Neutrino astronomy with the macro detector

M. Ambrosio; R. Antolini; G. Auriemma; D. Bakari; A. Baldini; G. C. Barbarino; B. C. Barish; G. Battistoni; R. Bellotti; C. Bemporad; P. Bernardini; H. Bilokon; V. Bisi; C. Bloise; C. Bower; M. Brigida; S. Bussino; F. Cafagna; M. Calicchio; D. Campana; M. Carboni; S. Cecchini; F. Cei; V. Chiarella; B. C. Choudhary; S. Coutu; G. de Cataldo; H. Dekhissi; C. de Marzo; I. de Mitri; J. Derkaoui; M. de Vincenzi; A. di Credico; O. Erriquez; C. Favuzzi; C. Forti; P. Fusco; G. Giacomelli; G. Giannini; N. Giglietto; M. Giorgini; M. Grassi; L. Gray; A. Grillo; F. Guarino; C. Gustavino; A. Habig; K. Hanson; R. Heinz; E. Iarocci; E. Katsavounidis; I. Katsavounidis; E. Kearns; H. Kim; S. Kyriazopoulou; E. Lamanna; C. Lane; D. S. Levin; P. Lipari; N. P. Longley; M. J. Longo; F. Loparco; F. Maaroufi; G. Mancarella; G. Mandrioli; S. Manzoor; A. Margiotta; A. Marini; D. Martello; A. Marzari-Chiesa; M. N. Mazziotta; D. G. Michael; S. Mikheyev; L. Miller; P. Monacelli; T. Montaruli; M. Monteno; S. Mufson; J. Musser; D. Nicolo; R. Nolty; C. Okada; C. Orth; G. Osteria; M. Ouchrif; O. Palamara; V. Patera; L. Patrizii; R. Pazzi; C. W. Peck; L. Perrone; S. Petrera; P. Pistilli; V. Popa; A. Raino; J. Reynoldson; F. Ronga; C. Satriano; L. Satta; E. Scapparone; K. Scholberg; A. Sciubba; P. Serra; M. Sioli; M. Sitta; P. Spinelli; M. Spinetti; M. Spurio; R. Steinberg; J. L. Stone; L. R. Sulak; A. Surdo; G. Tarle; V. Togo; M. Vakili; E. Vilela; C. W. Walter; R. Webb

doi:10.1086/318281

Neutrino astronomy with the macro detector

M. Ambrosio, R. Antolini, G. Auriemma, D. Bakari, A. Baldini, G. C. Barbarino, B. C. Barish, G. Battistoni, R. Bellotti, C. Bemporad, P. Bernardini, H. Bilokon, V. Bisi, C. Bloise, C. Bower, M. Brigida, S. Bussino, F. Cafagna, M. Calicchio, D. CampanaM. Carboni, S. Cecchini, F. Cei, V. Chiarella, B. C. Choudhary, S. Coutu, G. de Cataldo, H. Dekhissi, C. de Marzo, I. de Mitri, J. Derkaoui, M. de Vincenzi, A. di Credico, O. Erriquez, C. Favuzzi, C. Forti, P. Fusco, G. Giacomelli, G. Giannini, N. Giglietto, M. Giorgini, M. Grassi, L. Gray, A. Grillo, F. Guarino, C. Gustavino, A. Habig, K. Hanson, R. Heinz, E. Iarocci, E. Katsavounidis, I. Katsavounidis, E. Kearns, H. Kim, S. Kyriazopoulou, E. Lamanna, C. Lane, D. S. Levin, P. Lipari, N. P. Longley, M. J. Longo, F. Loparco, F. Maaroufi, G. Mancarella, G. Mandrioli, S. Manzoor, A. Margiotta, A. Marini, D. Martello, A. Marzari-Chiesa, M. N. Mazziotta, D. G. Michael, S. Mikheyev, L. Miller, P. Monacelli, T. Montaruli, M. Monteno, S. Mufson, J. Musser, D. Nicolo, R. Nolty, C. Okada, C. Orth, G. Osteria, M. Ouchrif, O. Palamara, V. Patera, L. Patrizii, R. Pazzi, C. W. Peck, L. Perrone, S. Petrera, P. Pistilli, V. Popa, A. Raino, J. Reynoldson, F. Ronga, C. Satriano, L. Satta, E. Scapparone, K. Scholberg, A. Sciubba, P. Serra, M. Sioli, M. Sitta, P. Spinelli, M. Spinetti, M. Spurio, R. Steinberg, J. L. Stone, L. R. Sulak, A. Surdo, G. Tarle, V. Togo, M. Vakili, E. Vilela, C. W. Walter, R. Webb

Risultato della ricerca: Contributo su rivista › Articolo in rivista › peer review

Abstract

High-energy gamma-ray astronomy is now a well-established field, and several sources have been discovered in the region from a few giga-electron volts up to several tera-electron volts. If sources involving hadronic processes exist, the production of photons would be accompanied by neutrinos too. Other possible neutrino sources could be related to the annihilation of weakly interacting, massive particles (WIMPs) at the center of galaxies with black holes. We present the results of a search for pointlike sources using 1100 upward-going muons produced by neutrino interactions in the rock below and inside the Monopole Astrophysics and Cosmic Ray Observatory (MACRO) detector in the underground Gran Sasso Laboratory. These data show no evidence of a possible neutrino pointlike source or of possible correlations between gamma-ray bursts and neutrinos. They have been used to set flux upper limits for candidate pointlike sources which are in the range 10^-14 _-10 ^-15 cm^-2 s^-1.

Lingua originale	Inglese
pagine (da-a)	1038-1054
Numero di pagine	17
Rivista	Astrophysical Journal
Volume	546
Numero di pubblicazione	2 PART 1
DOI	https://doi.org/10.1086/318281
Stato di pubblicazione	Pubblicato - 10 gen 2001
Pubblicato esternamente	Sì

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10.1086/318281

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Ambrosio, M., Antolini, R., Auriemma, G., Bakari, D., Baldini, A., Barbarino, G. C., Barish, B. C., Battistoni, G., Bellotti, R., Bemporad, C., Bernardini, P., Bilokon, H., Bisi, V., Bloise, C., Bower, C., Brigida, M., Bussino, S., Cafagna, F., Calicchio, M., ... Webb, R. (2001). Neutrino astronomy with the macro detector. Astrophysical Journal, 546(2 PART 1), 1038-1054. https://doi.org/10.1086/318281

@article{78b965883a4c4578a64c8eafdadf20e7,

title = "Neutrino astronomy with the macro detector",

abstract = "High-energy gamma-ray astronomy is now a well-established field, and several sources have been discovered in the region from a few giga-electron volts up to several tera-electron volts. If sources involving hadronic processes exist, the production of photons would be accompanied by neutrinos too. Other possible neutrino sources could be related to the annihilation of weakly interacting, massive particles (WIMPs) at the center of galaxies with black holes. We present the results of a search for pointlike sources using 1100 upward-going muons produced by neutrino interactions in the rock below and inside the Monopole Astrophysics and Cosmic Ray Observatory (MACRO) detector in the underground Gran Sasso Laboratory. These data show no evidence of a possible neutrino pointlike source or of possible correlations between gamma-ray bursts and neutrinos. They have been used to set flux upper limits for candidate pointlike sources which are in the range 10-14 -10 -15 cm-2 s-1.",

keywords = "Elementary particles, Gamma rays: observations",

author = "M. Ambrosio and R. Antolini and G. Auriemma and D. Bakari and A. Baldini and Barbarino, \{G. C.\} and Barish, \{B. C.\} and G. Battistoni and R. Bellotti and C. Bemporad and P. Bernardini and H. Bilokon and V. Bisi and C. Bloise and C. Bower and M. Brigida and S. Bussino and F. Cafagna and M. Calicchio and D. Campana and M. Carboni and S. Cecchini and F. Cei and V. Chiarella and Choudhary, \{B. C.\} and S. Coutu and \{de Cataldo\}, G. and H. Dekhissi and \{de Marzo\}, C. and \{de Mitri\}, I. and J. Derkaoui and \{de Vincenzi\}, M. and \{di Credico\}, A. and O. Erriquez and C. Favuzzi and C. Forti and P. Fusco and G. Giacomelli and G. Giannini and N. Giglietto and M. Giorgini and M. Grassi and L. Gray and A. Grillo and F. Guarino and C. Gustavino and A. Habig and K. Hanson and R. Heinz and E. Iarocci and E. Katsavounidis and I. Katsavounidis and E. Kearns and H. Kim and S. Kyriazopoulou and E. Lamanna and C. Lane and Levin, \{D. S.\} and P. Lipari and Longley, \{N. P.\} and Longo, \{M. J.\} and F. Loparco and F. Maaroufi and G. Mancarella and G. Mandrioli and S. Manzoor and A. Margiotta and A. Marini and D. Martello and A. Marzari-Chiesa and Mazziotta, \{M. N.\} and Michael, \{D. G.\} and S. Mikheyev and L. Miller and P. Monacelli and T. Montaruli and M. Monteno and S. Mufson and J. Musser and D. Nicolo and R. Nolty and C. Okada and C. Orth and G. Osteria and M. Ouchrif and O. Palamara and V. Patera and L. Patrizii and R. Pazzi and Peck, \{C. W.\} and L. Perrone and S. Petrera and P. Pistilli and V. Popa and A. Raino and J. Reynoldson and F. Ronga and C. Satriano and L. Satta and E. Scapparone and K. Scholberg and A. Sciubba and P. Serra and M. Sioli and M. Sitta and P. Spinelli and M. Spinetti and M. Spurio and R. Steinberg and Stone, \{J. L.\} and Sulak, \{L. R.\} and A. Surdo and G. Tarle and V. Togo and M. Vakili and E. Vilela and Walter, \{C. W.\} and R. Webb",

year = "2001",

month = jan,

day = "10",

doi = "10.1086/318281",

language = "English",

volume = "546",

pages = "1038--1054",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "2 PART 1",

}

Ambrosio, M, Antolini, R, Auriemma, G, Bakari, D, Baldini, A, Barbarino, GC, Barish, BC, Battistoni, G, Bellotti, R, Bemporad, C, Bernardini, P, Bilokon, H, Bisi, V, Bloise, C, Bower, C, Brigida, M, Bussino, S, Cafagna, F, Calicchio, M, Campana, D, Carboni, M, Cecchini, S, Cei, F, Chiarella, V, Choudhary, BC, Coutu, S, de Cataldo, G, Dekhissi, H, de Marzo, C, de Mitri, I, Derkaoui, J, de Vincenzi, M, di Credico, A, Erriquez, O, Favuzzi, C, Forti, C, Fusco, P, Giacomelli, G, Giannini, G, Giglietto, N, Giorgini, M, Grassi, M, Gray, L, Grillo, A, Guarino, F, Gustavino, C, Habig, A, Hanson, K, Heinz, R, Iarocci, E, Katsavounidis, E, Katsavounidis, I, Kearns, E, Kim, H, Kyriazopoulou, S, Lamanna, E, Lane, C, Levin, DS, Lipari, P, Longley, NP, Longo, MJ, Loparco, F, Maaroufi, F, Mancarella, G, Mandrioli, G, Manzoor, S, Margiotta, A, Marini, A, Martello, D, Marzari-Chiesa, A, Mazziotta, MN, Michael, DG, Mikheyev, S, Miller, L, Monacelli, P, Montaruli, T, Monteno, M, Mufson, S, Musser, J, Nicolo, D, Nolty, R, Okada, C, Orth, C, Osteria, G, Ouchrif, M, Palamara, O, Patera, V, Patrizii, L, Pazzi, R, Peck, CW, Perrone, L, Petrera, S, Pistilli, P, Popa, V, Raino, A, Reynoldson, J, Ronga, F, Satriano, C, Satta, L, Scapparone, E, Scholberg, K, Sciubba, A, Serra, P, Sioli, M, Sitta, M, Spinelli, P, Spinetti, M, Spurio, M, Steinberg, R, Stone, JL, Sulak, LR, Surdo, A, Tarle, G, Togo, V, Vakili, M, Vilela, E, Walter, CW & Webb, R 2001, 'Neutrino astronomy with the macro detector', Astrophysical Journal, vol. 546, n. 2 PART 1, pagg. 1038-1054. https://doi.org/10.1086/318281

TY - JOUR

T1 - Neutrino astronomy with the macro detector

AU - Ambrosio, M.

AU - Antolini, R.

AU - Auriemma, G.

AU - Bakari, D.

AU - Baldini, A.

AU - Barbarino, G. C.

AU - Barish, B. C.

AU - Battistoni, G.

AU - Bellotti, R.

AU - Bemporad, C.

AU - Bernardini, P.

AU - Bilokon, H.

AU - Bisi, V.

AU - Bloise, C.

AU - Bower, C.

AU - Brigida, M.

AU - Bussino, S.

AU - Cafagna, F.

AU - Calicchio, M.

AU - Campana, D.

AU - Carboni, M.

AU - Cecchini, S.

AU - Cei, F.

AU - Chiarella, V.

AU - Choudhary, B. C.

AU - Coutu, S.

AU - de Cataldo, G.

AU - Dekhissi, H.

AU - de Marzo, C.

AU - de Mitri, I.

AU - Derkaoui, J.

AU - de Vincenzi, M.

AU - di Credico, A.

AU - Erriquez, O.

AU - Favuzzi, C.

AU - Forti, C.

AU - Fusco, P.

AU - Giacomelli, G.

AU - Giannini, G.

AU - Giglietto, N.

AU - Giorgini, M.

AU - Grassi, M.

AU - Gray, L.

AU - Grillo, A.

AU - Guarino, F.

AU - Gustavino, C.

AU - Habig, A.

AU - Hanson, K.

AU - Heinz, R.

AU - Iarocci, E.

AU - Katsavounidis, E.

AU - Katsavounidis, I.

AU - Kearns, E.

AU - Kim, H.

AU - Kyriazopoulou, S.

AU - Lamanna, E.

AU - Lane, C.

AU - Levin, D. S.

AU - Lipari, P.

AU - Longley, N. P.

AU - Longo, M. J.

AU - Loparco, F.

AU - Maaroufi, F.

AU - Mancarella, G.

AU - Mandrioli, G.

AU - Manzoor, S.

AU - Margiotta, A.

AU - Marini, A.

AU - Martello, D.

AU - Marzari-Chiesa, A.

AU - Mazziotta, M. N.

AU - Michael, D. G.

AU - Mikheyev, S.

AU - Miller, L.

AU - Monacelli, P.

AU - Montaruli, T.

AU - Monteno, M.

AU - Mufson, S.

AU - Musser, J.

AU - Nicolo, D.

AU - Nolty, R.

AU - Okada, C.

AU - Orth, C.

AU - Osteria, G.

AU - Ouchrif, M.

AU - Palamara, O.

AU - Patera, V.

AU - Patrizii, L.

AU - Pazzi, R.

AU - Peck, C. W.

AU - Perrone, L.

AU - Petrera, S.

AU - Pistilli, P.

AU - Popa, V.

AU - Raino, A.

AU - Reynoldson, J.

AU - Ronga, F.

AU - Satriano, C.

AU - Satta, L.

AU - Scapparone, E.

AU - Scholberg, K.

AU - Sciubba, A.

AU - Serra, P.

AU - Sioli, M.

AU - Sitta, M.

AU - Spinelli, P.

AU - Spinetti, M.

AU - Spurio, M.

AU - Steinberg, R.

AU - Stone, J. L.

AU - Sulak, L. R.

AU - Surdo, A.

AU - Tarle, G.

AU - Togo, V.

AU - Vakili, M.

AU - Vilela, E.

AU - Walter, C. W.

AU - Webb, R.

PY - 2001/1/10

Y1 - 2001/1/10

N2 - High-energy gamma-ray astronomy is now a well-established field, and several sources have been discovered in the region from a few giga-electron volts up to several tera-electron volts. If sources involving hadronic processes exist, the production of photons would be accompanied by neutrinos too. Other possible neutrino sources could be related to the annihilation of weakly interacting, massive particles (WIMPs) at the center of galaxies with black holes. We present the results of a search for pointlike sources using 1100 upward-going muons produced by neutrino interactions in the rock below and inside the Monopole Astrophysics and Cosmic Ray Observatory (MACRO) detector in the underground Gran Sasso Laboratory. These data show no evidence of a possible neutrino pointlike source or of possible correlations between gamma-ray bursts and neutrinos. They have been used to set flux upper limits for candidate pointlike sources which are in the range 10-14 -10 -15 cm-2 s-1.

AB - High-energy gamma-ray astronomy is now a well-established field, and several sources have been discovered in the region from a few giga-electron volts up to several tera-electron volts. If sources involving hadronic processes exist, the production of photons would be accompanied by neutrinos too. Other possible neutrino sources could be related to the annihilation of weakly interacting, massive particles (WIMPs) at the center of galaxies with black holes. We present the results of a search for pointlike sources using 1100 upward-going muons produced by neutrino interactions in the rock below and inside the Monopole Astrophysics and Cosmic Ray Observatory (MACRO) detector in the underground Gran Sasso Laboratory. These data show no evidence of a possible neutrino pointlike source or of possible correlations between gamma-ray bursts and neutrinos. They have been used to set flux upper limits for candidate pointlike sources which are in the range 10-14 -10 -15 cm-2 s-1.

KW - Elementary particles

KW - Gamma rays: observations

UR - https://www.scopus.com/pages/publications/0035835110

U2 - 10.1086/318281

DO - 10.1086/318281

M3 - Article

SN - 0004-637X

VL - 546

SP - 1038

EP - 1054

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2 PART 1

ER -

Neutrino astronomy with the macro detector

Abstract

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