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 *

102 related articles for article (PubMed ID: 10016473)

  • 1. Are radiative corrections to the Mikheyev-Smirnov-Wolfenstein formula affected by finite temperature and density?
    Horvat R
    Phys Rev D Part Fields; 1993 Sep; 48(5):2345-2348. PubMed ID: 10016473
    [No Abstract]   [Full Text] [Related]  

  • 2. Experimental tests of the Mikheyev-Smirnov-Wolfenstein effect.
    LoSecco JM
    Phys Rev D Part Fields; 1993 Mar; 47(5):2032-2037. PubMed ID: 10015787
    [No Abstract]   [Full Text] [Related]  

  • 3. Mikheyev-Smirnov-Wolfenstein enhancement of oscillations as a possible solution to the solar-neutrino problem.
    Rosen SP; Gelb JM
    Phys Rev D Part Fields; 1986 Aug; 34(4):969-979. PubMed ID: 9957237
    [No Abstract]   [Full Text] [Related]  

  • 4. Mikheyev-Smirnov-Wolfenstein effect with flavor-changing neutrino interactions.
    Roulet E
    Phys Rev D Part Fields; 1991 Aug; 44(4):R935-R938. PubMed ID: 10014002
    [No Abstract]   [Full Text] [Related]  

  • 5. Mikheyev-Smirnov-Wolfenstein effect in electron-neutrino scattering experiments.
    Bahcall JN; Gelb JM; Rosen SP
    Phys Rev D Part Fields; 1987 May; 35(10):2976-2982. PubMed ID: 9957540
    [No Abstract]   [Full Text] [Related]  

  • 6. Exact analytic solutions for Mikheyev-Smirnov-Wolfenstein level crossings.
    Nötzold D
    Phys Rev D Part Fields; 1987 Sep; 36(6):1625-1633. PubMed ID: 9958343
    [No Abstract]   [Full Text] [Related]  

  • 7. Neutrino decay catalyzed by the Mikheyev-Smirnov-Wolfenstein effect.
    Raghavan RS; He XG; Pakvasa S
    Phys Rev D Part Fields; 1988 Aug; 38(4):1317-1320. PubMed ID: 9959271
    [No Abstract]   [Full Text] [Related]  

  • 8. Monte Carlo exploration of Mikheyev-Smirnov-Wolfenstein solutions to the solar neutrino problem.
    Shi X; Schramm DN; Bahcall JN
    Phys Rev Lett; 1992 Aug; 69(5):717-720. PubMed ID: 10047015
    [No Abstract]   [Full Text] [Related]  

  • 9. Solar neutrinos and the Mikheyev-Smirnov-Wolfenstein theory.
    Bethe HA; Bahcall JN
    Phys Rev D Part Fields; 1991 Nov; 44(10):2962-2969. PubMed ID: 10013753
    [No Abstract]   [Full Text] [Related]  

  • 10. Implications of new GALLEX results for the Mikheyev-Smirnov-Wolfenstein solution of the solar neutrino problem.
    Gelb JM; Kwong W; Rosen SP
    Phys Rev Lett; 1992 Sep; 69(13):1864-1866. PubMed ID: 10046335
    [No Abstract]   [Full Text] [Related]  

  • 11. Neutrino-electron scattering and the choice between different Mikheyev-Smirnov-Wolfenstein solutions of the solar neutrino problem.
    Rosen SP; Gelb JM
    Phys Rev D Part Fields; 1989 May; 39(10):3190-3193. PubMed ID: 9959563
    [No Abstract]   [Full Text] [Related]  

  • 12. Mikheyev-smirnov-wolfenstein effects in vacuum oscillations.
    Friedland A
    Phys Rev Lett; 2000 Jul; 85(5):936-9. PubMed ID: 10991443
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Mass relation for neutrinos.
    Babu KS; Barr SM
    Phys Rev Lett; 2000 Aug; 85(6):1170-3. PubMed ID: 10991504
    [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. Effect of Impurities on the Josephson Current through Helical Metals: Exploiting a Neutrino Paradigm.
    Ghaemi P; Nair VP
    Phys Rev Lett; 2016 Jan; 116(3):037001. PubMed ID: 26849609
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Coherent active-sterile neutrino flavor transformation in the early universe.
    Kishimoto CT; Fuller GM; Smith CJ
    Phys Rev Lett; 2006 Oct; 97(14):141301. PubMed ID: 17155237
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Large extra dimensions, sterile neutrinos and solar neutrino data.
    Caldwell DO; Mohapatra RN; Yellin SJ
    Phys Rev Lett; 2001 Jul; 87(4):041601. PubMed ID: 11461607
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Polarized x-ray emission from magnetized neutron stars: signature of strong-field vacuum polarization.
    Lai D; Ho WC
    Phys Rev Lett; 2003 Aug; 91(7):071101. PubMed ID: 12935001
    [TBL] [Abstract][Full Text] [Related]  

  • 19. 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]  

  • 20. 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]  

    [Next]    [New Search]
    of 6.