These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.


BIOMARKERS

Molecular Biopsy of Human Tumors

- a resource for Precision Medicine *

187 related articles for article (PubMed ID: 20866956)

  • 1. Self-refraction of supernova neutrinos: mixed spectra and three-flavor instabilities.
    Friedland A
    Phys Rev Lett; 2010 May; 104(19):191102. PubMed ID: 20866956
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Coherent development of neutrino flavor in the supernova environment.
    Duan H; Fuller GM; Carlson J; Qian YZ
    Phys Rev Lett; 2006 Dec; 97(24):241101. PubMed ID: 17280265
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Charged-current weak interaction processes in hot and dense matter and its impact on the spectra of neutrinos emitted from protoneutron star cooling.
    Martínez-Pinedo G; Fischer T; Lohs A; Huther L
    Phys Rev Lett; 2012 Dec; 109(25):251104. PubMed ID: 23368446
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Flavor evolution of the neutronization neutrino burst from an O-Ne-Mg core-collapse supernova.
    Duan H; Fuller GM; Carlson J; Qian YZ
    Phys Rev Lett; 2008 Jan; 100(2):021101. PubMed ID: 18232846
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Multiple spectral splits of supernova neutrinos.
    Dasgupta B; Dighe A; Raffelt GG; Smirnov AY
    Phys Rev Lett; 2009 Jul; 103(5):051105. PubMed ID: 19792481
    [TBL] [Abstract][Full Text] [Related]  

  • 6. Flavor oscillations in the supernova hot bubble region: nonlinear effects of neutrino background.
    Pastor S; Raffelt G
    Phys Rev Lett; 2002 Nov; 89(19):191101. PubMed ID: 12443110
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Neutrino mass hierarchy and stepwise spectral swapping of supernova neutrino flavors.
    Duan H; Fuller GM; Carlson J; Qian YZ
    Phys Rev Lett; 2007 Dec; 99(24):241802. PubMed ID: 18233438
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Signals of the QCD phase transition in core-collapse supernovae.
    Sagert I; Fischer T; Hempel M; Pagliara G; Schaffner-Bielich J; Mezzacappa A; Thielemann FK; Liebendörfer M
    Phys Rev Lett; 2009 Feb; 102(8):081101. PubMed ID: 19257729
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Instability in the dense supernova neutrino gas with flavor-dependent angular distributions.
    Mirizzi A; Serpico PD
    Phys Rev Lett; 2012 Jun; 108(23):231102. PubMed ID: 23003940
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Neutrino scattering and flavor transformation in supernovae.
    Cherry JF; Carlson J; Friedland A; Fuller GM; Vlasenko A
    Phys Rev Lett; 2012 Jun; 108(26):261104. PubMed ID: 23004955
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Collisional Triggering of Fast Flavor Conversions of Supernova Neutrinos.
    Capozzi F; Dasgupta B; Mirizzi A; Sen M; Sigl G
    Phys Rev Lett; 2019 Mar; 122(9):091101. PubMed ID: 30932530
    [TBL] [Abstract][Full Text] [Related]  

  • 12. Axial symmetry breaking in self-induced flavor conversionof supernova neutrino fluxes.
    Raffelt G; Sarikas S; de Sousa Seixas D
    Phys Rev Lett; 2013 Aug; 111(9):091101. PubMed ID: 24033018
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Mu-Tau Neutrinos: Influencing Fast Flavor Conversions in Supernovae.
    Capozzi F; Chakraborty M; Chakraborty S; Sen M
    Phys Rev Lett; 2020 Dec; 125(25):251801. PubMed ID: 33416371
    [TBL] [Abstract][Full Text] [Related]  

  • 14. Suppression of self-induced flavor conversion in the supernova accretion phase.
    Sarikas S; Raffelt GG; Hüdepohl L; Janka HT
    Phys Rev Lett; 2012 Feb; 108(6):061101. PubMed ID: 22401048
    [TBL] [Abstract][Full Text] [Related]  

  • 15. Roles of Fast Neutrino-Flavor Conversion on the Neutrino-Heating Mechanism of Core-Collapse Supernova.
    Nagakura H
    Phys Rev Lett; 2023 May; 130(21):211401. PubMed ID: 37295106
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Collisional Flavor Instabilities of Supernova Neutrinos.
    Johns L
    Phys Rev Lett; 2023 May; 130(19):191001. PubMed ID: 37243645
    [TBL] [Abstract][Full Text] [Related]  

  • 17. No collective neutrino flavor conversions during the supernova accretion phase.
    Chakraborty S; Fischer T; Mirizzi A; Saviano N; Tomàs R
    Phys Rev Lett; 2011 Oct; 107(15):151101. PubMed ID: 22107280
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Fast Flavor Depolarization of Supernova Neutrinos.
    Bhattacharyya S; Dasgupta B
    Phys Rev Lett; 2021 Feb; 126(6):061302. PubMed ID: 33635718
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Technique for direct eV-scale measurements of the Mu and tau neutrino masses using supernova neutrinos.
    Beacom JF; Boyd RN; Mezzacappa A
    Phys Rev Lett; 2000 Oct; 85(17):3568-71. PubMed ID: 11030952
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Simulation of the spherically symmetric stellar core collapse, bounce, and postbounce evolution of a star of 13 solar masses with boltzmann neutrino transport, and its implications for the supernova mechanism.
    Mezzacappa A; Liebendörfer M; Messer OE; Hix WR; Thielemann FK; Bruenn SW
    Phys Rev Lett; 2001 Mar; 86(10):1935-8. PubMed ID: 11289824
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 10.