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Wipro Supernova

Wipro Supernova is the name of a series of high-performance computing (HPC) solutions offered by Wipro Infotech.
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Papers overview

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Highly Cited
2015
Highly Cited
2015
A TWO-PARAMETER CRITERION FOR CLASSIFYING THE EXPLODABILITY OF MASSIVE STARS BY THE NEUTRINO-DRIVEN MECHANISM
Thus far, judging the fate of a massive star (either a neutron star [NS] or a black hole) solely by its structure prior to core… 
Review
2011
Review
2011
THE COSMIC CORE-COLLAPSE SUPERNOVA RATE DOES NOT MATCH THE MASSIVE-STAR FORMATION RATE
We identify a “supernova rate problem:” the measured cosmic core-collapse supernova rate is a factor of ∼2 smaller (with… 
Highly Cited
2010
Highly Cited
2010
Cooling neutron star in the Cassiopeia A supernova remnant: evidence for superfluidity in the core
According to recent results of Ho & Heinke, the Cassiopeia A supernova remnant contains a young (?330-yr-old) neutron star (NS… 
Review
2006
Review
2006
MAGPIS: A Multi-Array Galactic Plane Imaging Survey
We present the Multi-Array Galactic Plane Imaging Survey (MAGPIS), which maps portions of the first Galactic quadrant with an… 
Highly Cited
2003
Highly Cited
2003
Small-Scale Structure of the SN 1006 Shock with Chandra Observations
The northeast shell of SN 1006 is the most probable acceleration site of high-energy electrons (up to ~100 TeV) with the Fermi… 
Highly Cited
2001
Highly Cited
2001
Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic field
The maximum energy for cosmic ray acceleration at supernova shock fronts is usually thought to be limited to around 10 14 ±10 15… 
Highly Cited
1996
Highly Cited
1996
Constraints on Stellar Grain Formation from Presolar Graphite in the Murchison Meteorite
We report the results of isotopic, chemical, structural, and crystallographic microanalyses of graphitic spherules (0.3-9 μm… 
Highly Cited
1995
Highly Cited
1995
Discovery of explosion fragments outside the Vela supernova remnant shock-wave boundary
THE nearby (500 pc) Vela supernova remnant has presented several puzzles. Its true shape has been difficult to determine1, and as… 
Highly Cited
1993
Highly Cited
1993
The progenitor of supernova 1993J: a stripped supergiant in a binary system?
SUPERNOVA 1993J in the spiral galaxy M81 is the brightest supernova since SN1987A and, like the latter, appears to be another… 
Highly Cited
1983
Highly Cited
1983
Liquid–gas phase transition in nuclear matter
Every self-bound Fermi liquid will exhibit a liquid–gas phase equilibrium at low temperatures, because the pressure is positive… 
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