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W Bauer Slide 1 Neutrinos Double Beta Decay and Supernova Dynamics Wolfgang Bauer Michigan State University W Bauer Slide 2 1 meVc2 1 eVc2 1 keVc2 1 MeVc2 1 GeVc2 1 TeVc2…
talk_CapozziSupernova Neutrinos in the Standard Model Francesco Capozzi Francesco Capozzi - Virginia Tech 2 What are supernovae? When nuclear fuel ends, massive stars (>
Supernova neutrinos - Collective and matter effects at large detectorsAmol Dighe Changing paradigm of SN neutrino oscillations Neutrino-electron forward scattering: MSW effects
The sixth Astrophysical Multimessenger Observatory NetworkAMON Workshop May 22, 2019 Detection of supernova neutrinos at Super-Kamiokande 1 M. Nakahata Kamioka Observatory,…
Effects of sterile neutrinos on supernova and UHE neutrino fluxes Jukka Maalampi University of Jyväskylä AlbaNova, Stockholm April 16, 2004 Contents Backgound Sterile neutrinos?…
Neutrinos as a Unique Probe: 10−33 − 10+28 cm • Particle Physics – νN, µN, eN scattering: existence/properties of quarks, QCD – Weak
New supernova neutrino spectrum Gleb Sinev LArSoft Coordination Meeting April 12, 2016 2016412 New supernova neutrino spectrum 2 New SNν energy spectrum ● Original spectrum…
2. Double Beta Decays Neutrinos2. Double Beta Decays Neutrinos ––Present Status--Present Status-- Hiro Ejiri, JASRI Spring-8 RCNP Osaka Univ. April 2003, TIT ContentsContents…
Neutrinoless Double Beta Decay • 2νββ • Standard Model process • Emits two neutrinos which carry away energy • 0νββ • Violates lepton number • Signal at…
Neutrinoless Double Beta Decay and Particle Physics Werner Rodejohann MPIK, Heidelberg 01102012 1 2 Outline A,Z → A,Z + 2 + 2 e− 0νββ ⇒ Lepton Number Violation •…
NeutrinolessNeutrinoless doubledouble--ββ decaydecay Giorgio Gratta Physics Dept, Stanford SSI, August 2009 Double-Beta decay 2 ⎟ ⎟ ⎠ ⎞ ⎜ ⎜ ⎝ ⎛ •⎟ ⎟…
Slide 1 Supernova Watches and HALO SNOLAB Grand Opening Workshop May 14-16, 2012 Clarence J. Virtue Supernova neutrinos – First order expectations Approximate equipartition…
GADZOOKS! project at Super-Kamiokande MIkeda Kamioka ICRR Uof Tokyo for Super-K collaboration 201569@WIN2015 1 Contents • GADZOOKS! project • Supernova Relic Neutrino…
Light Sterile Neutrinos and Neutrinoless Double-Beta Decay Carlo Giunti INFN, Torino, Italy MEDEX’17 Matrix Elements for the Double-beta-decay EXperiments Prague, Czech…
Interactions SNR/MC Supernova remnants and molecular clouds Armand Fiasson LAPP - Annecy-le-vieux Where CRs originate? The usual suspects up to the knee are supernova remnants…
Slide 1 Microscopic Modeling of Supernova Matter Igor Mishustin FIAS, J. W. Goethe University, Frankfurt am Main, Germany and National Research Center “Kurchatov Institute”,…
26 The Messenger 167 – March 2017 made famous by HST, Chandra and ATCA images (see Figure 1, left), is readily visible in images from NAOS-CONICA (NACO), and the Spectrograph
H elium A nd L ead O bservatory A lead detector for supernova neutrinos in SNOLAB no nuclear energy from iron core → core collapse The end of a massive star's life:…
Near IR Emission from Supernova Remnants John Raymond Rho et al. IC 443 JHK Why do J and H come from a completely different region than K? Supernova Remnants X-rays T >…
Physics Potential of Future Supernova Neutrino ObservationsAmol Dighe Neutrino 2008 May 25-31, 2008, Christchurch, New Zealand Supernova for neutrino physics and astrophysics