%V 101
%J PHYS REV LETT
%L discovery148301
%O © 2008 The American Physical Society
%I AMER PHYSICAL SOC
%A P Adamson
%A C Andreopoulos
%A KE Arms
%A R Armstrong
%A DJ Auty
%A DS Ayres
%A B Baller
%A G Barr
%A WL Barrett
%A BR Becker
%A A Belias
%A RH Bernstein
%A D Bhattacharya
%A M Bishai
%A A Blake
%A GJ Bock
%A J Boehm
%A DJ Boehnlein
%A D Bogert
%A C Bower
%A E Buckley-Geer
%A S Cavanaugh
%A JD Chapman
%A D Cherdack
%A S Childress
%A BC Choudhary
%A SJ Coleman
%A AJ Culling
%A JK de Jong
%A MV Diwan
%A M Dorman
%A SA Dytman
%A CO Escobar
%A JJ Evans
%A EF Harris
%A GJ Feldman
%A MV Frohne
%A HR Gallagher
%A MC Goodman
%A P Gouffon
%A R Gran
%A EW Grashorn
%A N Grossman
%A K Grzelak
%A A Habig
%A D Harris
%A PG Harris
%A J Hartnell
%A R Hatcher
%A K Heller
%A A Himmel
%A A Holin
%A J Hylen
%A GM Irwin
%A M Ishitsuka
%A DE Jaffe
%A C James
%A D Jensen
%A T Kafka
%A SMS Kasahara
%A JJ Kim
%A G Koizumi
%A S Kopp
%A M Kordosky
%A DJ Koskinen
%A A Kreymer
%A S Kumaratunga
%A K Lang
%A J Ling
%A PJ Litchfield
%A RP Litchfield
%A L Loiacono
%A P Lucas
%A J Ma
%A WA Mann
%A ML Marshak
%A JS Marshall
%A N Mayer
%A AM McGowan
%A JR Meier
%A MD Messier
%A CJ Metelko
%A DG Michael
%A JL Miller
%A WH Miller
%A SR Mishra
%A CD Moore
%A J Morfin
%A L Mualem
%A S Mufson
%A S Murgia
%A J Musser
%A D Naples
%A JK Nelson
%A HB Newman
%A RJ Nichol
%A TC Nicholls
%A JP Ochoa-Ricoux
%A WP Oliver
%A R Ospanov
%A J Paley
%A V Paolone
%A A Para
%A T Patzak
%A Z Pavlovic
%A G Pawloski
%A GF Pearce
%A CW Peck
%A DA Petyt
%A R Pittam
%A RK Plunkett
%A A Rahaman
%A RA Rameika
%A TM Raufer
%A B Rebel
%A J Reichenbacher
%A PA Rodrigues
%A C Rosenfeld
%A HA Rubin
%A MC Sanchez
%A N Saoulidou
%A J Schneps
%A P Schreiner
%A P Shanahan
%A W Smart
%A A Sousa
%A B Speakman
%A P Stamoulis
%A M Strait
%A N Tagg
%A RL Talaga
%A MA Tavera
%A J Thomas
%A J Thompson
%A MA Thomson
%A JL Thron
%A G Tinti
%A G Tzanakos
%A J Urheim
%A P Vahle
%A B Viren
%A M Watabe
%A A Weber
%A RC Webb
%A A Wehmann
%A N West
%A C White
%A SG Wojcicki
%A T Yang
%A M Zois
%A K Zhang
%A R Zwaska
%A MINOS Collaboration
%X 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).
%T Testing Lorentz Invariance and CPT Conservation with NuMI Neutrinos in the MINOS Near Detector
%D 2008
%K STANDARD MODEL, VIOLATION
%N 15