Dynamos in Accretion Disks: A general review and some moderately biased comments Chicago - October 2003.
Supernova. Explosions Stars may explode cataclysmically. –Large energy release (10 3 – 10 6 L ) –Short time period (few days) These explosions used.
1 Detecting Supernova Neutrinos X.-H. Guo Beijing Normal University.
Modelling SN Type II: collapse and simple bounce From Woosley et al. (2002) Woosley Lectures 13 and 14.
Gravitational waves and neutrino emission from the merger of binary neutron stars Kenta Kiuchi Collaboration with Y. Sekiguchi, K. Kyutoku, M. Shibata.
Anti-Correlated Lags in Compact Stellar X-ray Sources Dr. Kandulapati Sriram Collaborators: Prof A. R. Rao (TIFR) Dr. Vivek Kumar Agrawal (ISRO/TIFR).
1 Testing Modified gravity and gravitational waves Takahiro Tanaka (Dept. of Phys./YITP Kyoto university) Gravitational waves.
Coincident search for gravitational-wave and neutrino signals from core-collapse supernovae L. Cadonati (U Mass, Amherst), E. Coccia (LNGS and U Rome II),
Determining the Neutrino Hierarchy From a Galactic Supernova David Webber APS April Meeting May 3, 2011 SN 1572 “Tycho’s Nova” 7,500 light years (2.3 kPc)
Detection of the Diffuse Supernova Neutrino Background in LENA & Study of Scintillator Properties Michael Wurm DPG Spring Meeting, 30.3.06 E15.
1 Relativistic Time Measurements and Other Experiments Require Going Beyond Einstein to the Yilmaz Theory of Gravity Carroll Alley Department of Physics.
Core-collapse Supernovae, Neutrinos, and the OMNIS project.