni. of WashingtonUSA
RobertsLukeCalifornia Institute of TechnologyUSA
RoepkeGerdUniversity of Rostock, Institut fuer PhysikGermany
SagertIrinaIndiana UniversityUSA
ShenGangTechnische University DarmstadtGermany
ShlomoShalomTexas A&M UniversityUSA
TrautmannWolfgangGSI Helmholtzzentrum DarmstadtGermany
TypelStefanGSI Helmholtzzentrum fuer Schwerionenforschung GmbHGermany
VerdeGiuseppeINFN, CataniaItaly
WanajoShinyaNational Astronomical Observatory of JapanJapan
WolterHermannUniversity of MunichGermany
WuosmaaAlanUniversity of ConnecticutUSA
YennelloSherryTexas A&M UniversityUSA