Results 261 to 270 of about 155,831 (295)

Mathematical Modeling of Physical Reality: From Numbers to Fractals, Quantum Mechanics and the Standard Model. [PDF]

Entropy (Basel)
Kupczynski M.
europepmc   +1 more source

Radiative heating achieves the ultimate regime of thermal convection. [PDF]

Proc Natl Acad Sci U S A, 2018
Lepot S, Aumaître S, Gallet B.
europepmc   +1 more source

Primordial black holes and their gravitational-wave signatures. [PDF]

Living Rev Relativ
Bagui E, Clesse S, De Luca V, Ezquiaga JM, Franciolini G, García-Bellido J, Joana C, Kumar Jain R, Kuroyanagi S, Musco I, Papanikolaou T, Raccanelli A, Renaux-Petel S, Riotto A, Ruiz Morales E, Scalisi M, Sergijenko O, Ünal C, Vennin V, Wands D, LISA Cosmology Working Group.   +20 more
europepmc   +1 more source

Infused ice can multiply IceCube's sensitivity. [PDF]

Nat Commun, 2018
Bartos I, Marka Z, Marka S.
europepmc   +1 more source

Strongest gravitational waves from neutrino oscillations at supernova core bounce [PDF]

, 2004
Herman J. Mosquera Cuesta, K. Fiuza
openalex  

Some of the next articles are maybe not open access.

Related searches:

Neutrinos and Supernovae

AIP Conference Proceedings, 2008
Core‐collapse supernovae are one of the few astrophysical environments in which neutrinos play a dominant role. Neutrinos emission is the means by which a newly‐born neutron star formed in a core‐collapse event cools. Neutrinos may play a significant role in causing the supernova explosion. Finally neutrinos may significantly affect the nucleosynthesis
Bradley S. Meyer, P. Demetriou, R. Julin, S. V. Harissopulos   +3 more
openaire   +2 more sources

Supernova neutrinos and their oscillations

Physical Review D, 1988
Three-neutrino oscillations, both in a vacuum and in matter, are applied to the supernova neutrino flux. It is found that oscillations can change the flux substantially, reducing the number of directional events in the Kamioka nucleon-decay experiment and increasing the number of isotropic events in the Irvine-Michigan-Brookhaven experiment.
James T. Pantaleone, Tzee-Ke Kuo
openaire   +3 more sources

Neutrino Heating in Supernovae

Physical Review Letters, 1988
I argue that standard descriptions of stellar collapse omit the primary mechanism for dissipative neutrino reactions in nuclear matter, nuclear excitation by neutral-current scattering. The nuclear heating rate, due to primarily to muon- and tauon-neutrino excitation of giant resonance states, is on the order of 90 MeV/nucleon sec at a radius of 100 km.
openaire   +3 more sources

SUPERNOVA NEUTRINOS

Neutrino Oscillations and Their Origin, 2002
We propose that neutrino-proton elastic scattering, {nu} + p {yields} {nu} + p, can be used for the detection of supernova neutrinos. Though the proton recoil kinetic energy spectrum is soft, with T{sub p} {approx_equal} 2E{sub {nu}}{sup 2}/M{sub p}, and the scintillation light output from slow, heavily ionizing protons is quenched, the yield above a ...
openaire   +1 more source

Neutrinos from Supernovae

Space Science Reviews, 2018
Neutrinos are fundamental particles in the collapse of massive stars. Because of their weakly interacting nature, neutrinos can travel undisturbed through the stellar core and be direct probes of the still uncertain and fascinating supernova mechanism. Intriguing recent developments on the role of neutrinos during the stellar collapse are reviewed, as ...
Tamborra, Irene, Murase, Kohta
openaire   +3 more sources