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1. First observations of separated atmospheric nu(mu) and (nu)over-bar(mu) events in the MINOS detector

Author

Adamson, P, Alexopoulos, T, Allison, WWM, Alner, GJ, Anderson, K, Andreopoulos, C, Andrews, M, Andrews, R, Arroyo, C, Avvakumov, S, Ayres, DS, Baller, B, Barish, B, Barker, MA, Barnes, PD, Barr, G, Barrett, WL, Beall, E, Becker, BR, Belias, A, Bergfeld, T, Bernstein, RH, Bhattacharya, D, Bishai, M, Blake, A, Bocean, V, Bock, B, Bock, GJ, Boehm, J, Boehnlein, DJ, Bogert, D, Border, PM, Bower, C, Boyd, S, Buckley-Geer, E, Byon-Wagner, A, Cabrera, A, Chapman, JD, Chase, TR, Chernichenko, SK, Childress, S, Choudhary, BC, Cobb, JH, Cossairt, JD, Courant, H, Crane, DA, Culling, AJ, Dawson, JW, DeMuth, DM, De Santo, A, Dierckxsens, M, Diwan, MV, Dorman, M, Drake, G, Ducar, R, Durkin, T, Erwin, AR, Escobar, CO, Evans, J, Fackler, OD, Harris, EF, Feldman, GJ, Felt, N, Fields, TH, Ford, R, Frohne, MV, Gallagher, HR, Gebhard, M, Godley, A, Gogos, J, Goodman, MC, Gornushkin, Y, Gouffon, P, Grashorn, E, Grossman, N, Grudzinski, JJ, Grzelak, K, Guarino, V, Habig, A, Halsall, R, Hanson, J, Harris, D, Harris, PG, Hartnell, J, Hartouni, EP, Hatcher, R, Heller, K, Hill, N, Ho, Y, Howcroft, C, Hylen, J, Ignatenko, M, Indurthy, D, Irwin, GM, James, C, Jenner, L, Jensen, D, Joffe-Minor, T, Kafka, T, Kang, HJ, Kasahara, SMS, Kilmer, J, Kim, H, Koizumi, G, Kopp, S, Kordosky, M, Koskinen, DJ, Kostin, M, Krakauer, DA, Kumaratunga, S, Ladran, AS, Lang, K, Laughton, C, Lebedev, A, Lee, R, Lee, WY, Libkind, MA, Liu, J, Litchfield, PJ, Litchfield, RP, Longley, NP, Lucas, P, Luebke, W, Madani, S, Maher, E, Makeev, V, Mann, WA, Marchionni, A, Marino, AD, Marshak, ML, Marshall, JS, McDonald, J, McGowan, A, Meier, JR, Merzon, GI, Messier, MD, Michael, DG, Milburn, RH, Miller, JL, Miller, WH, Mishra, SR, Miyagawa, PS, Moore, C, Morfin, J, Morse, R, Mualem, L, Mufson, S, Murgia, S, Murtagh, MJ, Musser, J, Naples, D, Nelson, C, Nelson, JK, Newman, HB, Nezrick, F, Nichol, RJ, Nicholls, TC, Ochoa-Ricoux, JP, Oliver, J, Oliver, WP, Onuchin, VA, Osiecki, T, Ospanov, R, Paley, J, Paolone, V, Para, A, Patzak, T, Pavlovich, Z, Pearce, GF, Pearson, N, Peck, CW, Perry, C, Peterson, EA, Petyt, DA, Ping, H, Piteira, R, Pla-Dalmau, A, Plunkett, RK, Price, LE, Proga, M, Pushka, DR, Rahman, D, Rameika, RA, Raufer, TM, Read, AL, Rebel, B, Reyna, DE, Rosenfeld, C, Rubin, HA, Ruddick, K, Ryabov, VA, Saakyan, R, Sanchez, MC, Saoulidou, N, Schneps, J, Schoessow, PV, Schreiner, P, Schwienhorst, R, Semenov, VK, Seun, SM, Shanahan, P, Shield, PD, Smart, W, Smirnitsky, V, Smith, C, Smith, PN, Sousa, A, Speakman, B, Stamoulis, P, Stefanik, A, Sullivan, P, Swan, JM, Symes, PA, Tagg, N, Talaga, RL, Tetteh-Lartey, E, Thomas, J, Thompson, J, Thomson, MA, Thron, JL, Trendler, R, Trevor, J, Trostin, I, Tsarev, VA, Tzanakos, G, Urheim, J, Vahle, P, Vakili, M, Vaziri, K, Velissaris, C, Verebryusov, V, Viren, B, Wai, L, Ward, CP, Ward, DR, Watabe, M, Weber, A, Webb, RC, Wehmann, A, West, N, White, C, White, RF, Wojcicki, SG, Wright, DM, Wu, QK, Yan, WG, Yang, T, Yumiceva, FX, Yun, JC, Zheng, H, Zois, M, Zwaska, R, and Collaboration, MMINOS

Published
2006

2. First observations of separated atmospheric νμ and ν̄μ events in the MINOS detector

Author

Adamson, P, Alexopoulos, T, Allison, WWM, Alner, GJ, Anderson, K, Andreopoulos, C, Andrews, M, Andrews, R, Arroyo, C, Avvakumov, S, Ayres, DS, Baller, B, Barish, B, Barker, MA, Barnes Jr, PD, Barr, G, Barrett, WL, Beall, E, Becker, BR, Belias, A, Bergfeld, T, Bernstein, RH, Bhattacharya, D, Bishai, M, Blake, A, Bocean, V, Bock, B, Bock, GJ, Boehm, J, Boehnlein, DJ, Bogert, D, Border, PM, Bower, C, Boyd, S, Buckley-Geer, E, Byon-Wagner, A, Cabrera, A, Chapman, JD, Chase, TR, Chernichenko, SK, Childress, S, Choudhary, BC, Cobb, JH, Cossairt, JD, Courant, H, Crane, DA, Culling, AJ, Dawson, JW, DeMuth, DM, De Santo, A, Dierckxsens, M, Diwan, MV, Dorman, M, Drake, G, Ducar, R, Durkin, T, Erwin, AR, Escobar, CO, Evans, J, Fackler, OD, Harris, EF, Feldman, GJ, Felt, N, Fields, TH, Ford, R, Frohne, MV, Gallagher, HR, Gebhard, M, Godley, A, Gogos, J, Goodman, MC, Gornushkin, Y, Gouffon, P, Grashorn, E, Grossman, N, Grudzinski, JJ, Grzelak, K, Guarino, V, Habig, A, Halsall, R, Hanson, J, Harris, D, Harris, PG, Hartnell, J, Hartouni, EP, Hatcher, R, Heller, K, Hill, N, Ho, Y, Howcroft, C, Hylen, J, Ignatenko, M, Indurthy, D, Irwin, GM, James, C, Jenner, L, Jensen, D, Joffe-Minor, T, Kafka, T, Kang, HJ, Kasahara, SMS, Kilmer, J, Kim, H, Koizumi, G, Kopp, S, Kordosky, M, Koskinen, DJ, Kostin, M, Krakauer, DA, Kumaratunga, S, Ladran, AS, Lang, K, Laughton, C, Lebedev, A, Lee, R, Lee, WY, Libkind, MA, Liu, J, Litchfield, PJ, Litchfield, RP, Longley, NP, Lucas, P, Luebke, W, Madani, S, Maher, E, Makeev, V, Mann, WA, Marchionni, A, Marino, AD, Marshak, ML, Marshall, JS, McDonald, J, McGowan, A, Meier, JR, Merzon, GI, Messier, MD, Michael, DG, Milburn, RH, Miller, JL, Miller, WH, Mishra, SR, Miyagawa, PS, Moore, C, Morfín, J, Morse, R, Mualem, L, Mufson, S, Murgia, S, Murtagh, MJ, Musser, J, Naples, D, Nelson, C, Nelson, JK, Newman, HB, Nezrick, F, Nichol, RJ, Nicholls, TC, Ochoa-Ricoux, JP, Oliver, J, Oliver, WP, Onuchin, VA, Osiecki, T, Ospanov, R, Paley, J, Paolone, V, Para, A, Patzak, T, Pavlovich, Z, Pearce, GF, Pearson, N, Peck, CW, Perry, C, Peterson, EA, Petyt, DA, Ping, H, Piteira, R, Pla-Dalmau, A, Plunkett, RK, Price, LE, Proga, M, Pushka, DR, Rahman, D, Rameika, RA, Raufer, TM, Read, AL, Rebel, B, Reyna, DE, Rosenfeld, C, Rubin, HA, Ruddick, K, Ryabov, VA, Saakyan, R, Sanchez, MC, Saoulidou, N, Schneps, J, Schoessow, PV, Schreiner, P, Schwienhorst, R, Semenov, VK, Seun, S-M, Shanahan, P, Shield, PD, Smart, W, Smirnitsky, V, Smith, C, Smith, PN, Sousa, A, Speakman, B, Stamoulis, P, Stefanik, A, Sullivan, P, Swan, JM, Symes, PA, Tagg, N, Talaga, RL, Tetteh-Lartey, E, Thomas, J, Thompson, J, Thomson, MA, Thron, JL, Trendler, R, Trevor, J, Trostin, I, Tsarev, VA, Tzanakos, G, Urheim, J, Vahle, P, Vakili, M, Vaziri, K, Velissaris, C, Verebryusov, V, Viren, B, Wai, L, Ward, CP, Ward, DR, Watabe, M, Weber, A, Webb, RC, Wehmann, A, West, N, White, C, White, RF, Wojcicki, SG, Wright, DM, Wu, QK, Yan, WG, Yang, T, Yumiceva, FX, Yun, JC, Zheng, H, Zois, M, and Zwaska, R

Abstract

The complete 5.4 kton MINOS far detector has been taking data since the beginning of August 2003 at a depth of 2070 meters water-equivalent in the Soudan mine, Minnesota. This paper presents the first MINOS observations of νμ and ν̄μ charged-current atmospheric neutrino interactions based on an exposure of 418 days. The ratio of upward- to downward-going events in the data is compared to the Monte Carlo expectation in the absence of neutrino oscillations, giving Rup/downdata/Rup/downMC=0.62-0.14+0.19(stat.) ±0.02(sys.). An extended maximum likelihood analysis of the observed L/E distributions excludes the null hypothesis of no neutrino oscillations at the 98% confidence level. Using the curvature of the observed muons in the 1.3 T MINOS magnetic field νμ and ν̄μ interactions are separated. The ratio of ν̄μ to νμ events in the data is compared to the Monte Carlo expectation assuming neutrinos and antineutrinos oscillate in the same manner, giving Rν̄μ/νμdata/Rν̄μ/νμMC=0.96-0. 27+0.38(stat.)±0.15(sys.), where the errors are the statistical and systematic uncertainties. Although the statistics are limited, this is the first direct observation of atmospheric neutrino interactions separately for νμ and ν̄μ. © 2006 The American Physical Society.

Published
2006

3. First observations of separated atmospheric nu(mu) and (nu)over-bar(mu) events in the MINOS detector

Author

Adamson, P Alexopoulos, T Allison, WWM Alner, GJ and Anderson, K Andreopoulos, C Andrews, M Andrews, R and Arroyo, C Avvakumov, S Ayres, DS Baller, B Barish, B and Barker, MA Barnes, PD Barr, G Barrett, WL Beall, E and Becker, BR Belias, A Bergfeld, T Bernstein, RH and Bhattacharya, D Bishai, M Blake, A Bocean, V Bock, B and Bock, GJ Boehm, J Boehnlein, DJ Bogert, D Border, PM and Bower, C Boyd, S Buckley-Geer, E Byon-Wagner, A Cabrera, A Chapman, JD Chase, TR Chernichenko, SK Childress, S and Choudhary, BC Cobb, JH Cossairt, JD Courant, H and Crane, DA Culling, AJ Dawson, JW DeMuth, DM De Santo, A and Dierckxsens, M Diwan, MV Dorman, M Drake, G Ducar, R and Durkin, T Erwin, AR Escobar, CO Evans, J Fackler, OD and Harris, EF Feldman, GJ Felt, N Fields, TH Ford, R and Frohne, MV Gallagher, HR Gebhard, M Godley, A Gogos, J Goodman, MC Gornushkin, Y Gouffon, P Grashorn, E and Grossman, N Grudzinski, JJ Grzelak, K Guarino, V Habig, A Halsall, R Hanson, J Harris, D Harris, PG and Hartnell, J Hartouni, EP Hatcher, R Heller, K Hill, N and Ho, Y Howcroft, C Hylen, J Ignatenko, M Indurthy, D and Irwin, GM James, C Jenner, L Jensen, D Joffe-Minor, T Kafka, T Kang, HJ Kasahara, SMS Kilmer, J Kim, H and Koizumi, G Kopp, S Kordosky, M Koskinen, DJ Kostin, M Krakauer, DA Kumaratunga, S Ladran, AS Lang, K and Laughton, C Lebedev, A Lee, R Lee, WY Libkind, MA and Liu, J Litchfield, PJ Litchfield, RP Longley, NP Lucas, P Luebke, W Madani, S Maher, E Makeev, V Mann, WA and Marchionni, A Marino, AD Marshak, ML Marshall, JS and McDonald, J McGowan, A Meier, JR Merzon, GI Messier, MD and Michael, DG Milburn, RH Miller, JL Miller, WH and Mishra, SR Miyagawa, PS Moore, C Morfin, J Morse, R and Mualem, L Mufson, S Murgia, S Murtagh, MJ Musser, J and Naples, D Nelson, C Nelson, JK Newman, HB Nezrick, F and Nichol, RJ Nicholls, TC Ochoa-Ricoux, JP Oliver, J and Oliver, WP Onuchin, VA Osiecki, T Ospanov, R Paley, J and Paolone, V Para, A Patzak, T Pavlovich, Z Pearce, GF and Pearson, N Peck, CW Perry, C Peterson, EA Petyt, DA and Ping, H Piteira, R Pla-Dalmau, A Plunkett, RK Price, LE Proga, M Pushka, DR Rahman, D Rameika, RA Raufer, TM Read, AL Rebel, B Reyna, DE Rosenfeld, C Rubin, HA Ruddick, K Ryabov, VA Saakyan, R Sanchez, MC and Saoulidou, N Schneps, J Schoessow, PV Schreiner, P and Schwienhorst, R Semenov, VK Seun, SM Shanahan, P Shield, PD Smart, W Smirnitsky, V Smith, C Smith, PN Sousa, A Speakman, B Stamoulis, P Stefanik, A Sullivan, P and Swan, JM Symes, PA Tagg, N Talaga, RL Tetteh-Lartey, E and Thomas, J Thompson, J Thomson, MA Thron, JL and Trendler, R Trevor, J Trostin, I Tsarev, VA Tzanakos, G and Urheim, J Vahle, P Vakili, M Vaziri, K Velissaris, C and Verebryusov, V Viren, B Wai, L Ward, CP Ward, DR and Watabe, M Weber, A Webb, RC Wehmann, A West, N and White, C White, RF Wojcicki, SG Wright, DM Wu, QK and Yan, WG Yang, T Yumiceva, FX Yun, JC Zheng, H Zois, M Zwaska, R MMINOS Collaboration

Subjects
Physics::Instrumentation and Detectors, High Energy Physics::Experiment
Abstract

The complete 5.4 kton MINOS far detector has been taking data since the beginning of August 2003 at a depth of 2070 meters water-equivalent in the Soudan mine, Minnesota. This paper presents the first MINOS observations of nu(mu) and (nu) over bar (mu) charged-current atmospheric neutrino interactions based on an exposure of 418 days. The ratio of upward- to downward-going events in the data is compared to the Monte Carlo expectation in the absence of neutrino oscillations, giving R-up/down(data)/R-up/down(MC)=0.62(-0.14)(+0.19)(stat.)+/- 0.02(sys.). An extended maximum likelihood analysis of the observed L/E distributions excludes the null hypothesis of no neutrino oscillations at the 98% confidence level. Using the curvature of the observed muons in the 1.3 T MINOS magnetic field nu(mu) and (nu) over bar (mu) interactions are separated. The ratio of (nu) over bar (mu) to nu(mu) events in the data is compared to the Monte Carlo expectation assuming neutrinos and antineutrinos oscillate in the same manner, giving R-(nu) over bar mu/nu(data)(mu)/R-(nu) over bar mu/nu(MC)(mu)=0.96(-0.27)(+0.38)(stat.)+/- 0.15(sys.), where the errors are the statistical and systematic uncertainties. Although the statistics are limited, this is the first direct observation of atmospheric neutrino interactions separately for nu(mu) and (nu) over bar (mu).

Published
2006

4. First observations of separated atmospheric vμ and v̄μ events in the MINOS detector

Author

Adamson, P, Alexopoulos, T, Allison, WWM, Alner, GJ, Andersen, K, Andreopoulos, C, Andrews, M, Andrews, R, Arroyo, C, Avvakumov, S, Ayres, DS, Baller, B, Barish, B, Barker, MA, Barnes Jr, PD, Barr, G, Barrett, WL, Beall, E, Becker, BR, Belias, A, Bergfeld, T, Bernstein, RH, Bhattacharya, D, Bishai, M, Blake, A, Bocean, V, Bock, B, Bock, GJ, Boehm, J, Boehnlein, DJ, Bogert, D, Border, PM, Bower, C, Boyd, S, Buckley-Geer, E, Byon-Wagner, A, Cabrera, A, Chapman, JD, Chase, TR, Chernichenko, SK, Childress, S, Choudhary, BC, Cobb, JH, Cossairt, JD, Courant, H, Crane, DA, Culling, AJ, Dawson, JW, DeMuth, DM, De Santo, A, Dierckxsens, M, Diwan, MV, Dorman, M, Drake, G, Ducar, R, Durkin, T, Erwin, AR, Escobar, CO, Evans, J, Fackler, OD, Falk Harris, E, Feldman, GJ, Felt, N, Fields, TH, Ford, R, Frohne, MV, Gallagher, HR, Gebhard, M, Godley, A, Gogos, J, Goodman, MC, Gornushkin, Y, Gouffon, P, Grashorn, E, Grossman, N, Grudzinski, JJ, Grzelak, K, Guarino, V, Habig, A, Halsall, R, Hanson, J, Harris, D, Harris, PG, Hartnell, J, Hartouni, EP, Hatcher, R, Heller, K, Hill, N, Ho, Y, Howcroft, C, Hylen, J, Ignatenko, M, Indurthy, D, Irwin, GM, James, C, Jenner, L, Jensen, D, Joffe-Minor, T, and Kafka, T

Published
2006

5. First observations of separated atmospheric nu(mu) and (nu)over-bar(mu) events in the MINOS detector

Author

Adamson, P Alexopoulos, T Allison, WWM Alner, GJ and Anderson, K Andreopoulos, C Andrews, M Andrews, R and Arroyo, C Avvakumov, S Ayres, DS Baller, B Barish, B and Barker, MA Barnes, PD Barr, G Barrett, WL Beall, E and Becker, BR Belias, A Bergfeld, T Bernstein, RH and Bhattacharya, D Bishai, M Blake, A Bocean, V Bock, B and Bock, GJ Boehm, J Boehnlein, DJ Bogert, D Border, PM and Bower, C Boyd, S Buckley-Geer, E Byon-Wagner, A Cabrera, A Chapman, JD Chase, TR Chernichenko, SK Childress, S and Choudhary, BC Cobb, JH Cossairt, JD Courant, H and Crane, DA Culling, AJ Dawson, JW DeMuth, DM De Santo, A and Dierckxsens, M Diwan, MV Dorman, M Drake, G Ducar, R and Durkin, T Erwin, AR Escobar, CO Evans, J Fackler, OD and Harris, EF Feldman, GJ Felt, N Fields, TH Ford, R and Frohne, MV Gallagher, HR Gebhard, M Godley, A Gogos, J Goodman, MC Gornushkin, Y Gouffon, P Grashorn, E and Grossman, N Grudzinski, JJ Grzelak, K Guarino, V Habig, A Halsall, R Hanson, J Harris, D Harris, PG and Hartnell, J Hartouni, EP Hatcher, R Heller, K Hill, N and Ho, Y Howcroft, C Hylen, J Ignatenko, M Indurthy, D and Irwin, GM James, C Jenner, L Jensen, D Joffe-Minor, T Kafka, T Kang, HJ Kasahara, SMS Kilmer, J Kim, H and Koizumi, G Kopp, S Kordosky, M Koskinen, DJ Kostin, M Krakauer, DA Kumaratunga, S Ladran, AS Lang, K and Laughton, C Lebedev, A Lee, R Lee, WY Libkind, MA and Liu, J Litchfield, PJ Litchfield, RP Longley, NP Lucas, P Luebke, W Madani, S Maher, E Makeev, V Mann, WA and Marchionni, A Marino, AD Marshak, ML Marshall, JS and McDonald, J McGowan, A Meier, JR Merzon, GI Messier, MD and Michael, DG Milburn, RH Miller, JL Miller, WH and Mishra, SR Miyagawa, PS Moore, C Morfin, J Morse, R and Mualem, L Mufson, S Murgia, S Murtagh, MJ Musser, J and Naples, D Nelson, C Nelson, JK Newman, HB Nezrick, F and Nichol, RJ Nicholls, TC Ochoa-Ricoux, JP Oliver, J and Oliver, WP Onuchin, VA Osiecki, T Ospanov, R Paley, J and Paolone, V Para, A Patzak, T Pavlovich, Z Pearce, GF and Pearson, N Peck and Adamson, P Alexopoulos, T Allison, WWM Alner, GJ and Anderson, K Andreopoulos, C Andrews, M Andrews, R and Arroyo, C Avvakumov, S Ayres, DS Baller, B Barish, B and Barker, MA Barnes, PD Barr, G Barrett, WL Beall, E and Becker, BR Belias, A Bergfeld, T Bernstein, RH and Bhattacharya, D Bishai, M Blake, A Bocean, V Bock, B and Bock, GJ Boehm, J Boehnlein, DJ Bogert, D Border, PM and Bower, C Boyd, S Buckley-Geer, E Byon-Wagner, A Cabrera, A Chapman, JD Chase, TR Chernichenko, SK Childress, S and Choudhary, BC Cobb, JH Cossairt, JD Courant, H and Crane, DA Culling, AJ Dawson, JW DeMuth, DM De Santo, A and Dierckxsens, M Diwan, MV Dorman, M Drake, G Ducar, R and Durkin, T Erwin, AR Escobar, CO Evans, J Fackler, OD and Harris, EF Feldman, GJ Felt, N Fields, TH Ford, R and Frohne, MV Gallagher, HR Gebhard, M Godley, A Gogos, J Goodman, MC Gornushkin, Y Gouffon, P Grashorn, E and Grossman, N Grudzinski, JJ Grzelak, K Guarino, V Habig, A Halsall, R Hanson, J Harris, D Harris, PG and Hartnell, J Hartouni, EP Hatcher, R Heller, K Hill, N and Ho, Y Howcroft, C Hylen, J Ignatenko, M Indurthy, D and Irwin, GM James, C Jenner, L Jensen, D Joffe-Minor, T Kafka, T Kang, HJ Kasahara, SMS Kilmer, J Kim, H and Koizumi, G Kopp, S Kordosky, M Koskinen, DJ Kostin, M Krakauer, DA Kumaratunga, S Ladran, AS Lang, K and Laughton, C Lebedev, A Lee, R Lee, WY Libkind, MA and Liu, J Litchfield, PJ Litchfield, RP Longley, NP Lucas, P Luebke, W Madani, S Maher, E Makeev, V Mann, WA and Marchionni, A Marino, AD Marshak, ML Marshall, JS and McDonald, J McGowan, A Meier, JR Merzon, GI Messier, MD and Michael, DG Milburn, RH Miller, JL Miller, WH and Mishra, SR Miyagawa, PS Moore, C Morfin, J Morse, R and Mualem, L Mufson, S Murgia, S Murtagh, MJ Musser, J and Naples, D Nelson, C Nelson, JK Newman, HB Nezrick, F and Nichol, RJ Nicholls, TC Ochoa-Ricoux, JP Oliver, J and Oliver, WP Onuchin, VA Osiecki, T Ospanov, R Paley, J and Paolone, V Para, A Patzak, T Pavlovich, Z Pearce, GF and Pearson, N Peck

Abstract

The complete 5.4 kton MINOS far detector has been taking data since the beginning of August 2003 at a depth of 2070 meters water-equivalent in the Soudan mine, Minnesota. This paper presents the first MINOS observations of nu(mu) and (nu) over bar (mu) charged-current atmospheric neutrino interactions based on an exposure of 418 days. The ratio of upward- to downward-going events in the data is compared to the Monte Carlo expectation in the absence of neutrino oscillations, giving R-up/down(data)/R-up/down(MC)=0.62(-0.14)(+0.19)(stat.)+/- 0.02(sys.). An extended maximum likelihood analysis of the observed L/E distributions excludes the null hypothesis of no neutrino oscillations at the 98% confidence level. Using the curvature of the observed muons in the 1.3 T MINOS magnetic field nu(mu) and (nu) over bar (mu) interactions are separated. The ratio of (nu) over bar (mu) to nu(mu) events in the data is compared to the Monte Carlo expectation assuming neutrinos and antineutrinos oscillate in the same manner, giving R-(nu) over bar mu/nu(data)(mu)/R-(nu) over bar mu/nu(MC)(mu)=0.96(-0.27)(+0.38)(stat.)+/- 0.15(sys.), where the errors are the statistical and systematic uncertainties. Although the statistics are limited, this is the first direct observation of atmospheric neutrino interactions separately for nu(mu) and (nu) over bar (mu).

Published
2006

6. Improved measurement of muon antineutrino disappearance in MINOS.

Author

Adamson P, Ayres DS, Backhouse C, Barr G, Bishai M, Blake A, Bock GJ, Boehnlein DJ, Bogert D, Cao SV, Childress S, Coelho JA, Corwin L, Cronin-Hennessy D, Danko IZ, de Jong JK, Devenish NE, Diwan MV, Escobar CO, Evans JJ, Falk E, Feldman GJ, Frohne MV, Gallagher HR, Gomes RA, Goodman MC, Gouffon P, Graf N, Gran R, Grzelak K, Habig A, Hartnell J, Hatcher R, Himmel A, Holin A, Huang X, Hylen J, Irwin GM, Isvan Z, Jaffe DE, James C, Jensen D, Kafka T, Kasahara SM, Koizumi G, Kopp S, Kordosky M, Kreymer A, Lang K, Ling J, Litchfield PJ, Loiacono L, Lucas P, Mann WA, Marshak ML, Mathis M, Mayer N, Mehdiyev R, Meier JR, Messier MD, Michael DG, Miller WH, Mishra SR, Mitchell J, Moore CD, Mualem L, Mufson S, Musser J, Naples D, Nelson JK, Newman HB, Nichol RJ, Nowak JA, Oliver WP, Orchanian M, Pahlka RB, Paley J, Patterson RB, Pawloski G, Phan-Budd S, Plunkett RK, Qiu X, Radovic A, Ratchford J, Rebel B, Rosenfeld C, Rubin HA, Sanchez MC, Schneps J, Schreckenberger A, Schreiner P, Sharma R, Sousa A, Strait M, Tagg N, Talaga RL, Thomas J, Thomson MA, Tinti G, Toner R, Torretta D, Tzanakos G, Urheim J, Vahle P, Viren B, Walding JJ, Weber A, Webb RC, White C, Whitehead L, Wojcicki SG, and Zwaska R

Abstract

We report an improved measurement of ν(μ) disappearance over a distance of 735 km using the MINOS detectors and the Fermilab Main Injector neutrino beam in a ν(μ)-enhanced configuration. From a total exposure of 2.95×10(20) protons on target, of which 42% have not been previously analyzed, we make the most precise measurement of Δm2=[2.62(-0.28)(+0.31)(stat)±0.09(syst)]×10(-3)  eV2 and constrain the ν(μ) mixing angle sin2(2θ)>0.75 (90% C.L.). These values are in agreement with Δm2 and sin2(2θ) measured for ν(μ), removing the tension reported in [P. Adamson et al. (MINOS), Phys. Rev. Lett. 107, 021801 (2011).].

Published
2012
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7. Improved search for Muon-neutrino to electron-neutrino oscillations in MINOS.

Author

Adamson P, Auty DJ, Ayres DS, Backhouse C, Barr G, Betancourt M, Bishai M, Blake A, Bock GJ, Boehnlein DJ, Bogert D, Cao SV, Cavanaugh S, Cherdack D, Childress S, Coelho JA, Corwin L, Cronin-Hennessy D, Danko IZ, de Jong JK, Devenish NE, Diwan MV, Dorman M, Escobar CO, Evans JJ, Falk E, Feldman GJ, Frohne MV, Gallagher HR, Gomes RA, Goodman MC, Gouffon P, Graf N, Gran R, Grzelak K, Habig A, Hartnell J, Hatcher R, Himmel A, Holin A, Huang X, Hylen J, Irwin GM, Isvan Z, Jaffe DE, James C, Jensen D, Kafka T, Kasahara SM, Koizumi G, Kopp S, Kordosky M, Kreymer A, Lang K, Lefeuvre G, Ling J, Litchfield PJ, Loiacono L, Lucas P, Mann WA, Marshak ML, Mathis M, Mayer N, McGowan AM, Mehdiyev R, Meier JR, Messier MD, Michael DG, Miller WH, Mishra SR, Mitchell J, Moore CD, Mualem L, Mufson S, Musser J, Naples D, Nelson JK, Newman HB, Nichol RJ, Nowak JA, Ochoa-Ricoux JP, Oliver WP, Orchanian M, Paley J, Patterson RB, Pawloski G, Pearce GF, Phan-Budd S, Plunkett RK, Qiu X, Ratchford J, Rebel B, Rosenfeld C, Rubin HA, Sanchez MC, Schneps J, Schreckenberger A, Schreiner P, Shanahan P, Sharma R, Sousa A, Tagg N, Talaga RL, Thomas J, Thomson MA, Toner R, Torretta D, Tzanakos G, Urheim J, Vahle P, Viren B, Walding JJ, Weber A, Webb RC, White C, Whitehead L, Wojcicki SG, Yang T, and Zwaska R

Abstract

We report the results of a search for ν(e) appearance in a ν(μ) beam in the MINOS long-baseline neutrino experiment. With an improved analysis and an increased exposure of 8.2 × 10(20) protons on the NuMI target at Fermilab, we find that 2 sin(2) (θ(23))sin(2)(2θ(13))<0.12(0.20) at 90% confidence level for δ = 0 and the normal (inverted) neutrino mass hierarchy, with a best-fit of 2sin(2) (θ(23))sin(2)(2θ(13)) = 0.041(-0.031)(+0.047) (0.079(-0.053) (+0.071)). The θ(13) = 0 hypothesis is disfavored by the MINOS data at the 89% confidence level.

Published
2011
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8. First direct observation of muon antineutrino disappearance.

Author

Adamson P, Andreopoulos C, Auty DJ, Ayres DS, Backhouse C, Barr G, Bishai M, Blake A, Bock GJ, Boehnlein DJ, Bogert D, Cavanaugh S, Cherdack D, Childress S, Choudhary BC, Coelho JA, Coleman SJ, Corwin L, Cronin-Hennessy D, Danko IZ, de Jong JK, Devenish NE, Diwan MV, Dorman M, Escobar CO, Evans JJ, Falk E, Feldman GJ, Frohne MV, Gallagher HR, Gomes RA, Goodman MC, Gouffon P, Graf N, Gran R, Grant N, Grzelak K, Habig A, Harris D, Hartnell J, Hatcher R, Himmel A, Holin A, Howcroft C, Huang X, Hylen J, Ilic J, Irwin GM, Isvan Z, Jaffe DE, James C, Jensen D, Kafka T, Kasahara SM, Koizumi G, Kopp S, Kordosky M, Kreymer A, Lang K, Lefeuvre G, Ling J, Litchfield PJ, Loiacono L, Lucas P, Mann WA, Marshak ML, Mayer N, McGowan AM, Mehdiyev R, Meier JR, Messier MD, Miller WH, Mishra SR, Mitchell J, Moore CD, Morfín J, Mualem L, Mufson S, Musser J, Naples D, Nelson JK, Newman HB, Nichol RJ, Nicholls TC, Nowak JA, Ochoa-Ricoux JP, Oliver WP, Orchanian M, Ospanov R, Paley J, Patterson RB, Pawloski G, Pearce GF, Petyt DA, Phan-Budd S, Plunkett RK, Qiu X, Ratchford J, Raufer TM, Rebel B, Rodrigues PA, Rosenfeld C, Rubin HA, Sanchez MC, Schneps J, Schreiner P, Shanahan P, Sousa A, Stamoulis P, Strait M, Tagg N, Talaga RL, Tetteh-Lartey E, Thomas J, Thomson MA, Tinti G, Toner R, Tzanakos G, Urheim J, Vahle P, Viren B, Weber A, Webb RC, White C, Whitehead L, Wojcicki SG, Yang T, and Zwaska R

Abstract

This Letter reports the first direct observation of muon antineutrino disappearance. The MINOS experiment has taken data with an accelerator beam optimized for ν(μ) production, accumulating an exposure of 1.71 × 10²⁰ protons on target. In the Far Detector, 97 charged current ν(μ) events are observed. The no-oscillation hypothesis predicts 156 events and is excluded at 6.3σ. The best fit to oscillation yields |Δm²| = [3.36(-0.40)(+0.46)(stat) ± 0.06(syst)] × 10⁻³ eV², sin²(2θ) = 0.86(-0.12)(+0.11)(stat) ± 0.01(syst). The MINOS ν(μ) and ν(μ) measurements are consistent at the 2.0% confidence level, assuming identical underlying oscillation parameters.

Published
2011
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9. Active to sterile neutrino mixing limits from neutral-current interactions in MINOS.

Author

Adamson P, Auty DJ, Ayres DS, Backhouse C, Barr G, Bishai M, Blake A, Bock GJ, Boehnlein DJ, Bogert D, Cavanaugh S, Cherdack D, Childress S, Coelho JA, Coleman SJ, Corwin L, Cronin-Hennessy D, Danko IZ, de Jong JK, Devenish NE, Diwan MV, Dorman M, Escobar CO, Evans JJ, Falk E, Feldman GJ, Frohne MV, Gallagher HR, Gomes RA, Goodman MC, Gouffon P, Graf N, Gran R, Grant N, Grzelak K, Habig A, Harris D, Hartnell J, Hatcher R, Himmel A, Holin A, Huang X, Hylen J, Ilic J, Irwin GM, Isvan Z, Jaffe DE, James C, Jensen D, Kafka T, Kasahara SM, Koizumi G, Kopp S, Kordosky M, Kreymer A, Lang K, Lefeuvre G, Ling J, Litchfield PJ, Loiacono L, Lucas P, Mann WA, Marshak ML, Mayer N, McGowan AM, Mehdiyev R, Meier JR, Messier MD, Miller WH, Mishra SR, Mitchell J, Moore CD, Morfín J, Mualem L, Mufson S, Musser J, Naples D, Nelson JK, Newman HB, Nichol RJ, Nicholls TC, Nowak JA, Oliver WP, Orchanian M, Paley J, Patterson RB, Pawloski G, Pearce GF, Petyt DA, Phan-Budd S, Pittam R, Plunkett RK, Qiu X, Ratchford J, Raufer TM, Rebel B, Rodrigues PA, Rosenfeld C, Rubin HA, Sanchez MC, Schneps J, Schreiner P, Sharma R, Shanahan P, Sousa A, Stamoulis P, Strait M, Tagg N, Talaga RL, Tetteh-Lartey E, Thomas J, Thomson MA, Tinti G, Toner R, Torretta D, Tzanakos G, Urheim J, Vahle P, Viren B, Walding JJ, Weber A, Webb RC, White C, Whitehead L, Wojcicki SG, and Zwaska R

Abstract

Results are reported from a search for active to sterile neutrino oscillations in the MINOS long-baseline experiment, based on the observation of neutral-current neutrino interactions, from an exposure to the NuMI neutrino beam of 7.07×10(20) protons on target. A total of 802 neutral-current event candidates is observed in the Far Detector, compared to an expected number of 754 ± 28(stat) ± 37(syst) for oscillations among three active flavors. The fraction f(s) of disappearing ν(μ) that may transition to ν(s) is found to be less than 22% at the 90% C.L.

Published
2011
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10. Measurement of the neutrino mass splitting and flavor mixing by MINOS.

Author

Adamson P, Andreopoulos C, Armstrong R, Auty DJ, Ayres DS, Backhouse C, Barr G, Bishai M, Blake A, Bock GJ, Boehnlein DJ, Bogert D, Cavanaugh S, Cherdack D, Childress S, Choudhary BC, Coelho JA, Coleman SJ, Corwin L, Cronin-Hennessy D, Danko IZ, de Jong JK, Devenish NE, Diwan MV, Dorman M, Escobar CO, Evans JJ, Falk E, Feldman GJ, Frohne MV, Gallagher HR, Gomes RA, Goodman MC, Gouffon P, Graf N, Gran R, Grant N, Grzelak K, Habig A, Harris D, Hartnell J, Hatcher R, Himmel A, Holin A, Huang X, Hylen J, Ilic J, Irwin GM, Isvan Z, Jaffe DE, James C, Jensen D, Kafka T, Kasahara SM, Koizumi G, Kopp S, Kordosky M, Kreymer A, Lang K, Lefeuvre G, Ling J, Litchfield PJ, Litchfield RP, Loiacono L, Lucas P, Mann WA, Marshak ML, Mayer N, McGowan AM, Mehdiyev R, Meier JR, Messier MD, Michael DG, Miller WH, Mishra SR, Mitchell J, Moore CD, Morfín J, Mualem L, Mufson S, Musser J, Naples D, Nelson JK, Newman HB, Nichol RJ, Nowak JA, Oliver WP, Orchanian M, Ospanov R, Paley J, Patterson RB, Pawloski G, Pearce GF, Petyt DA, Phan-Budd S, Plunkett RK, Qiu X, Ratchford J, Raufer TM, Rebel B, Rodrigues PA, Rosenfeld C, Rubin HA, Sanchez MC, Schneps J, Schreiner P, Shanahan P, Smith C, Sousa A, Stamoulis P, Strait M, Tagg N, Talaga RL, Thomas J, Thomson MA, Tinti G, Toner R, Tzanakos G, Urheim J, Vahle P, Viren B, Weber A, Webb RC, White C, Whitehead L, Wojcicki SG, Yang T, and Zwaska R

Abstract

Measurements of neutrino oscillations using the disappearance of muon neutrinos from the Fermilab NuMI neutrino beam as observed by the two MINOS detectors are reported. New analysis methods have been applied to an enlarged data sample from an exposure of 7.25×10(20) protons on target. A fit to neutrino oscillations yields values of |Δm(2)|=(2.32(-0.08)(+0.12))×10(-3) eV(2) for the atmospheric mass splitting and sin(2)(2θ)>0.90 (90% C.L.) for the mixing angle. Pure neutrino decay and quantum decoherence hypotheses are excluded at 7 and 9 standard deviations, respectively.

Published
2011
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11. Search for Lorentz invariance and CPT violation with the MINOS far detector.

Author

Adamson P, Auty DJ, Ayres DS, Backhouse C, Barr G, Barrett WL, Bishai M, Blake A, Bock GJ, Boehnlein DJ, Bogert D, Bower C, Budd S, Cavanaugh S, Cherdack D, Childress S, Choudhary BC, Coelho JA, Cobb JH, Coleman SJ, Corwin L, Cravens JP, Cronin-Hennessy D, Danko IZ, de Jong JK, Devenish NE, Diwan MV, Dorman M, Escobar CO, Evans JJ, Falk E, Feldman GJ, Frohne MV, Gallagher HR, Gomes RA, Goodman MC, Gouffon P, Gran R, Grant N, Grzelak K, Habig A, Harris D, Harris PG, Hartnell J, Hatcher R, Himmel A, Holin A, Huang X, Hylen J, Ilic J, Irwin GM, Isvan Z, Jaffe DE, James C, Jensen D, Kafka T, Kasahara SM, Koizumi G, Kopp S, Kordosky M, Krahn Z, Kreymer A, Lang K, Lefeuvre G, Ling J, Litchfield PJ, Loiacono L, Lucas P, Mann WA, Marshak ML, Mayer N, McGowan AM, Mehdiyev R, Meier JR, Messier MD, Michael DG, Miller JL, Miller WH, Mishra SR, Mitchell J, Moore CD, Mualem L, Mufson S, Musser J, Naples D, Nelson JK, Newman HB, Nichol RJ, Oliver WP, Orchanian M, Paley J, Patterson RB, Patzak T, Pawloski G, Pearce GF, Pittam R, Plunkett RK, Ratchford J, Raufer TM, Rebel B, Rodrigues PA, Rosenfeld C, Rubin HA, Ryabov VA, Sanchez MC, Saoulidou N, Schneps J, Schreiner P, Semenov VK, Shanahan P, Smart W, Sousa A, Strait M, Tagg N, Talaga RL, Thomas J, Thomson MA, Tinti G, Toner R, Tzanakos G, Urheim J, Vahle P, Viren B, Weber A, Webb RC, White C, Whitehead L, Wojcicki SG, Wright DM, Yang T, Zois M, and Zwaska R

Abstract

We searched for a sidereal modulation in the MINOS far detector neutrino rate. Such a signal would be a consequence of Lorentz and CPT violation as described by the standard-model extension framework. It also would be the first detection of a perturbative effect to conventional neutrino mass oscillations. We found no evidence for this sidereal signature, and the upper limits placed on the magnitudes of the Lorentz and CPT violating coefficients describing the theory are an improvement by factors of 20-510 over the current best limits found by using the MINOS near detector.

Published
2010
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12. Search for muon-neutrino to electron-neutrino transitions in MINOS.

Author

Adamson P, Andreopoulos C, Arms KE, Armstrong R, Auty DJ, Ayres DS, Backhouse C, Barnes PD Jr, Barr G, Barrett WL, Becker BR, Belias A, Bernstein RH, Betancourt M, Bhattacharya D, Bishai M, Blake A, Bock GJ, Boehm J, Boehnlein DJ, Bogert D, Bower C, Cavanaugh S, Chapman JD, Cherdack D, Childress S, Choudhary BC, Cobb JH, Coelho JA, Coleman SJ, Cronin-Hennessy D, Culling AJ, Danko IZ, de Jong JK, Devenish NE, Diwan MV, Dorman M, Erwin AR, Escobar CO, Evans JJ, Falk E, Feldman GJ, Frohne MV, Gallagher HR, Godley A, Goodman MC, Gouffon P, Gran R, Grashorn EW, Grzelak K, Habig A, Harris D, Harris PG, Hartnell J, Hatcher R, Heller K, Himmel A, Holin A, Howcroft C, Huang X, Hylen J, Irwin GM, Isvan Z, Jaffe DE, James C, Jensen D, Kafka T, Kasahara SM, Koizumi G, Kopp S, Kordosky M, Koskinen DJ, Krahn Z, Kreymer A, Lang K, Ling J, Litchfield PJ, Litchfield RP, Loiacono L, Lucas P, Ma J, Mann WA, Marshak ML, Marshall JS, Mayer N, McGowan AM, Mehdiyev R, Meier JR, Messier MD, Metelko CJ, Michael DG, Miller WH, Mishra SR, Mitchell J, Moore CD, Morfín J, Mualem L, Mufson S, Musser J, Naples D, Nelson JK, Newman HB, Nichol RJ, Nicholls TC, Ochoa-Ricoux JP, Oliver WP, Ospanov R, Paley J, Para A, Patterson RB, Patzak T, Pavlović Z, Pawloski G, Pearce GF, Petyt DA, Pittam R, Plunkett RK, Rahaman A, Rameika RA, Raufer TM, Rebel B, Reichenbacher J, Rodrigues PA, Rosenfeld C, Rubin HA, Ryabov VA, Sanchez MC, Saoulidou N, Schneps J, Schreiner P, Shanahan P, Smart W, Smith C, Sousa A, Speakman B, Stamoulis P, Strait M, Tagg N, Talaga RL, Thomas J, Thomson MA, Thron JL, Tinti G, Toner R, Tsarev VA, Tzanakos G, Urheim J, Vahle P, Viren B, Ward DR, Watabe M, Weber A, Webb RC, West N, White C, Whitehead L, Wojcicki SG, Wright DM, Yang T, Zhang K, Zheng H, Zois M, and Zwaska R

Abstract

This Letter reports on a search for nu(mu) --> nu(e) transitions by the MINOS experiment based on a 3.14x10(20) protons-on-target exposure in the Fermilab NuMI beam. We observe 35 events in the Far Detector with a background of 27+/-5(stat)+/-2(syst) events predicted by the measurements in the Near Detector. If interpreted in terms of nu(mu) --> nu(e) oscillations, this 1.5sigma excess of events is consistent with sin2(2theta(13)) comparable to the CHOOZ limit when |Delta m2|=2.43x10(-3) eV2 and sin2(2theta(23))=1.0 are assumed.

Published
2009
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13. Search for active neutrino disappearance using neutral-current interactions in the MINOS long-baseline experiment.

Author

Adamson P, Andreopoulos C, Arms KE, Armstrong R, Auty DJ, Ayres DS, Backhouse C, Baller B, Barr G, Barrett WL, Becker BR, Belias A, Bernstein RH, Bhattacharya D, Bishai M, Blake A, Bock GJ, Boehm J, Boehnlein DJ, Bogert D, Bower C, Buckley-Geer E, Cavanaugh S, Chapman JD, Cherdack D, Childress S, Choudhary BC, Cobb JH, Coleman SJ, Culling AJ, de Jong JK, Dierckxsens M, Diwan MV, Dorman M, Dytman SA, Escobar CO, Evans JJ, Harris EF, Feldman GJ, Frohne MV, Gallagher HR, Godley A, Goodman MC, Gouffon P, Gran R, Grashorn EW, Grossman N, Grzelak K, Habig A, Harris D, Harris PG, Hartnell J, Hatcher R, Heller K, Himmel A, Holin A, Hsu L, Hylen J, Irwin GM, Ishitsuka M, Jaffe DE, James C, Jensen D, Kafka T, Kasahara SM, Kim JJ, Kim MS, Koizumi G, Kopp S, Kordosky M, Koskinen DJ, Kotelnikov SK, Kreymer A, Kumaratunga S, Lang K, Ling J, Litchfield PJ, Litchfield RP, Loiacono L, Lucas P, Ma J, Mann WA, Marchionni A, Marshak ML, Marshall JS, Mayer N, McGowan AM, Meier JR, Messier MD, Metelko CJ, Michael DG, Miller WH, Mishra SR, Moore CD, Morfín J, Mualem L, Mufson S, Murgia S, Musser J, Naples D, Nelson JK, Newman HB, Nichol RJ, Nicholls TC, Ochoa-Ricoux JP, Oliver WP, Ospanov R, Paley J, Paolone V, Para A, Patzak T, Pavlović Z, Pawloski G, Pearce GF, Peck CW, Petyt DA, Pittam R, Plunkett RK, Rahaman A, Rameika RA, Raufer TM, Rebel B, Reichenbacher J, Rodrigues PA, Rosenfeld C, Rubin HA, Ryabov VA, Sanchez MC, Saoulidou N, Schneps J, Schreiner P, Shanahan P, Smart W, Smith C, Sousa A, Speakman B, Stamoulis P, Strait M, Tagg N, Talaga RL, Tavera MA, Thomas J, Thomson MA, Thron JL, Tinti G, Trostin I, Tsarev VA, Tzanakos G, Urheim J, Vahle P, Viren B, Ward DR, Watabe M, Weber A, Webb RC, Wehmann A, West N, White C, Wojcicki SG, Wright DM, Yang T, Zhang K, and Zwaska R

Abstract

We report the first detailed comparisons of the rates and spectra of neutral-current neutrino interactions at two widely separated locations. A depletion in the rate at the far site would indicate mixing between nu(mu) and a sterile particle. No anomalous depletion in the reconstructed energy spectrum is observed. Assuming oscillations occur at a single mass-squared splitting, a fit to the neutral- and charged-current energy spectra limits the fraction of nu(mu) oscillating to a sterile neutrino to be below 0.68 at 90% confidence level. A less stringent limit due to a possible contribution to the measured neutral-current event rate at the far site from nu(e) appearance at the current experimental limit is also presented.

Published
2008
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14. Testing Lorentz invariance and CPT conservation with NuMI neutrinos in the MINOS near detector.

Author

Adamson P, Andreopoulos C, Arms KE, Armstrong R, Auty DJ, Ayres DS, Baller B, Barr G, Barrett WL, Becker BR, Belias A, Bernstein RH, Bhattacharya D, Bishai M, Blake A, Bock GJ, Boehm J, Boehnlein DJ, Bogert D, Bower C, Buckley-Geer E, Cavanaugh S, Chapman JD, Cherdack D, Childress S, Choudhary BC, Coleman SJ, Culling AJ, de Jong JK, Diwan MV, Dorman M, Dytman SA, Escobar CO, Evans JJ, Falk Harris E, Feldman GJ, Frohne MV, Gallagher HR, Goodman MC, Gouffon P, Gran R, Grashorn EW, Grossman N, Grzelak K, Habig A, Harris D, Harris PG, Hartnell J, Hatcher R, Heller K, Himmel A, Holin A, Hylen J, Irwin GM, Ishitsuka M, Jaffe DE, James C, Jensen D, Kafka T, Kasahara SM, Kim JJ, Koizumi G, Kopp S, Kordosky M, Koskinen DJ, Kreymer A, Kumaratunga S, Lang K, Ling J, Litchfield PJ, Litchfield RP, Loiacono L, Lucas P, Ma J, Mann WA, Marshak ML, Marshall JS, Mayer N, McGowan AM, Meier JR, Messier MD, Metelko CJ, Michael DG, Miller JL, Miller WH, Mishra SR, Moore CD, Morfín J, Mualem L, Mufson S, Murgia S, Musser J, Naples D, Nelson JK, Newman HB, Nichol RJ, Nicholls TC, Ochoa-Ricoux JP, Oliver WP, Ospanov R, Paley J, Paolone V, Para A, Patzak T, Pavlović Z, Pawloski G, Pearce GF, Peck CW, Petyt DA, Pittam R, Plunkett RK, Rahaman A, Rameika RA, Raufer TM, Rebel B, Reichenbacher J, Rodrigues PA, Rosenfeld C, Rubin HA, Sanchez MC, Saoulidou N, Schneps J, Schreiner P, Shanahan P, Smart W, Sousa A, Speakman B, Stamoulis P, Strait M, Tagg N, Talaga RL, Tavera MA, Thomas J, Thompson J, Thomson MA, Thron JL, Tinti G, Tzanakos G, Urheim J, Vahle P, Viren B, Watabe M, Weber A, Webb RC, Wehmann A, West N, White C, Wojcicki SG, Yang T, Zois M, Zhang K, and Zwaska R

Abstract

A search for a sidereal modulation in the MINOS near detector neutrino data was performed. If present, this signature could be a consequence of Lorentz and CPT violation as predicted by the effective field theory called the standard-model extension. No evidence for a sidereal signal in the data set was found, implying that there is no significant change in neutrino propagation that depends on the direction of the neutrino beam in a sun-centered inertial frame. Upper limits on the magnitudes of the Lorentz and CPT violating terms in the standard-model extension lie between 10(-4) and 10(-2) of the maximum expected, assuming a suppression of these signatures by a factor of 10(-17).

Published
2008
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15. Measurement of neutrino oscillations with the MINOS detectors in the NuMI beam.

Author

Adamson P, Andreopoulos C, Arms KE, Armstrong R, Auty DJ, Ayres DS, Baller B, Barnes PD Jr, Barr G, Barrett WL, Becker BR, Belias A, Bernstein RH, Bhattacharya D, Bishai M, Blake A, Bock GJ, Boehm J, Boehnlein DJ, Bogert D, Bower C, Buckley-Geer E, Cavanaugh S, Chapman JD, Cherdack D, Childress S, Choudhary BC, Cobb JH, Coleman SJ, Culling AJ, de Jong JK, Dierckxsens M, Diwan MV, Dorman M, Dytman SA, Escobar CO, Evans JJ, Harris EF, Feldman GJ, Frohne MV, Gallagher HR, Godley A, Goodman MC, Gouffon P, Gran R, Grashorn EW, Grossman N, Grzelak K, Habig A, Harris D, Harris PG, Hartnell J, Hatcher R, Heller K, Himmel A, Holin A, Hylen J, Irwin GM, Ishitsuka M, Jaffe DE, James C, Jensen D, Kafka T, Kasahara SM, Kim JJ, Kim MS, Koizumi G, Kopp S, Kordosky M, Koskinen DJ, Kotelnikov SK, Kreymer A, Kumaratunga S, Lang K, Ling J, Litchfield PJ, Litchfield RP, Loiacono L, Lucas P, Ma J, Mann WA, Marchionni A, Marshak ML, Marshall JS, Mayer N, McGowan AM, Meier JR, Merzon GI, Messier MD, Metelko CJ, Michael DG, Miller JL, Miller WH, Mishra SR, Moore CD, Morfín J, Mualem L, Mufson S, Murgia S, Musser J, Naples D, Nelson JK, Newman HB, Nichol RJ, Nicholls TC, Ochoa-Ricoux JP, Oliver WP, Ospanov R, Paley J, Paolone V, Para A, Patzak T, Pavlović Z, Pawloski G, Pearce GF, Peck CW, Peterson EA, Petyt DA, Pittam R, Plunkett RK, Rahaman A, Rameika RA, Raufer TM, Rebel B, Reichenbacher J, Rodrigues PA, Rosenfeld C, Rubin HA, Ruddick K, Ryabov VA, Sanchez MC, Saoulidou N, Schneps J, Schreiner P, Seun SM, Shanahan P, Smart W, Smith C, Sousa A, Speakman B, Stamoulis P, Strait M, Symes P, Tagg N, Talaga RL, Tavera MA, Thomas J, Thompson J, Thomson MA, Thron JL, Tinti G, Trostin I, Tsarev VA, Tzanakos G, Urheim J, Vahle P, Viren B, Ward CP, Ward DR, Watabe M, Weber A, Webb RC, Wehmann A, West N, White C, Wojcicki SG, Wright DM, Yang T, Zois M, Zhang K, and Zwaska R

Abstract

This Letter reports new results from the MINOS experiment based on a two-year exposure to muon neutrinos from the Fermilab NuMI beam. Our data are consistent with quantum-mechanical oscillations of neutrino flavor with mass splitting |Deltam2| = (2.43+/-0.13) x 10(-3) eV2 (68% C.L.) and mixing angle sin2(2theta) > 0.90 (90% C.L.). Our data disfavor two alternative explanations for the disappearance of neutrinos in flight: namely, neutrino decays into lighter particles and quantum decoherence of neutrinos, at the 3.7 and 5.7 standard-deviation levels, respectively.

Published
2008
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16. Observation of muon neutrino disappearance with the MINOS detectors in the NuMI neutrino beam.

Author

Michael DG, Adamson P, Alexopoulos T, Allison WW, Alner GJ, Anderson K, Andreopoulos C, Andrews M, Andrews R, Arms KE, Armstrong R, Arroyo C, Auty DJ, Avvakumov S, Ayres DS, Baller B, Barish B, Barker MA, Barnes PD Jr, Barr G, Barrett WL, Beall E, Becker BR, Belias A, Bergfeld T, Bernstein RH, Bhattacharya D, Bishai M, Blake A, Bocean V, Bock B, Bock GJ, Boehm J, Boehnlein DJ, Bogert D, Border PM, Bower C, Boyd S, Buckley-Geer E, Bungau C, Byon-Wagner A, Cabrera A, Chapman JD, Chase TR, Cherdack D, Chernichenko SK, Childress S, Choudhary BC, Cobb JH, Cossairt JD, Courant H, Crane DA, Culling AJ, Dawson JW, de Jong JK, DeMuth DM, De Santo A, Dierckxsens M, Diwan MV, Dorman M, Drake G, Drakoulakos D, Ducar R, Durkin T, Erwin AR, Escobar CO, Evans JJ, Fackler OD, Falk Harris E, Feldman GJ, Felt N, Fields TH, Ford R, Frohne MV, Gallagher HR, Gebhard M, Giurgiu GA, Godley A, Gogos J, Goodman MC, Gornushkin Y, Gouffon P, Gran R, Grashorn E, Grossman N, Grudzinski JJ, Grzelak K, Guarino V, Habig A, Halsall R, Hanson J, Harris D, Harris PG, Hartnell J, Hartouni EP, Hatcher R, Heller K, Hill N, Ho Y, Holin A, Howcroft C, Hylen J, Ignatenko M, Indurthy D, Irwin GM, Ishitsuka M, Jaffe DE, James C, Jenner L, Jensen D, Joffe-Minor T, Kafka T, Kang HJ, Kasahara SM, Kilmer J, Kim H, Kim MS, Koizumi G, Kopp S, Kordosky M, Koskinen DJ, Kostin M, Kotelnikov SK, Krakauer DA, Kreymer A, Kumaratunga S, Ladran AS, Lang K, Laughton C, Lebedev A, Lee R, Lee WY, Libkind MA, Ling J, Liu J, Litchfield PJ, Litchfield RP, Longley NP, Lucas P, Luebke W, Madani S, Maher E, Makeev V, Mann WA, Marchionni A, Marino AD, Marshak ML, Marshall JS, Mayer N, McDonald J, McGowan AM, Meier JR, Merzon GI, Messier MD, Milburn RH, Miller JL, Miller WH, Mishra SR, Mislivec A, Miyagawa PS, Moore CD, Morfín J, Morse R, Mualem L, Mufson S, Murgia S, Murtagh MJ, Musser J, Naples D, Nelson C, Nelson JK, Newman HB, Nezrick F, Nichol RJ, Nicholls TC, Ochoa-Ricoux JP, Oliver J, Oliver WP, Onuchin VA, Osiecki T, Ospanov R, Paley J, Paolone V, Para A, Patzak T, Pavlović Z, Pearce GF, Pearson N, Peck CW, Perry C, Peterson EA, Petyt DA, Ping H, Piteira R, Pittam R, Pla-Dalmau A, Plunkett RK, Price LE, Proga M, Pushka DR, Rahman D, Rameika RA, Raufer TM, Read AL, Rebel B, Reichenbacher J, Reyna DE, Rosenfeld C, Rubin HA, Ruddick K, Ryabov VA, Saakyan R, Sanchez MC, Saoulidou N, Schneps J, Schoessow PV, Schreiner P, Schwienhorst R, Semenov VK, Seun SM, Shanahan P, Shield PD, Smart W, Smirnitsky V, Smith C, Smith PN, Sousa A, Speakman B, Stamoulis P, Stefanik A, Sullivan P, Swan JM, Symes PA, Tagg N, Talaga RL, Terekhov A, Tetteh-Lartey E, Thomas J, Thompson J, Thomson MA, Thron JL, Tinti G, Trendler R, Trevor J, Trostin I, Tsarev VA, Tzanakos G, Urheim J, Vahle P, Vakili M, Vaziri K, Velissaris C, Verebryusov V, Viren B, Wai L, Ward CP, Ward DR, Watabe M, Weber A, Webb RC, Wehmann A, West N, White C, White RF, Wojcicki SG, Wright DM, Wu QK, Yan WG, Yang T, Yumiceva FX, Yun JC, Zheng H, Zois M, and Zwaska R

Abstract

This Letter reports results from the MINOS experiment based on its initial exposure to neutrinos from the Fermilab NuMI beam. The rates and energy spectra of charged current nu(mu) interactions are compared in two detectors located along the beam axis at distances of 1 and 735 km. With 1.27 x 10(20) 120 GeV protons incident on the NuMI target, 215 events with energies below 30 GeV are observed at the Far Detector, compared to an expectation of 336+/-14 events. The data are consistent with nu(mu) disappearance via oscillations with |Delta(m)2/32|=2.74 +0.44/-0.26 x10(-3)eV(2) and sin(2)(2theta(23))>0.87 (68% C.L.).

Published
2006
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