He thought the theory sounded plausible and developed a new way to describe neutrino
physics in supernovae, working on newly available $ 25 million supercomputers at the Max Planck Institute, one of the few places in Europe where the computers were available for unclassified research.
Not exact matches
Further studies of SN 2009ip and its aftermath will help tease out the
physics of these exotic
supernovae, says Armin Rest, an astronomer at the Space Telescope Science Institute
in Maryland, who was not part of the study team.
Although previous
supernovas have been seen this early, the new observation is the earliest one with a spectrum — an accounting of the emitted light broken up by wavelength — taken six hours after the explosion, Yaron and colleagues report online February 13
in Nature
Physics.
An international collaboration led by the Kavli Institute for the
Physics and Mathematics of the Universe (Kavli IPMU) have discovered that the color of
supernovae during a specific phase could be an indicator for detecting the most distant and oldest
supernovae in the Universe — more than 13 billion years old.
Gravitational waves might also reveal some of the
physics of the strange stew of neutrons that makes up a protoneutron star — the beginnings of an incredibly dense star formed
in a
supernova.
«Currently, Super-Kamiokande can detect neutrinos from
supernova explosions anywhere
in our own Milky Way galaxy,» says Vagins, of the Kavli Institute for the
Physics and Mathematics of the Universe.
The current technique, based on
supernovas, garnered three cosmologists the 2011 Nobel prize
in physics.
Dr David Sloan, Co-author and Post-Doctoral Research Associate
in the Department of
Physics at Oxford University, said: «A lot of previous work has focused on «doomsday» scenarios on Earth — astrophysical events like
supernovae that could wipe out the human race.
«Some stars get the boot when their companion star explodes
in a
supernova, and others can get kicked out of crowded star clusters,» says William Chick, a UW doctoral student
in physics, who presented his team's new results Jan. 5 at the 227th American Astronomical Society meeting
in Kissimmee, Fla. «The gravitational boost increases a star's speed relative to other stars.»
Saul Perlmutter, Brian Schmidt and Adam Reiss share the 2011 Nobel Prize
in Physics for their observations that type Ia
supernovae indicate that the expansion of the universe is accelerating.
There were several observations that suggested the accelerated cosmic expansion, including distant
supernovae for which the 2011 Nobel Prize
in Physics was awarded.
Understanding the
physics of these astrophysical objects is crucial as they are considered as the possible progenitors of thermonuclear
supernovae, being used
in cosmology to measure the acceleration of the universe expansion linked to dark energy.
Type 1a
supernovae have already played a profound role at the Keck Observatory when a team of astronomers were awarded the 2011 Nobel Prize
in Physics.
Specifically, the NuStar will map radioactive material
in supernovae remnants
in an attempt to study the origins of cosmic rays and extreme
physics surrounding collapsed stars.