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Dynamos in Accretion Disks: A general review and some moderately biased comments Chicago - October 2003.
Documents Dynamos in Accretion Disks: A general review and some moderately biased comments Chicago - October.....

Slide 1Dynamos in Accretion Disks: A general review and some moderately biased comments Chicago - October 2003 Slide 2 What is an Accretion Disk? Flattened, rotionally supported,…

Supernova. Explosions Stars may explode cataclysmically. –Large energy release (10 3 – 10 6 L ) –Short time period (few days) These explosions used.
Documents Supernova. Explosions Stars may explode cataclysmically. –Large energy release (10 3 – 10 6 L )...

Slide 1 Supernova Slide 2 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.
Documents 1 Detecting Supernova Neutrinos X.-H. Guo Beijing Normal University.

Slide 1 1 Detecting Supernova Neutrinos X.-H. Guo Beijing Normal University Slide 2 2 Contents I. SN neutrinos’ production and propagation II. Detection of SN neutrinos…

Modelling SN Type II: collapse and simple bounce From Woosley et al. (2002) Woosley Lectures 13 and 14.
Documents Modelling SN Type II: collapse and simple bounce From Woosley et al. (2002) Woosley Lectures 13 and....

Slide 1 Modelling SN Type II: collapse and simple bounce From Woosley et al. (2002) Woosley Lectures 13 and 14 Slide 2 Most distant explosion smashes previous record NASA…

Gravitational waves and neutrino emission from the merger of binary neutron stars Kenta Kiuchi Collaboration with Y. Sekiguchi, K. Kyutoku, M. Shibata.
Documents Gravitational waves and neutrino emission from the merger of binary neutron stars Kenta Kiuchi...

Gravitational waves and neutrino emission from the merger of binary neutron stars Gravitational waves and neutrino emission from the merger of binary neutron stars Kenta…

Anti-Correlated Lags in Compact Stellar X-ray Sources Dr. Kandulapati Sriram Collaborators: Prof A. R. Rao (TIFR) Dr. Vivek Kumar Agrawal (ISRO/TIFR).
Documents Anti-Correlated Lags in Compact Stellar X-ray Sources Dr. Kandulapati Sriram Collaborators: Prof A.....

Anti-Correlated Lags in Compact Stellar X-ray Sources Dr. Kandulapati Sriram Collaborators: Prof A. R. Rao (TIFR) Dr. Vivek Kumar Agrawal (ISRO/TIFR). Dr. Ranjeev Misra (IUCAA)…

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)
Documents Determining the Neutrino Hierarchy From a Galactic Supernova David Webber APS April Meeting May 3,.....

Slide 1 Determining the Neutrino Hierarchy From a Galactic Supernova David Webber APS April Meeting May 3, 2011 SN 1572 âTychoâs Novaâ 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.
Documents Detection of the Diffuse Supernova Neutrino Background in LENA & Study of Scintillator Properties...

Detection of the Diffuse Supernova Neutrino Background in LENA & Study of Scintillator Properties Michael Wurm DPG Spring Meeting, 30.3.06 Neutrinos from Supernovae Detection…

Core-collapse Supernovae, Neutrinos, and the OMNIS project.
Documents Core-collapse Supernovae, Neutrinos, and the OMNIS project.

The 7 stages of Core Collapse... For a ~10M star… Stage Temp (K) Ashes Duration H burning 2x107 He few x 106 yrs He 2x108 C, O few x 104 yrs C 8x108 Ne, O ~600 yrs Ne…

Dark Matter and the Equivalence Principle
Documents Dark Matter and the Equivalence Principle

Dark Matter and the Equivalence Principle Marc Kamionkowski Caltech (work done with Michael Kesden, astro-ph/0606566 [PRL], 0608095) 20 September 2006 Aristotle (384-322…

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