Literature DB >> 25164744

Neutrino physics: What makes the Sun shine.

Wick Haxton1.   

Abstract

Year:  2014        PMID: 25164744     DOI: 10.1038/512378a

Source DB:  PubMed          Journal:  Nature        ISSN: 0028-0836            Impact factor:   49.962


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  5 in total

1.  Solar Neutrino Data Covering Solar Cycle 22.

Authors: 
Journal:  Phys Rev Lett       Date:  1996-08-26       Impact factor: 9.161

2.  Measurement of day and night neutrino energy spectra at SNO and constraints on neutrino mixing parameters.

Authors:  Q R Ahmad; R C Allen; T C Andersen; J D Anglin; J C Barton; E W Beier; M Bercovitch; J Bigu; S D Biller; R A Black; I Blevis; R J Boardman; J Boger; E Bonvin; M G Boulay; M G Bowler; T J Bowles; S J Brice; M C Browne; T V Bullard; G Bühler; J Cameron; Y D Chan; H H Chen; M Chen; X Chen; B T Cleveland; E T H Clifford; J H M Cowan; D F Cowen; G A Cox; X Dai; F Dalnoki-Veress; W F Davidson; P J Doe; G Doucas; M R Dragowsky; C A Duba; F A Duncan; M Dunford; J A Dunmore; E D Earle; S R Elliott; H C Evans; G T Ewan; J Farine; H Fergani; A P Ferraris; R J Ford; J A Formaggio; M M Fowler; K Frame; E D Frank; W Frati; N Gagnon; J V Germani; S Gil; K Graham; D R Grant; R L Hahn; A L Hallin; E D Hallman; A S Hamer; A A Hamian; W B Handler; R U Haq; C K Hargrove; P J Harvey; R Hazama; K M Heeger; W J Heintzelman; J Heise; R L Helmer; J D Hepburn; H Heron; J Hewett; A Hime; M Howe; J G Hykawy; M C P Isaac; P Jagam; N A Jelley; C Jillings; G Jonkmans; K Kazkaz; P T Keener; J R Klein; A B Knox; R J Komar; R Kouzes; T Kutter; C C M Kyba; J Law; I T Lawson; M Lay; H W Lee; K T Lesko; J R Leslie; I Levine; W Locke; S Luoma; J Lyon; S Majerus; H B Mak; J Maneira; J Manor; A D Marino; N McCauley; A B McDonald; D S McDonald; K McFarlane; G McGregor; R Meijer Drees; C Mifflin; G G Miller; G Milton; B A Moffat; M Moorhead; C W Nally; M S Neubauer; F M Newcomer; H S Ng; A J Noble; E B Norman; V M Novikov; M O'Neill; C E Okada; R W Ollerhead; M Omori; J L Orrell; S M Oser; A W P Poon; T J Radcliffe; A Roberge; B C Robertson; R G H Robertson; S S E Rosendahl; J K Rowley; V L Rusu; E Saettler; K K Schaffer; M H Schwendener; A Schülke; H Seifert; M Shatkay; J J Simpson; C J Sims; D Sinclair; P Skensved; A R Smith; M W E Smith; T Spreitzer; N Starinsky; T D Steiger; R G Stokstad; L C Stonehill; R S Storey; B Sur; R Tafirout; N Tagg; N W Tanner; R K Taplin; M Thorman; P M Thornewell; P T Trent; Y I Tserkovnyak; R Van Berg; R G Van de Water; C J Virtue; C E Waltham; J-X Wang; D L Wark; N West; J B Wilhelmy; J F Wilkerson; J R Wilson; P Wittich; J M Wouters; M Yeh
Journal:  Phys Rev Lett       Date:  2002-06-13       Impact factor: 9.161

3.  Precision measurement of the (7)Be solar neutrino interaction rate in Borexino.

Authors:  G Bellini; J Benziger; D Bick; S Bonetti; G Bonfini; M Buizza Avanzini; B Caccianiga; L Cadonati; F Calaprice; C Carraro; P Cavalcante; A Chavarria; D D'Angelo; S Davini; A Derbin; A Etenko; K Fomenko; D Franco; C Galbiati; S Gazzana; C Ghiano; M Giammarchi; M Goeger-Neff; A Goretti; L Grandi; E Guardincerri; S Hardy; Aldo Ianni; Andrea Ianni; V Kobychev; D Korablev; G Korga; Y Koshio; D Kryn; M Laubenstein; T Lewke; E Litvinovich; B Loer; F Lombardi; P Lombardi; L Ludhova; I Machulin; S Manecki; W Maneschg; G Manuzio; Q Meindl; E Meroni; L Miramonti; M Misiaszek; D Montanari; P Mosteiro; V Muratova; L Oberauer; M Obolensky; F Ortica; M Pallavicini; L Papp; C Peña-Garay; L Perasso; S Perasso; A Pocar; R S Raghavan; G Ranucci; A Razeto; A Re; A Romani; A Sabelnikov; R Saldanha; C Salvo; S Schönert; H Simgen; M Skorokhvatov; O Smirnov; A Sotnikov; S Sukhotin; Y Suvorov; R Tartaglia; G Testera; D Vignaud; R B Vogelaar; F von Feilitzsch; J Winter; M Wojcik; A Wright; M Wurm; J Xu; O Zaimidoroga; S Zavatarelli; G Zuzel
Journal:  Phys Rev Lett       Date:  2011-09-30       Impact factor: 9.161

4.  First evidence of pep solar neutrinos by direct detection in Borexino.

Authors:  G Bellini; J Benziger; D Bick; S Bonetti; G Bonfini; D Bravo; M Buizza Avanzini; B Caccianiga; L Cadonati; F Calaprice; C Carraro; P Cavalcante; A Chavarria; A Chepurnov; D D'Angelo; S Davini; A Derbin; A Etenko; K Fomenko; D Franco; C Galbiati; S Gazzana; C Ghiano; M Giammarchi; M Goeger-Neff; A Goretti; L Grandi; E Guardincerri; S Hardy; Aldo Ianni; Andrea Ianni; D Korablev; G Korga; Y Koshio; D Kryn; M Laubenstein; T Lewke; E Litvinovich; B Loer; F Lombardi; P Lombardi; L Ludhova; I Machulin; S Manecki; W Maneschg; G Manuzio; Q Meindl; E Meroni; L Miramonti; M Misiaszek; D Montanari; P Mosteiro; V Muratova; L Oberauer; M Obolensky; F Ortica; K Otis; M Pallavicini; L Papp; L Perasso; S Perasso; A Pocar; J Quirk; R S Raghavan; G Ranucci; A Razeto; A Re; A Romani; A Sabelnikov; R Saldanha; C Salvo; S Schönert; H Simgen; M Skorokhvatov; O Smirnov; A Sotnikov; S Sukhotin; Y Suvorov; R Tartaglia; G Testera; D Vignaud; R B Vogelaar; F von Feilitzsch; J Winter; M Wojcik; A Wright; M Wurm; J Xu; O Zaimidoroga; S Zavatarelli; G Zuzel
Journal:  Phys Rev Lett       Date:  2012-02-02       Impact factor: 9.161

5.  Neutrinos from the primary proton-proton fusion process in the Sun.

Authors: 
Journal:  Nature       Date:  2014-08-28       Impact factor: 49.962

  5 in total

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