OperaV1, PascalFrancis, Corpus, bibRecord, 000601

Neutrino oscillation parameters from MINOS, ICARUS, and OPERA combined

Identifieur interne : 000601 ( PascalFrancis/Corpus ); précédent : 000600; suivant : 000602

Neutrino oscillation parameters from MINOS, ICARUS, and OPERA combined

Auteurs : V. Barger ; A. M. Gago ; D. Marfatia ; W. J. C. Teves ; B. P. Wood ; R. Zukanovich Funchal

Source :

Physical review. D. Particles and fields [ 0556-2821 ] ; 2002-03-01.

RBID : Pascal:02-0145356

Descripteurs français

Pascal (Inist)
- 1460P, 1460L, Etude théorique, Etude expérimentale, Oscillation neutrino, Neutrino cosmique.

English descriptors

KwdEn :
- Cosmic neutrinos, Experimental study, Neutrino oscillations, Theoretical study.

Abstract

We perform a detailed analysis of the capabilities of the MINOS, ICARUS and OPERA experiments to measure neutrino oscillation parameters at the atmospheric scale with their data taken separately and in combination. MINOS will determine Δm₃₂² and sin²2θ₂₃ to within 10% at the 99% C.L. with 10 kton-years of data. While no one experiment will determine sin²2θ₁₃ with much precision, if its value lies in the combined sensitivity region of the three experiments, it will be possible to place a lower bound of O(0.01) at the 95% C.L. on this parameter by combining the data from the three experiments. The same bound can be placed with a combination of MINOS and ICARUS data alone.

Notice en format standard (ISO 2709)

Pour connaître la documentation sur le format Inist Standard.

A01	`01`	`1`		`@0 0556-2821`
A02	`01`			`@0 PRVDAQ`
A03		`1`		`@0 Phys. rev. D, Part. fields`
A05				`@2 65`
A06				`@2 5`
A08	`01`	`1`	`ENG`	`@1 Neutrino oscillation parameters from MINOS, ICARUS, and OPERA combined`
A11	`01`	`1`		`@1 BARGER (V.)`
A11	`02`	`1`		`@1 GAGO (A. M.)`
A11	`03`	`1`		`@1 MARFATIA (D.)`
A11	`04`	`1`		`@1 TEVES (W. J. C.)`
A11	`05`	`1`		`@1 WOOD (B. P.)`
A11	`06`	`1`		`@1 ZUKANOVICH FUNCHAL (R.)`
A14	`01`			`@1 Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706 @Z 1 aut. @Z 3 aut. @Z 5 aut.`
A14	`02`			`@1 Department of Physics, California State University, Dominguez Hills, Carson, California 90747 @Z 2 aut.`
A14	`03`			`@1 Instituto de Fisica, Universidade de Sao Paulo, C. P. 66.318, 05315-970 Sao Paulo, Brazil @Z 2 aut. @Z 4 aut. @Z 6 aut.`
A14	`04`			`@1 Seccion Fisica, Departamento de Ciencias, Pontificia Universidad Catolica del Peru, Apartado 1761, Lima, Peru @Z 2 aut.`
A14	`05`			`@1 Department of Physics, Boston University, Boston, Massachusetts 02215 @Z 3 aut.`
A20				`@2 053016-053016-11`
A21				`@1 2002-03-01`
A23	`01`			`@0 ENG`
A43	`01`			`@1 INIST @2 144 D`
A44				`@0 8100 @1 © 2002 American Institute of Physics. All rights reserved.`
A47	`01`	`1`		`@0 02-0145356`
A60				`@1 P`
A61				`@0 A`
A64	`01`	`1`		`@0 Physical review. D. Particles and fields`
A66	`01`			`@0 USA`
C01	`01`		`ENG`	@0 We perform a detailed analysis of the capabilities of the MINOS, ICARUS and OPERA experiments to measure neutrino oscillation parameters at the atmospheric scale with their data taken separately and in combination. MINOS will determine Δm₃₂² and sin²2θ₂₃ to within 10% at the 99% C.L. with 10 kton-years of data. While no one experiment will determine sin²2θ₁₃ with much precision, if its value lies in the combined sensitivity region of the three experiments, it will be possible to place a lower bound of O(0.01) at the 95% C.L. on this parameter by combining the data from the three experiments. The same bound can be placed with a combination of MINOS and ICARUS data alone.
C02	`01`	`3`		`@0 001B10D60P`
C02	`02`	`3`		`@0 001B10D60L`
C03	`01`	`3`	`FRE`	`@0 1460P @2 PAC @4 INC`
C03	`02`	`3`	`FRE`	`@0 1460L @2 PAC @4 INC`
C03	`03`	`3`	`FRE`	`@0 Etude théorique`
C03	`03`	`3`	`ENG`	`@0 Theoretical study`
C03	`04`	`3`	`FRE`	`@0 Etude expérimentale`
C03	`04`	`3`	`ENG`	`@0 Experimental study`
C03	`05`	`3`	`FRE`	`@0 Oscillation neutrino`
C03	`05`	`3`	`ENG`	`@0 Neutrino oscillations`
C03	`06`	`3`	`FRE`	`@0 Neutrino cosmique`
C03	`06`	`3`	`ENG`	`@0 Cosmic neutrinos`
N21				`@1 077`
N47	`01`	`1`		`@0 0210M000694`

Format Inist (serveur)

NO :	PASCAL 02-0145356 AIP
ET :	Neutrino oscillation parameters from MINOS, ICARUS, and OPERA combined
AU :	BARGER (V.); GAGO (A. M.); MARFATIA (D.); TEVES (W. J. C.); WOOD (B. P.); ZUKANOVICH FUNCHAL (R.)
AF :	Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706 (1 aut., 3 aut., 5 aut.); Department of Physics, California State University, Dominguez Hills, Carson, California 90747 (2 aut.); Instituto de Fisica, Universidade de Sao Paulo, C. P. 66.318, 05315-970 Sao Paulo, Brazil (2 aut., 4 aut., 6 aut.); Seccion Fisica, Departamento de Ciencias, Pontificia Universidad Catolica del Peru, Apartado 1761, Lima, Peru (2 aut.); Department of Physics, Boston University, Boston, Massachusetts 02215 (3 aut.)
DT :	Publication en série; Niveau analytique
SO :	Physical review. D. Particles and fields; ISSN 0556-2821; Coden PRVDAQ; Etats-Unis; Da. 2002-03-01; Vol. 65; No. 5; 053016-053016-11
LA :	Anglais
EA :	We perform a detailed analysis of the capabilities of the MINOS, ICARUS and OPERA experiments to measure neutrino oscillation parameters at the atmospheric scale with their data taken separately and in combination. MINOS will determine Δm₃₂² and sin²2θ₂₃ to within 10% at the 99% C.L. with 10 kton-years of data. While no one experiment will determine sin²2θ₁₃ with much precision, if its value lies in the combined sensitivity region of the three experiments, it will be possible to place a lower bound of O(0.01) at the 95% C.L. on this parameter by combining the data from the three experiments. The same bound can be placed with a combination of MINOS and ICARUS data alone.
CC :	001B10D60P; 001B10D60L
FD :	1460P; 1460L; Etude théorique; Etude expérimentale; Oscillation neutrino; Neutrino cosmique
ED :	Theoretical study; Experimental study; Neutrino oscillations; Cosmic neutrinos
LO :	INIST-144 D
ID :	02-0145356

Links to Exploration step

Pascal:02-0145356

Le document en format XML

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<front><div type="abstract" xml:lang="en">We perform a detailed analysis of the capabilities of the MINOS, ICARUS and OPERA experiments to measure neutrino oscillation parameters at the atmospheric scale with their data taken separately and in combination. MINOS will determine Δm<sub>32</sub>
<sup>2</sup>
 and sin<sup>2</sup>
2θ<sub>23</sub>
 to within 10% at the 99% C.L. with 10 kton-years of data. While no one experiment will determine sin<sup>2</sup>
2θ<sub>13</sub>
 with much precision, if its value lies in the combined sensitivity region of the three experiments, it will be possible to place a lower bound of O(0.01) at the 95% C.L. on this parameter by combining the data from the three experiments. The same bound can be placed with a combination of MINOS and ICARUS data alone.</div>
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<sup>2</sup>
 and sin<sup>2</sup>
2θ<sub>23</sub>
 to within 10% at the 99% C.L. with 10 kton-years of data. While no one experiment will determine sin<sup>2</sup>
2θ<sub>13</sub>
 with much precision, if its value lies in the combined sensitivity region of the three experiments, it will be possible to place a lower bound of O(0.01) at the 95% C.L. on this parameter by combining the data from the three experiments. The same bound can be placed with a combination of MINOS and ICARUS data alone.</s0>
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<EA>We perform a detailed analysis of the capabilities of the MINOS, ICARUS and OPERA experiments to measure neutrino oscillation parameters at the atmospheric scale with their data taken separately and in combination. MINOS will determine Δm<sub>32</sub>
<sup>2</sup>
 and sin<sup>2</sup>
2θ<sub>23</sub>
 to within 10% at the 99% C.L. with 10 kton-years of data. While no one experiment will determine sin<sup>2</sup>
2θ<sub>13</sub>
 with much precision, if its value lies in the combined sensitivity region of the three experiments, it will be possible to place a lower bound of O(0.01) at the 95% C.L. on this parameter by combining the data from the three experiments. The same bound can be placed with a combination of MINOS and ICARUS data alone.</EA>
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   |texte=   Neutrino oscillation parameters from MINOS, ICARUS, and OPERA combined
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Neutrino oscillation parameters from MINOS, ICARUS, and OPERA combined

Neutrino oscillation parameters from MINOS, ICARUS, and OPERA combined

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