Probing Neutrino Vacuum Oscillations with the GALLEX Solar Neutrino Results
We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter se...
Ausführliche Beschreibung
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1999 |
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Online-Ressource 4 |
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APS Digital Backfile Archive 1893-2003 |
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Enthalten in: Physical review letters - College Park, Md. : APS, 1958, 83(1999), 6, Seite 1088-1091 |
Übergeordnetes Werk: |
volume:83 ; year:1999 ; number:6 ; pages:1088-1091 ; extent:4 |
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520 | |a We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter sets of Δm2=5.0×10-10 eV2, sin22θ=0.85 and Δm2=9.8×10-10 eV2, sin22θ=1.0 provide the best fits to the results from both GALLEX data analysis methods. A time-constant suppression is also well compatible with the data. The potential of GNO and BOREXINO in this context is outlined. | ||
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(DE-627)NLEJ250681706 (DE-601)aps:d33ca3bd07309ae0ba09931fc3cb7d7256075935 DE-627 ger DE-627 rakwb Probing Neutrino Vacuum Oscillations with the GALLEX Solar Neutrino Results 1999 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter sets of Δm2=5.0×10-10 eV2, sin22θ=0.85 and Δm2=9.8×10-10 eV2, sin22θ=1.0 provide the best fits to the results from both GALLEX data analysis methods. A time-constant suppression is also well compatible with the data. The potential of GNO and BOREXINO in this context is outlined. APS Digital Backfile Archive 1893-2003 Wänninger, S. oth Altmann, M. oth Feilitzsch, F. v. oth Hagner, C. oth Kemmather, B. oth Oberauer, L. oth Schnagl, J. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 83(1999), 6, Seite 1088-1091 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:83 year:1999 number:6 pages:1088-1091 extent:4 https://www.tib.eu/de/suchen/id/aps%3Ad33ca3bd07309ae0ba09931fc3cb7d7256075935 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 83 1999 6 1088-1091 4 |
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(DE-627)NLEJ250681706 (DE-601)aps:d33ca3bd07309ae0ba09931fc3cb7d7256075935 DE-627 ger DE-627 rakwb Probing Neutrino Vacuum Oscillations with the GALLEX Solar Neutrino Results 1999 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter sets of Δm2=5.0×10-10 eV2, sin22θ=0.85 and Δm2=9.8×10-10 eV2, sin22θ=1.0 provide the best fits to the results from both GALLEX data analysis methods. A time-constant suppression is also well compatible with the data. The potential of GNO and BOREXINO in this context is outlined. APS Digital Backfile Archive 1893-2003 Wänninger, S. oth Altmann, M. oth Feilitzsch, F. v. oth Hagner, C. oth Kemmather, B. oth Oberauer, L. oth Schnagl, J. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 83(1999), 6, Seite 1088-1091 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:83 year:1999 number:6 pages:1088-1091 extent:4 https://www.tib.eu/de/suchen/id/aps%3Ad33ca3bd07309ae0ba09931fc3cb7d7256075935 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 83 1999 6 1088-1091 4 |
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(DE-627)NLEJ250681706 (DE-601)aps:d33ca3bd07309ae0ba09931fc3cb7d7256075935 DE-627 ger DE-627 rakwb Probing Neutrino Vacuum Oscillations with the GALLEX Solar Neutrino Results 1999 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter sets of Δm2=5.0×10-10 eV2, sin22θ=0.85 and Δm2=9.8×10-10 eV2, sin22θ=1.0 provide the best fits to the results from both GALLEX data analysis methods. A time-constant suppression is also well compatible with the data. The potential of GNO and BOREXINO in this context is outlined. APS Digital Backfile Archive 1893-2003 Wänninger, S. oth Altmann, M. oth Feilitzsch, F. v. oth Hagner, C. oth Kemmather, B. oth Oberauer, L. oth Schnagl, J. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 83(1999), 6, Seite 1088-1091 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:83 year:1999 number:6 pages:1088-1091 extent:4 https://www.tib.eu/de/suchen/id/aps%3Ad33ca3bd07309ae0ba09931fc3cb7d7256075935 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 83 1999 6 1088-1091 4 |
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(DE-627)NLEJ250681706 (DE-601)aps:d33ca3bd07309ae0ba09931fc3cb7d7256075935 DE-627 ger DE-627 rakwb Probing Neutrino Vacuum Oscillations with the GALLEX Solar Neutrino Results 1999 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter sets of Δm2=5.0×10-10 eV2, sin22θ=0.85 and Δm2=9.8×10-10 eV2, sin22θ=1.0 provide the best fits to the results from both GALLEX data analysis methods. A time-constant suppression is also well compatible with the data. The potential of GNO and BOREXINO in this context is outlined. APS Digital Backfile Archive 1893-2003 Wänninger, S. oth Altmann, M. oth Feilitzsch, F. v. oth Hagner, C. oth Kemmather, B. oth Oberauer, L. oth Schnagl, J. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 83(1999), 6, Seite 1088-1091 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:83 year:1999 number:6 pages:1088-1091 extent:4 https://www.tib.eu/de/suchen/id/aps%3Ad33ca3bd07309ae0ba09931fc3cb7d7256075935 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 83 1999 6 1088-1091 4 |
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(DE-627)NLEJ250681706 (DE-601)aps:d33ca3bd07309ae0ba09931fc3cb7d7256075935 DE-627 ger DE-627 rakwb Probing Neutrino Vacuum Oscillations with the GALLEX Solar Neutrino Results 1999 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter sets of Δm2=5.0×10-10 eV2, sin22θ=0.85 and Δm2=9.8×10-10 eV2, sin22θ=1.0 provide the best fits to the results from both GALLEX data analysis methods. A time-constant suppression is also well compatible with the data. The potential of GNO and BOREXINO in this context is outlined. APS Digital Backfile Archive 1893-2003 Wänninger, S. oth Altmann, M. oth Feilitzsch, F. v. oth Hagner, C. oth Kemmather, B. oth Oberauer, L. oth Schnagl, J. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 83(1999), 6, Seite 1088-1091 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:83 year:1999 number:6 pages:1088-1091 extent:4 https://www.tib.eu/de/suchen/id/aps%3Ad33ca3bd07309ae0ba09931fc3cb7d7256075935 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 83 1999 6 1088-1091 4 |
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probing neutrino vacuum oscillations with the gallex solar neutrino results |
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Probing Neutrino Vacuum Oscillations with the GALLEX Solar Neutrino Results |
abstract |
We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter sets of Δm2=5.0×10-10 eV2, sin22θ=0.85 and Δm2=9.8×10-10 eV2, sin22θ=1.0 provide the best fits to the results from both GALLEX data analysis methods. A time-constant suppression is also well compatible with the data. The potential of GNO and BOREXINO in this context is outlined. |
abstractGer |
We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter sets of Δm2=5.0×10-10 eV2, sin22θ=0.85 and Δm2=9.8×10-10 eV2, sin22θ=1.0 provide the best fits to the results from both GALLEX data analysis methods. A time-constant suppression is also well compatible with the data. The potential of GNO and BOREXINO in this context is outlined. |
abstract_unstemmed |
We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter sets of Δm2=5.0×10-10 eV2, sin22θ=0.85 and Δm2=9.8×10-10 eV2, sin22θ=1.0 provide the best fits to the results from both GALLEX data analysis methods. A time-constant suppression is also well compatible with the data. The potential of GNO and BOREXINO in this context is outlined. |
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Probing Neutrino Vacuum Oscillations with the GALLEX Solar Neutrino Results |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000naa a22002652 4500</leader><controlfield tag="001">NLEJ250681706</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20231114105413.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">231114s1999 xx |||||o 00| ||und c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ250681706</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-601)aps:d33ca3bd07309ae0ba09931fc3cb7d7256075935</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Probing Neutrino Vacuum Oscillations with the GALLEX Solar Neutrino Results</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1999</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">4</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We present a fit of a two-flavor neutrino vacuum oscillation scenario to the GALLEX individual run results. The predicted flux variation during exposure is taken into account for every run. Investigating the published 65 GALLEX solar runs performed during a six-year period we found that parameter sets of Δm2=5.0×10-10 eV2, sin22θ=0.85 and Δm2=9.8×10-10 eV2, sin22θ=1.0 provide the best fits to the results from both GALLEX data analysis methods. A time-constant suppression is also well compatible with the data. The potential of GNO and BOREXINO in this context is outlined.</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">APS Digital Backfile Archive 1893-2003</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wänninger, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Altmann, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Feilitzsch, F. v.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hagner, C.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kemmather, B.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Oberauer, L.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Schnagl, J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Physical review letters</subfield><subfield code="d">College Park, Md. : APS, 1958</subfield><subfield code="g">83(1999), 6, Seite 1088-1091</subfield><subfield code="h">Online-Ressource</subfield><subfield code="w">(DE-627)NLEJ248237888</subfield><subfield code="w">(DE-600)1472655-5</subfield><subfield code="x">1079-7114</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:83</subfield><subfield code="g">year:1999</subfield><subfield code="g">number:6</subfield><subfield code="g">pages:1088-1091</subfield><subfield code="g">extent:4</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://www.tib.eu/de/suchen/id/aps%3Ad33ca3bd07309ae0ba09931fc3cb7d7256075935</subfield><subfield code="x">Verlag</subfield><subfield code="z">Deutschlandweit zugänglich</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-APS</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_NL_ARTICLE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">83</subfield><subfield code="j">1999</subfield><subfield code="e">6</subfield><subfield code="h">1088-1091</subfield><subfield code="g">4</subfield></datafield></record></collection>
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