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Result in Neutrino Oscillations from 400-Days

Result in Neutrino Oscillations from 400-Days

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p‚yw RHHEhe‰ƒ he„eyp

ƒ €i‚Euewsyuexhi

‰oshit—k— stow

u—miok— y˜serv—tory

snstitute for gosmi™ ‚—y ‚ese—r™hD niversityof„okyoDrig—shiEwozumiD

u—miok—D qifuD SHTEIPD t—p—n

I

‚epresenting ƒup erEu—miok—nde goll—˜ or—tion

efƒ„‚eg„

„he ƒup erEu—miok—nde exp erimentD using the l—rgest underground w—E

ter gerenkov dete™torD h—s ˜ een running sin™e epril ID IWWTF „he tot—l

live time for the —n—lysis h—s re—™hed more th—n QHH d—ysF „he newest

results in —tmospheri™ neutrinoD sol—r —nd rel—ted topi™s —re rep ortedF

pigure IX „he s™hem—ti™ view of ƒup erEu—miok—nde dete™torF

I sntro du™tion

„he ƒup erEu—miok—nde dete™tor is — SHDHHH ton w—ter gerenkov dete™tor lo ™—ted

—t — depth of PDUHH meters w—ter equiv—lent in the u—miok— mine in t—p—nF e

s™hem—ti™ view of dete™tor is shown —s pig IF „he dete™tor ™—vityisRPmin

height —nd QW m in di—meterD lled with SHDHHH tons of pure w—terF „he du™i—l

m—ss for the me—surement of sol—r —nd —tmospheri™ neutrino inter—™tions is PPDHHH

tonsD whi™h is more th—n PH times l—rger th—n th—t of u—miok—ndeF st ™onsists

of twol—yers of dete™torF „he inner t—nk h—s QQFV m di—meter —nd QTFP m highF

IIDIRT SH ™m 0 photomultiplier tu˜ es @€w„sAD instrumented on —ll surf—™es of the

inner dete™torD dete™t gerenkov photons r—di—ted ˜y rel—tivisti™ ™h—rged p—rti™lesF

„he outer l—yerD —pproxim—tely P m thi™kD is used —s —n —ntiE™ounter where IDVVS

PH ™m 0 €w„s is instrumentedF „he —ntiE™ounter is useful for identifying entering

™osmi™Er—y —nd for redu™ing g—mm—Er—ys or neutrons from surrounding

ro ™kF €ulseEheight —nd timing inform—tion from e—™h €w„ —re re™orded —nd used in the d—t— —n—lysisF

ƒup erEu—miok—nde h—s ˜ een su™™essfully op er—ted without —ny serious trou˜les

sin™e epril IstD IWWTF „he dete™tor h—s ˜ een —live in VS 7 of the timeF wost

of the de—d time is due to ™—li˜r—tionsF „he ™umul—tive liveEtime of op er—tion

re—™hed more th—n SHH d—ys in the f—ll of IWWUF „he tr—nsp—ren™y of w—ter is

—˜ out VH m me—sured ˜y using ele™trons from " de™—yF „he trigger threshold h—d

˜ een —˜ out SFT we† for ele™trons —t SH7 e™ien™y from the ˜ eginning of the

exp erimentF st h—s ˜ een set to —˜ out RFT we† sin™e w—y IWWU to ™olle™t — mu™h

lower d—t— s—mpleF „he ™on™entr—tion of ‚n in the w—ter is less th—n S m

Q

fqGm whi™h is two order of m—gnitude lower th—n th—t in u—miok—ndeF „he tot—l

liveEtime of d—t— s—mple for —n—lysis of sol—r neutrinoD upEgoing "D —tmospheri™

neutrino —nd proton de™—y h—s re—™hed more th—n QHH d—ysF xow it is time to

o˜t—in the ™on™lusive results in neutrino os™ill—tion studies with l—rge st—tisti™sF sn

the following se™tionsD new results in sol—r neutrino —nd in —tmospheri™ neutrino

—n—lyses —re presentedF

P ƒol—r

„he ƒun m—int—ins its luminosity ˜y the energy of nu™le—r fusion re—™tionsF „hus

the ƒun emits lowEenergy @i IS we†A ele™tron neutrinos @# A th—t —re pro dE

# e

u™ts of the nu™le—r pro ™esses inside the ƒunF yur underst—nding of those proE

™esses is ree™ted in the st—nd—rd sol—r mo del @ƒƒwAF „he ux —nd sp e™trum of

neutrinos ™orresp onding to e—™h nu™le—r pro ™ess —re well predi™ted ˜y ƒƒwF pigE

ure P shows the energy sp e™tr— of the sol—r neutrino ux on the e—rth ™—l™ul—ted

P

˜y ƒƒw of f—h™—ll —nd €insonne—ult in IWWS @f€EWSAF elso shown —re the enE

ergy threshold of ve ™urrent existing sol—r neutrino exp erimentsD the romest—ke

Q R S T

exp erimentD u—miok—ndeD ƒeqiD qevviˆ —nd the presented exp erimentD

U

ƒup erEu—miok—ndeD in the s—me gureF

„he rst o˜serv—tion of the sol—r neutrino w—s —™hieved in the e—rly IWUH9s

QU QU

˜y h—vis et —lF ˜y using of following re—™tionsY gl C # 3 el C e @i !

e #

HFVIR we†AF „heir o˜t—ined result h—ve shown — signi™—nt de™it of the yield

™omp—red to predi™tions ˜—sed on v—rious versions of the ƒƒwF „he ƒeqi —nd

UI UI

qevviˆ exp eriments used following re—™tionsY q— C # 3 qe C e @i ! HFPQQ

e #

we†AF „hose exp eriments ™—n dete™t mu™hlower energy neutrinos pro du™ed vi—

’pEp4 ™h—in th—t m—int—in most of the ƒun9s luminosityF „he o˜t—ined results

—re —˜ out h—lf of the exp e™ted oneF u—miok—nde h—s p erformed the rst re—l

time me—surement of sol—r neutrinos ˜y using of w—ter gerenkov te™hniqueF ƒol—r

neutrinos ™—n ˜ e dete™ted through neutrinoEele™tron s™—tteringD #e 3 #eF „he

ele™tron energyD dire™tion —nd the time of the re—™tion —re me—suredF „he o˜t—ined

result w—s —˜ out RH 7 of the exp e™t—tionF

„he ux me—surements —re summ—rized in the „—˜le IF ell the exp eriments

showed signi™—ntly lower ux th—n th—t from the ƒƒw predi™tionD while the

dete™tion metho ds —nd the energy thresholds of the me—surement —re dierent

—mong e—™h otherF st is h—rd to expl—in —ll the existing results ™onsistently with

ƒƒwF „he sol—r neutrinos whi™h —re exp e™ted to ˜ e dete™ted in the romest—ke

V U

exp eriment —re —˜ out VH 7 from fEneutrino —nd —˜ out IS 7 from feEneutrinoD

V

while only fEneutrino ™—n ˜ e dete™ted ˜y the w—ter gerenkov dete™torsF „he

o˜t—ined h—t—Gƒƒw in the romest—ke exp eriment is —˜ out IGQD while it is —˜ out

one h—lf in u—miok—ndeF „his dieren™e suggests —lmost no ™ontri˜ution from

U

feEneutrino in the romest—ke d—t—F yn the other h—ndD the ™ontri˜ution of ’pE

U V

p4EneutrinosD feEneutrino —nd fEneutrino in the d—t— s—mple of q— exp eriments

—re exp e™ted to ˜ e —˜ out SH 7D QH 7 —nd IH 7D resp e™tivelyF „he ux of ’pEp4E

neutrino is ™onstr—ined ˜y tot—l luminosity of the ƒunF st —g—in m—y suggest strong

U

suppression of feEneutrinosF „hose results from the existing exp eriments hints —

p ossi˜le distortion of energy sp e™trum of sol—r neutrinos whi™h ™—n ˜ e expl—ined ˜y

the hyp othesis of # 3 # os™ill—tions os™ill—tionF „he dist—n™e ˜ etween the e—rth

e x

II IH P

—nd the ƒun is $ IH m —nd i $ IH we†D so th—t typi™—l iGv is IH F sf the m

#

IH P

is su˜st—nti—lly l—rger th—n IH e† D sol—r neutrinos with —ny energy —re fully

os™ill—ted in the ™—se of v—™uum os™ill—tionsF „hus h—t—Gƒƒw of —ll the existing

exp eriments should ˜ e s—me —nd the dierent h—t—Gƒƒw —mong the exp eriments

P

P

—re h—rdly expl—inedF yne of the s™en—rio is th—t m —nd sin P eventu—lly t—ke

P

P IH

’go o d4 v—luesD for ex—mple @m Dsin P A$@IH DIAD to expl—in —ll the resultsF

„his s™en—rio is soE™—lled the justEso os™ill—tionF pigure QD t—ken from ‚efFV shows

P

P

the WS7 gFvF —llowed regions of justEso solution in @m D sin P A sp—™eF „he

other —ttr—™tive s™en—rio whi™h ™ould expl—in —ll the exp eriment—l results is m—tter

W

enh—n™ed os™ill—tions of sol—r neutrinosD soE™—lled wƒ‡ os™ill—tionF pigure RD

V P

t—ken from ‚efF shows the WS7 gFvF —llowed regions of wƒ‡ solution in @m D

P

sin P A sp—™eF „here —re two dom—ins of —llowed regionsD so ™—lled sm—ll —ngle

solution —nd l—rge —ngle solutionF st is predi™ted th—t the energy sp e™trum of sol—r

neutrinos would ˜ e distorted in the ™—se of the sm—ll —ngle solutionF yn the other

h—ndD the d—yGnight ee™tD th—t isD — dieren™e ˜ etween d—y —nd night uxD would

pigure PX „he energy sp e™tr— of the sol—r neutrino uxF elso shown —re the energy

threshold of the existing sol—r neutrino exp erimentsF

˜ e o˜served in the ™—se of the l—rge —ngle solutionF ‚e—lEtime me—surement of

sol—r neutrino is indisp ens—˜le to dete™t those ee™tsD whi™h would ˜ e — strong

eviden™e of wƒ‡ os™ill—tionF ƒup erEu—miok—nde ™—n provide — huge st—tisti™s for

those me—surement with its l—rge du™i—l m—ssF

„he presented sol—r neutrino d—t— of QURFP liveEd—ysD ™overing — p erio d from

w—y QID IWWT through y™t PHD IWWUF pirstD ™osmi™ r—ymuons —nd de™—y ele™E

trons —re dis™—rded from the d—t— s—mple using tot—l energy dep osit in the deE

te™tor —nd time dieren™e of the eventsF „he vertex p osition of # Ee s™—ttering

—nd the dire™tion of ele™trons h—ve ˜ een re™onstru™ted ˜y using —rriv—lEtime inE

form—tion of gerenkov photons on the €w„9s of inner dete™torF „he energy of

ele™tron h—s ˜ een determined from — num˜er of hit €w„9s in — SH ns windowF

„he energy s™—leD the energy resolutionD the —ngul—r resolution —nd the vertex

p osition resolution —re ™—li˜r—ted m—inly with the ele™tron ˜ e—m from — vsxeg

systemF „he vsxeg system ™—n pro du™e —n ele™tron ˜ e—m of S$IT we† inje™ted

to v—rious p ositions in the dete™torF „he energyD —ngul—r —nd p osition resoluE

tions for VFT we† ele™trons —re IT 7D PU degF —nd VS ™mD resp e™tivelyF „he

un™ert—inty of —˜solute energy s™—le is I 7F foth of the p osition dep enden™e

—nd time v—ri—n™e of the energy s™—le —re I7D whi™h h—s ˜ een ™he™ked with

— xiEgf sour™e ˜y using the re—™tion xi@nD AxiF „o elimin—te the ˜—™kground

@A

„—rget@ixpFA h—t— ƒƒw @f€EWSA h—t—Gƒƒw

CS CV CHXHVP

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TWIH IQU HFSHR q—@ƒeqiA

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CQXW CV CHXHSU

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q—@qevviˆA TWFUTFU IQU HFSHW

RXS U HXHSW

CIXP

QU

gl@romest—keA PFSSHFIRHFIR WFQ HFPUQHFHPI

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CHXWQ

e @r yDu—miok—ndeA PFVHHFIWHFQQ TFTP HFRPQHFHSV

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IXIP

CHXHT CHXHW CHXWQ CHXHIU

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e @r yDƒup erEu—mFA PFQU TFTP HFQSV

P

HXHS HXHU IXIP HXHIQ

@A ixp eriment—l errors onlyF ƒt—tisti™—l —nd system—ti™ errors —re —dded in qu—dr—tureF

@A €relimin—ryF

P

„—˜le IX ‚esults from ™urrent ve exp eriments —nd the ƒƒw f€EWS predi™tions on

QU UI T P

the sol—r neutrino uxF rere the unit is ƒx for gl —nd q— —nd IH #a™m ase™

for e @r yA t—rgetD resp e™tivelyD where ƒx me—ns ’sol—r neutrino unit4 dened

P

QT

˜y I ƒx aIH # ™—ptures p er —tom p er se™ondF )) 2 -9.4 (eV 2 m

∆ -9.6

log( -9.8

-10

-10.2

-10.4

-10.6

-10.8

-11

-11.2 spectrum 0 0.2 0.4 0.6 0.8 1

sin22θ

pigure QX „he WS 7 gFvF —llowed region of justEso os™ill—tion ˜y r—t— —nd v—nE

V

g—™ker —re shown ˜y the sh—ded regionF elso shown —re the prelimin—ry WS7

gFvF —nd WW7 gFvF ™ontours —t justEso region from sp e™trum —n—lysis without ux

™onstr—int in ƒup erEu—miok—ndeF snsides of d—shed lines —re —llowed —t WS7 gFvFD

—nd right side of solid line is ex™luded —t WW7 gFvF from sp e™trum —n—lysisF )) -3

)) -3 2 2 2 (eV (eV 2 2 2 m m ∆ ∆ -4 log( log(

-5

-6

-7

spectrum day and night 5bins -8 -4 -3.5 -3 -2.5 -2 -1.5 -1 -0.5 0

log(sin22θ)

V

pigure RX WS7 gFvF —llowed region of wƒ‡ os™ill—tion ˜y r—t— —nd v—ng—™ker

—re shown ˜y the sh—ded regionF elso shown is WS7 gFvF ex™luded region of wƒ‡

P

P

os™ill—tion —n—lysis without ux ™onstr—intin@m Dsin P A sp—™eF h—yGnight

—n—lysis ex™ludes region inside of solid line —nd sp e™trum —n—lysis ex™ludes regions inside of d—shed linesF 0.3 SK 374day 6.5-20MeV 22.5kt ALL 0.25

0.2 Events/day/kton/bin

0.15

0.1

0.05

0 -1 -0.5 0 0.5 1 θ

cos

pigure SX €relimin—ry sol—r neutrino d—t— from the ƒup erEu—miok—nde exp eriment

in QURFP d—ys of o˜serv—tionF e ™le—r ex™ess of events ne—r ™os aI is seenF „he

sun

sh—p e of the ex™ess distri˜ution is repro du™ed well ˜y the wg simul—tion with the

V

f ux of HFQSVƒƒwF

events due to —™tivity from surrounding ro ™ksD we required — dist—n™e of the verE

tex from the inner dete™tor w—ll is more th—n P mF „his ™orresp onds PPFS kt —s

— du™i—l m—ssF enother ˜—™kground due to the —™tivity from nu™le—r fr—gments

pro du™ed ˜y " sp—ll—tion h—s ˜ een redu™ed ˜y ™he™king the dist—n™e —nd time

interv—l ˜ etween — event —nd — prior ™osmi™ r—y " eventF pin—lly the distri˜ution

of dire™tion—l ™orrel—tion to the ƒun h—s ˜ een o˜t—ined for the events where enE

ergy of ele™trons —re ˜ etween TFS —nd PH we† —s shown in pigF SF „he num˜er of

CIIUXW CRRR

o˜t—ined sol—r neutrino events is RWSIFV @st—tFA @systFA whi™h ™orresp onds

IIIXQ ISR

CHXHT CHXHW

T P V

to PFQU @st—tFA @systFA IH G™m Gs —s — fEneutrino uxF „he o˜t—ined

HXHS HXHU

CHXHHW CHXHIR

h—t—Gƒƒw is HFQSV @st—tFA @systFAF „he presented result of tot—l ux is

HXHHV HXHIH

™onsistent to the previous result o˜served in u—miok—ndeF xote th—t the num˜er

of o˜t—ined sol—r neutrinos ˜y ƒup erEu—miok—nde in IFS ye—r op er—tion is more

th—n eight times l—rger th—n th—t ˜y u—miok—nde in seven ye—rs op er—tionF

„he ux dieren™e ˜ etween d—y —nd night is expressed —sX @h—yExightA a 1

BP95 cosθ 0.9 day SK night1 0.8 night2 night3 data/SSM

0.7 night4

0.6 night5

0.5

0.4

0.3

0.2 day night1 night2 night3 night4 night5 0.1

0

-0.2 0 0.2 0.4 0.6 0.8 1

pigure TX €relimin—ry reslts in h—yGxight ee™tF irror ˜—rs —re st—tisti™—l onlyF

xight d—t— is divided into S ˜insF xightI is horizont—l dire™tion —nd nightS is

verti™—l dire™tionF „he histogr—m with dotted lines is the exp e™ted v—ri—tion of

the typi™—l l—rge —ngle solution —nd histogr—m with d—shed lines is th—t of the

typi™—l sm—ll —ngle solution @see textAF

@h—yCxightA a EHFHQIHFHPR@st—tFAHFHIR@systFAF ‡ithin the st—tisti™sD there isD

so f—rD no eviden™e for the d—yGnight ee™tF pigure P shows the sol—r neutrino

ux in d—y —nd night p erio dsF „he night —nd d—y ux —re su˜ divided into S ˜ins

—™™ording to the —ngle ˜ etween the dire™tion to the ƒun —nd the n—dir of the

dete™torF „he SE˜inned histogr—ms exp e™ted from wƒ‡ os™ill—tion with typi™—l

P

P Q T

p—r—meters in the sm—ll mixing solutionD @m Dsin P Aa@WXIP  IH DTXQI  IH A

P

P S

—nd in the l—rge —ngle solutionD @m Dsin P Aa@PXVP  IH D HFTTA —re —lso shown

in the gureF „he d—t— seems to —gree with no d—yGnight ee™tD ˜ut —lso to —gree

with the d—yGnight ee™t with some p—r—meters of the l—rge —ngle solutionF „he

impli™—tion in the wƒ‡ os™ill—tion h—s ˜ een p erformed for the SE˜inned d—yGnight

result —s shown in pig PF „his —n—lysis is — mo del indep endent —n—lysisD sin™e only

V

the v—ri—tion of fEneutrino ux ˜ etween d—y —nd night is usedF „he ex™luded 1.2 BP95

1 data/SSM

0.8

0.6

0.4

0.2

0 7 8 9 10 11 12 13 14 15

MeV

"

pigure UX €relimin—ry plot of h—t—Gƒƒw —s — fun™tion of ele™tron energy from

ƒup erEu—miok—ndeF „he most right ˜in shows the d—t— with ele™tron energy more

th—n IR we†F snner error ˜—rs —re the st—tisti™—l ones —nd outer ˜—rs —re the

system—ti™ errors —dded line—rly with st—tisti™—l onesF h—shed histogr—m is the

exp e™ted sp e™trum of the typi™—l sm—ll —ngle solution —nd dotted histogr—m is

th—t of the typi™—l justEso solution @see textAF

region —t WS7 gFvF from the —n—lysis of o˜t—ined results in d—yGnight ee™t —re

P

plotted in pigure RF „he presented results h—ve ex™luded lower m region in

the l—rge —ngle solutionF

pigure U shows h—t—Gƒƒw —s — fun™tion of ele™tron energyF „he inside error

˜—rs show st—tisti™—l errorsD —nd outside ˜—rs show the system—ti™ error m—inly

due to un™ert—inty in the energy s™—le —nd energy resolutionF „hese system—ti™

errors —re fully ™orrel—ted to the energy of ele™tronsF elso shown —re the exp e™ted

P

P Q T

sp e™trum of typi™—l sm—ll —ngle solutionD @m Dsin P Aa@WXIP  IH DTXQI  IH A

P

P II

—nd the typi™—l just so os™ill—tionD @m Dsin P Aa@UXHV  IH D HFVQAF „here

—pp e—rs to ˜ e no signi™—nt distortion in the o˜t—ined sp e™trumF roweverD it is

interesting th—t p ossi˜le distorted sp e™tr— ˜y neutrino os™ill—tionsD for ex—mple —s

P

shown in the gureD —lso —gree with d—t— —nd even give ˜ etter 1 for the ttingF „he mo del indep endent impli™—tion of the energy sp e™trum h—s ˜ een p erformed

in wƒ‡ p—r—meter region —nd in justEso p—r—meter regionF ‡eh—ve not used the

V

™onstr—int to fEneutrino ux from ƒƒw due to PH 7 un™ert—inty for the —n—lysisF

„he ™ontour plots for wƒ‡ os™ill—tion —nd for justEso os™ill—tion —re shown in

pigF R —nd in pigF QD resp e™tivelyF „he —˜sen™e of signi™—nt distortion of the

energy sp e™trum ex™ludes some region in ˜ oth of the p—r—meter sp—™eF fe™—use of

— go o d t of the sp e™trum in justEso regionD the WS 7 gFvF —llowed region —pp e—rs

—s shown in pig QD though the no os™ill—tion hypothesis is still —llowed —t WW 7

gFvF

Q etmospheri™ neutrino

etmospheri™ neutrinos —re pro du™ed ˜y the de™—y of % or u pro du™ed ˜y the

inter—™tion of prim—ry ™omp onent of ™osmi™ r—y in the —tmosphereF „he typi™—l

—ltitude where —tmospheri™ neutrinos —re pro du™ed is IH km so th—t the typi™—l

R

ight length of neutrinos is $ IH km for downgoing ones —nd $ IH km for upgoing

onesF „he # a# r—tio of the —tmospheri™ neutrino ux ˜ elow — few qe† is roughly

" e

PD sin™e % de™—y is domin—nt —nd the % 3 " 3 e de™—y ™h—in —s following is

   

% 3 " C # @"# AY" 3 e C # @"# AC# " @# AF @rere—fter # represents # C"# FA st

" " e e " "

go es up more th—n P for higher energy neutrinos sin™e high energy "9s hits grounds

˜ efore their de™—yF „he tot—l ux of —tmospheri™ neutrinos h—s ˜ een ™—l™ul—ted

˜y sever—l mo delF „he un™ert—inty of the ux is —˜ out PH7D while the un™ert—inty

of # a# r—tio isS7˜elow — few qe† regionF „o ™op e with dete™tion e™ien™y

" e

of the dete™torD the ’dou˜le r—tio ‚4 dened —sY

@# a# A

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‚ a Y @IA

@# a# A

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is often usedF sf @# a# A is ™onsistent with the predi™tionD ‚ should t—ke unityF

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sn re™ent ye—rsD there h—ve ˜ een sever—l me—surements of # a# r—tio ˜y w—ter

" e

IH II IP

gerenkov dete™torsD swfEQ D u—miok—ndeD —nd tr—™king type dete™torsD x E

IQ IR IS

ƒiˆD prejus —nd ƒoud—nEPF „wo w—ter gerenkov exp erimentsD u—miok—nde

—nd swfD h—ve o˜t—ined ™onsistent result whi™h is su˜st—nti—lly sm—ller th—n unityF

„he —nom—ly of "ae r—tio ™—n ˜ e interpreted —s p ossi˜le neutrino os™ill—tionD for

ex—mpleD # 3 # or # 3 # F yn the other h—ndD the result of x ƒiˆ —nd

" e " (

prejus seems to ˜ e ™onsistent with unityD while their st—tisti™s —re not su™ient

for ™on™lusive resultF purthermoreD re™ent d—t— from ƒoud—nEP —gree with the d—t—

from the w—ter gerenkov dete™torsD —lthough the v—lue of unity is still —llowed —t

„—˜le PX ixp eriment—l results on the —tmospheri™ @# G# A r—tioF

" e

ixpF h—t— wg @"aeA a@"aeA

d—t— wg

eElike "Elike eElike "Elike

CHXQS

x ƒiˆ IV QP PHFS QTFV HFWW c

HXPS

prejus US IPS VIFR IQTFP IFHHHFISHFHV

CHXHR

ƒoud—nEP UWFI SRFT HFTUHFIS

HXHT

QPS IVP PSUFQ PTVFH HFSRHFHSHFIP swfEQ@su˜Eqe†A

@A

@multiEqe†A PS RU QHFV RIFP IFRHHFTTHFPI

CHXHT

u—miok—nde@su˜Eqe†A PRV PQR PPUFT QSTFV HFTH HFHS

HXHS

CHXHV

WV IQS TTFS ITPFP HFSU HFHU @multiEqe†A

HXHU

CHXHPW

@A

ƒup erEu—mF@su˜Eqe†A WVQ WHH VIPFP IPIVFQ HFTI HFHRW

HXHPV

CHXHTW

@A

@multiEqe†A PIV IUT IVPFU PPWFH HFTR HFHWU

HXHTP

CHXHSW

@A @A

| PHH | PRRFV HFTU HFHVI @€gA

HXHSR

€relimin—ryF

@A „he dou˜le r—tio is for the ™om˜ined s—mple of pg —nd €g eventsF

P' levelF „hough the theoreti™—l un™ert—inty of —˜solute ux —nd inter—™tion ™ross

se™tions of neutrinos —re l—rgeD they should ™—n™el in the dou˜le r—tioF ren™eD the

sm—ll dou˜le r—tio ™—n ˜ e ™onsidered —s p ossi˜le eviden™e of # 3 # or # 3 #

" e " (

os™ill—tionsF

enother indi™—tion of the os™ill—tion of —tmospheri™ neutrinos is the distortion

of zenith —ngle distri˜ution of neutrino uxF „he ux of —tmospheri™ neutrinos

dep ends on zenith —ngleF „his dep enden™e is ™—used ˜y the dieren™e of ee™tive

thi™kness of —tmosphereF ren™eD the sh—p e of zenith —ngle distri˜ution should ˜ e

symmetri™ for upgoing versus downgoing neutrinosF „ypi™—l iGv for —tmospheri™

I R

neutrinosD for ex—mpleD of I qe† is IH for downgoing —nd IH for upgoingF

„hereforeD p ossi˜le distortion of zenith —ngle distri˜ution is ™le—r eviden™e of neuE

trino os™ill—tionsF ynly the u—miok—nde exp eriment h—s rep orted the zenith —ngle

IP

distri˜utions of neutrino ux for the time ˜ eingF „hey rep orted — p ossi˜le disE

tortion of zenith —ngle distri˜utions in multiEqe† s—mple @i higher th—n roughly

#

P P P

I qe†AD whi™h suggests the neutrino os™ill—tion with m $ IH e† —nd with

the l—rge mixing —ngle —s shown in pigF VF wu™h more d—t— —re needed to est—˜E

lish the os™ill—tion of —tmospheri™ neutrinosF ƒup erEu—miok—nde ™—n ™olle™t l—rge

st—tisti™s whi™h —re indisp ens—˜le to test the os™ill—tion hypothesis —nd to derive 0 0

)) (a) (b) 2 U

(eV F

2 -0.5 -0.5 m ∆ Kamiokande

log( -1 -1

Kr Kamiokande -1.5 -1.5

-2 B -2

Super- -2.5 -2.5 Kamiokande

-3 -3 Ch I -3.5 -3.5 0 0.2 0.4 0.6 0.8 1 0 0.2 0.4 0.6 0.8 1

sin22θ sin22θ

P

P

pigure VX ellowed regions @WH 7 gvA in the @m Y sin P A sp—™e @—A for # #

" e

os™ill—tion —nd @˜A for # # os™ill—tionF ‚egions with di—gon—l lines show the

" (

IP

—llowed regions o˜t—ined ˜y u—miok—nde F „he sh—ded region in @˜A is the prelimE

in—ry —llowed region ˜y ƒup erEu—miok—ndeF yther lines indi™—te the regions —˜ ove

IT

—nd to their right —re ex™ludedY fD fugey re—™tor exp eriment Y urD ur—snoy—rsk

IU IV

re—™tor exp eriment Y ghD gho oz re—™tor exp eriment YpDprejus fullyE™ont—ined

IR IW

—tmospheri™ neutrinos Y D ™ompil—tion of upw—rd throughEgoing muons d—t— Y

PH

sD swf upw—rd stopping muons F ƒup erEu—miok—nde9s —n—lysis on # # os™ilE

" e

l—tion w—s not re—dyF

the os™ill—tion p—r—meters from dou˜le r—tio —nd zenith —ngle distri˜utionF

‡e h—ve —n—lyzed fullyE™ont—ined @pgA events of RIRFP live d—ys @PSFS ktonE

ye—rsA —nd — p—rti—llyE™ont—ined @€gA events QUHFV live d—ys @PPFV ktonEye—rsAF

sn — pg eventD —ll the ™h—rged p—rti™les —re ™ont—ined in the inner dete™tor —nd

the tot—l energy of the event is fully re™onstru™tedF sn — €g eventD one ™h—rged

p—rti™leD usu—lly "D es™—p es from the inner dete™tor —nd dep osits energy in the

outer dete™torF „o sep—r—te — pg event from — €g eventD we h—ve required tot—l

num˜er of hits in — sp—ti—l ™luster in the outer dete™tor to ˜ e less th—n IHF foth pg

—nd €g events h—ve ˜ een dou˜ly s™—nned ˜y physi™ists to elimin—te ˜—™kground

events due to dete™tor noiseF „hen the vertex p osition of the neutrino inter—™tion

—nd gerenkov rings h—ve ˜ een re™onstru™ted —utom—ti™—lly ˜y — ™omputerF „he

vertex p osition resolution is estim—ted to ˜ e QH ™m for single ring pg eventsF „he

—ngul—r resolution of single ring pgevents is estim—ted to ˜ e Q degreesF pin—llyD

— P m du™i—l ™ut h—s ˜ een —pplied for events in ˜ oth the pg —nd €g s—mplesF

„ot—l visi˜le energy ™utsD i ! QH we† —nd i ! QSH we† h—ve ˜ een —pplied

vis vis

for the pg —nd the €g s—mpleD resp e™tivelyF „he —™™ur—™y of the —˜solute energy

s™—le is estim—ted to ˜ e PFR 7 ˜—sed on sever—l ™—li˜r—tion sour™esX ™osmi™ r—y

throughEgoing muonsD stopping muonsD muonEde™—y ele™tronsD the inv—ri—nt m—ss

H

of % 9s pro du™ed ˜y neutrino inter—™tionsD xiEgf sour™e ™—li˜r—tionD —nd the SEIT

we† vsxegF „he of p—rti™les —re determined from the tot—l num˜er of

photoEele™trons within — UH degrees h—lfE—ngle ™one rel—tive to the tr—™k dire™tionF

p

„he estim—ted momentum resolution for ele™trons —nd muons is PFS7G i CHFS 7

—nd Q 7D resp e™tivelyD where i is the energy of ele™tron in qe† unitF efter those

redu™tionsD the num˜ er of neutrinos is QDRTP for the pg s—mple —nd PHH for the

€g s—mpleF ivents p er d—y is VFR for the pg s—mple —nd HFSR for the €g s—mpleF

sn the pg eventsD single ring events h—ve ˜ een sele™tedF pigure W shows — typi™—l

single ring ’"Elike4 event —nd —n ’eElike4 eventF „here is — dieren™e ˜ etween the

sh—p e of rings in the gureD sin™e — gerenkov ring from ele™trom—gneti™ ™—s™—des

™—use — more diuse photon distri˜ution th—n th—t from muonsF „he p—rti™le

identi™—tion @€shA metho d whi™h uses the distri˜ution of gerenkov photons in

— ring —s well —s the op ening —ngle of the ring —re —pplied to distinguish muons

from ele™tronsF pigure IH shows the result of €sh for single ring pg eventsF „hose

two p e—ks ™orresp onding to " —nd e —re ™le—rly sep—r—ted in these distri˜utionsF

„he pro˜—˜ility of misEidenti™—tion dedu™ed from wonteg—rlo is less th—n HFS7

for the single ring pg s—mpleF „he €g events —re reg—rded —s "Elike eventsD sin™e a)

b)

pigure WX „ypi™—l s—mples of —A I ring eElike event —nd ˜A "Elike event a) 70 b) 120

60 100

50 80 40

60 30

40 20

20 10

0 0 -10 -8 -6 -4 -2 0 2 4 6 8 10 -30 -20 -10 0 10 20 30

PID parameter PID parameter

pigure IHX histri˜ution of the €sh p—r—meter for "Elike events @€sh`HA —nd

for eElikeevents @€shbHA in —A su˜Eqe† s—mple —nd in ˜A multiEqe† s—mpleF

„he ™losed ™ir™les —nd histogr—ms —re for the d—t— —nd for wonte g—rlo eventsD

resp e™tivelyF

WU7 of the €g events —re ™—used ˜y ™h—rged ™urrent # inter—™tionsF

"

„—˜le P shows the n—l results of two dierent energy regionsD n—mely su˜E

qe† —nd multiEqe†D —™™ording to the denition of sele™tion ™riteri— used in

u—miok—ndeF „he su˜Eqe† s—mple is the su˜set of pg events where IA i `

vis

IFQQ qe†D PA € b IHH we†G™ for eElike eventsD —nd QA € b PHH we†G™ for

e "

"Elike eventsF sn su˜Eqe† s—mpleD the num˜ers of single ring eElike —nd "Elike

events —re WVQ —nd WHHD resp e™tivelyD while the exp e™ted num˜ers using rond—9s

ux —re VIPFP —nd IPIVFQ for the single ring eElike —nd "Elike eventsD resp e™tivelyF

„he multiEqe† s—mple is the su˜set of pgevents with i ! IFQQ qe†F „he

vis

num˜er of single ring eElike —nd "Elike events —re PIV —nd IUTD resp e™tivelyD while

the exp e™ted num˜ers —re IVPFU —nd PPWFHF „he num˜er €g events is PHHD while

the exp e™ted num˜er is PRRFVF „hose num˜ ers —re summ—rized in „—˜F PF es

shown —˜ oveD ƒup erEu—miok—nde o˜served sm—ll dou˜le r—tios for ˜ oth the su˜E

CHXHPW

qe† —nd the multiEqe† energy s—mpleF „he dou˜le r—tio —re HFTII HFHRW

HXHPV

CHXHSW

—nd HFTTS HFHVI for the su˜Eqe† pg s—mple —nd ™om˜ined s—mple of multiE

HXHSR

qe† pg —nd €gD resp e™tivelyF y˜t—ined dou˜le r—tios in ƒup erEu—miok—nde —re

therefore in™onsistent with unityD —nd ™onsistent with the previous results of w—E

ter gerenkov exp erimentsF „husD the —tmospheri™ neutrino —nom—ly h—s ˜ een

est—˜lishedF

pigF II shows the momentum distri˜ution for the pg eventsF yne ™—n see th—t

the sh—p e of the distri˜utions for the eElike —nd "Elike events —re repro du™ed well

˜y the wonte g—rloF ‡e ™—n not determine whether # de™it or # ex™ess t—kes

" e

pl—™e due to PS 7 un™ert—inty in —˜solute norm—liz—tion ™oming from un™ert—inty

of neutrino ux —nd of neutrino inter—™tion ™ross se™tionsF „he de™it@ex™essA of

events in the muons @ele™tronsA of the d—t—D howeverD ™—n not ˜ e expl—ined within —

S 7 un™ert—inty of exp e™ted "ae r—tioF pigure IP shows the dou˜le r—tio vs

momentum in ˜ oth of the s—mplesF st —pp e—rs th—t the sm—ll dou˜le r—tio do es not

dep end strongly on the momentumF pigure IQ shows the dou˜le r—tio vs h D

w —ll

dist—n™e from the inner w—llF i—™h ˜in of h is ™hosen to give the s—me du™i—l

w —ll

m—ssF st is ™le—r th—t the dou˜le r—tio is not dep endent on the vertex p ositionF

„his proves the o˜t—ined sm—ll dou˜le r—tios —re not due to ™ont—min—tion from

—ny kind of in™oming p—rti™les like ™osmi™ r—y muons or neutrons from ro ™kF

„he higher energy neutrinos h—ve the ˜ etter —ngul—r ™orrel—tion to the lepton

pro du™ed vi— gg inter—™tionF por ex—mpleD the —ngle ˜ etween the neutrino —nd

the lepton is roughly PH degrees in multiEqe† s—mpleF „he dire™tion of neutrinos

™—n ˜ e me—sured ˜y using the dire™tion of — single ringF pigF IR shows the zenith

—ngle distri˜ution of "Elike events —nd eElike events in su˜Eqe† —nd multiEqe† C

€g s—mples together with wonte g—rlo exp e™t—tionsF e l—rge de™it of upw—rd

going neutrinos —re signi™—ntly o˜served in the multiEqe† "Elike s—mpleF xote

th—t —ny system—ti™ ee™ts due to the ™ross se™tion —nd neutrino ux ™—l™ul—tion

—re ™—n™eled in the symmetry of the zenith —ngle distri˜utionD —nd ™—nnot expl—in

the presented l—rge distortionF „he hypothesis of neutrino os™ill—tions ™—n n—tuE

r—lly expl—in this —symmetryF €relimin—ry os™ill—tion —n—lysis —ssuming # 3 #

" (

os™ill—tion h—s ˜ een m—deF „he WH 7 gFvF —llowed region is shown in pig VF elE

P

though the suggested region is slightly lower in m th—n th—t of u—miok—ndeD

Q P

the overl—p region with the u—miok—nde result —pp e—rs —t —round SIH e† F

R ‚esults in upw—rdEgoing muons

enother indi™—tion of neutrino os™ill—tions ™—n ˜ e derived from upw—rdEgoing

d—t—F „he upw—rdEgoing muons —re pro du™ed ˜y ™h—rged ™urrent # interE

"

—™tions in the ro ™k ne—r the dete™torF sf the energy of muons is l—rger th—n sever—l 200 a) 300 b)

175 250

150 200 125

100 150

75 100

50 50 25

0 0 0 200 400 600 800 1000 1200 1400 0 200 400 600 800 1000 1200 1400 MeV/c MeV/c

80 120 c) d) 70 100 60

80 50

40 60

30 40 20

20 10

0 0 100 1 10 100 110

GeV GeV

pigure IIX womentum distri˜ution for @—AeElike —nd @˜A"Elike events in the su˜E

qe† s—mple —nd ™A eElike —nd dA "Elike events in the wultiEqe† s—mple from

ƒup erEu—miok—ndeF „he histogr—ms show the wg predi™tionF 4 R 1.4 (a) (b) 3.5 1.2 3 1 2.5 0.8 2

0.6 1.5

0.4 1

0.2 0.5

0 0 0 500 1000 1500 1 10 100

momentum (MeV/c) momentum (GeV/c)

pigure IPX „he momentum dep enden™e of the dou˜le r—tio ‚ for —A su˜Eqe† —nd

˜A multiEqe†F „he ™losed ™ir™les show the d—t—F „he histogr—ms with dotted line

P

P

show the exp e™ted one with # 3 # os™ill—tion in the ™—se of @m Dsin P Aa

" (

Q

@S  IH DIFAF

2.5 2.5

2.25 a) 2.25 b)

2 2

1.75 1.75

1.5 1.5 R R 1.25 1.25

1 1

0.75 0.75

0.5 0.5

0.25 0.25

0 0 0 200 400 600 800 1000 1200 1400 1600 0 200 400 600 800 1000 1200 1400 1600 (cm) (cm)

Dwall Dwall

pigure IQX „he dou˜le r—tio ‚ in e—™h h ˜in for —A the su˜Eqe† —nd ˜A the

w —ll

multiEqe† s—mpleF „he Pm du™i—l volume ™uts —re —lso shownF 300 300 (a) (b)

200 200 Number of Events Number of Events

100 100

0 0 -1 -0.5 0 0.5 1 -1 -0.5 0 0.5 1

COS Θ COS Θ 200 200 (c) (d)

150 150

100 100 Number of Events Number of Events

50 50

0 0 -1 -0.5 0 0.5 1 -1 -0.5 0 0.5 1

COS Θ COS Θ

pigure IRX „he dou˜le r—tio ‚ —s — fun™tion of zenith —ngle for @—Asu˜Eqe† eElikeD

@˜A su˜Eqe† "ElikeD @™A multiEqe† eElikeD @dA multiEqe† "Elike eventsF ristogr—ms

with solid line show the exp e™t—tion from wonte g—rlo without os™ill—tionsF „he

h—t™hed ˜ oxes show the errors due to wonte g—rlo st—tisti™sF ristogr—m with

P

P

d—shed line show the exp e™t—tion with # 3 # os™ill—tion with @m Dsin P Aa

" e

Q

@S  IH DIFAF gos aI ™orresp onds to down going p—rti™lesF

qe†D they p—ss through the dete™torF „hese —re ™—lled upw—rdEgoingEthrough

muonsF „he typi™—l neutrino energy is the order of IHH qe† for upw—rdEgoingE

through muonsF

pw—rdEgoing through muons h—ve ˜ een sele™ted in QTP live d—ys d—t— s—mE

pleF ell the dire™tion —nd entering p osition of muons h—ve ˜ een re™onstru™ted

—utom—ti™—lly ˜y — progr—mD then l—ter ˜y m—nu—l tting to me—sure them more

pre™iselyF gosmi™ r—y muonsD whi™h —re the m—in ˜—™kground eventsD h—ve ˜ een

e—sily reje™ted ˜y —pplying the zenith —ngle ™ut @ ™os  H AF „he p—th length

z

of the muon tr—™k in the inner dete™tor h—s ˜ een required to ˜ e more th—n U mF

„his ™orresp onds to — IFU qe† ™utF „he tot—l o˜served num˜er of upw—rdEgoingE

through muons is RHW in QTP live d—ysF „he exp e™ted num˜er of upw—rdEgoing

through muons from — ™—l™ul—tion is RRS  VWF st is h—rd to ™omp—re the o˜t—ined

num˜er of upgoing muons to the exp e™ted one sin™e —˜solute num˜er h—s —˜ out

PH 7 un™ert—inty due to the ux of —tmospheri™ neutrinos —nd the ™ross se™tionF

roweverD p ossi˜le distortion of zenith —ngle distri˜ution is free from su™h systemE

—ti™sD —nd ™ould ˜ e eviden™e of neutrino os™ill—tions just —s in the vertexE™ont—ined

event d—t—F

pigure IS shows the zenith —ngle distri˜ution o˜t—ined from u—miok—nde —nd

from ƒup erEu—miok—nde together with the exp e™t—tionF „he ™losed ™ir™les —nd

op en ™ir™les show the d—t— of u—miok—nde —nd of ƒup erEu—miok—ndeD resp e™E

tivelyF „hose d—t— of two exp eriments —gree wellF „he exp e™ted distri˜utions in

P

P Q

the ™—se of no os™ill—tion —nd the os™ill—tion with @m Dsin P Aa@S IH DIFAF

for ˜ oth exp eriments —re —lso shown with thin solid lines —nd with thin d—shed

linesD resp e™tivelyF „hose plotted histogr—ms —re ˜ estEtted ones within PH 7 unE

™ert—inty in —˜solute norm—liz—tionF „he d—t— of two exp eriments —re ™onsistent

with e—™h exp e™t—tion with no os™ill—tion with in errorsD though the st—tisti™s is

not enough so f—rF roweverD it is interesting th—t the hypothesis of # 3 # osE

" x

P

™ill—tion with the p—r—meter suggested ˜y the ™ont—ined d—t—D for ex—mple @m D

P

Q P

sin P Aa@S  IH e† DIFAD —grees well with the d—t—D orD even ts ˜ etterF epE

p—rently mu™h more st—tisti™s —nd further study of system—ti™ error —re needed to

give — de™isive —nswer for neutrino os™ill—tionsF

pigure ISX „he zenith —ngle distri˜ution of upw—rd going through muons from

u—miok—nde @full ™ir™leA —nd ƒup erEu—miok—nde @op en ™ir™leAF ristogr—ms show

the exp e™ted distri˜utions from no os™ill—tion @thi™k solid —nd d—shed lines for

ƒup erEu—miok—nde —nd u—miok—ndeD resp e™tivelyA —nd from # # os™ill—tion

" (

P

P Q P

with m aS IH e† —nd sin P a I @thin solid —nd d—shed lines for ƒup erE

u—miok—nde —nd u—miok—ndeD resp e™tivelyAF „he results —nd exp e™ted lines for

u—miok—nde were multiplied ˜y — f—™tor HFVIW to s™—le its geometri™—l ee™t to

ƒup erEu—miok—ndeF „he exp e™ted lines —re the ˜ est tted ones o˜t—ined within

the —˜solute s™—le un™ert—inty of PH7F

RFI puture longE˜—seline exp eriment —t uiu

„he ee™t of neutrino os™ill—tion suggested ˜y the —tmospheri™ neutrino d—t— ™—n

˜ e studied ˜y longE˜—seline neutrino os™ill—tion exp eriments using high intensity

# ˜ e—mF yne of the p ossi˜le exp eriment is the one ˜ etween uiuE€ƒ —nd ƒup erE

"

PI

u—miok—nde @™—lled uPuAF st h—s the ˜—seline length of PSH km —nd the —ver—ge

P P

energy of # ˜ e—m is roughly IFS qe† so th—t it is just sensitive to the m $ IH

"

P

e† region suggested ˜y the ƒup erEu—miok—nde d—t—F

„he IP qe† proton ˜ e—m is extr—™ted from uiuE€ƒ within I "se™ ˜y every

C

P se™ondsF % 9s pro du™ed ˜y IP qe† protons —re fo ™used ˜y horn m—gnets —nd

C

de™—y into " # in the PHH m long de™—y tunnelF „he fr—™tion of # in the ˜ e—m

" e

is less th—n I 7F „here —re two kind of ˜ e—m monitorsD the % monitor —nd the

" monitorD in the de™—y tunnelF „he % monitor downstre—m the horn m—gnets is

— g—s gerenkov dete™tor whi™h me—sures the emission —ngle of gerenkov photons

pro du™ed ˜y the % ˜ e—m with v—rious g—s pressureF „his monitor provides the

inform—tion —˜ out distri˜ution of momentum —nd divergen™e of % ˜ e—mF „he

" monitor downstre—m the ˜ e—m dump me—sures the prole of "9s from the %

de™—ysF „hose two monitors —re useful to underst—nd pro du™tion of # ˜ e—mF

"

„here is — front dete™tor QHH m —p—rt from the t—rget to me—sure initi—l ux of

# ˜ e—mF „he front dete™tor ™onsists of the pine qr—in hete™tor —nd IHHH ton w—E

"

ter gerenkov dete™torF „he pine qr—in hete™tor is — tr—™kingEtype dete™tor whi™h

™onsists of — ’s—ndwi™h4 of s™intill—ting ˜ er tr—™ker —nd w—ter l—yer —s — t—rgetF

„he —im of the dete™tor is to me—sure the —˜solute # ux with S 7 —™™ur—™y ˜y

"

™hoosing qu—siEel—sti™ gg inter—™tionF „he IHHH ton w—ter gerenkov dete™tor h—s

the s—me ™ongur—tion —s ƒup erEu—miok—ndeF „he —im of the dete™tor is to study

the dete™tor resp onse whi™h is ™h—r—™teristi™ for w—ter gerenkov te™hnique with

neutrino ˜ e—m wellEme—sured ˜y the pine qr—in hete™torF

„he num˜er of ™h—rged ™urrent inter—™tions —t ƒup erEu—miok—nde is —˜ out

PH

QSH for IH protons on t—rget @€y„A in twoye—rs of runningF „his exp eriment

™—n se—r™h for # 3 # —nd # 3 # indep endentlyF # 3 # os™ill—tion ™—n

" e " ( " e

˜ e o˜served —s —n —pp e—r—n™e of eElike events —t ƒup erEu—miok—ndeF # 3 #

" (

os™ill—tion ™—n ˜ e o˜served —s p ossi˜le distortion of # energy sp e™trum whi™h

"

™—n ˜ e re™onstru™ted from single ring "Elikeevents —t ƒup erEu—miok—ndeF pigE

ure IT shows re™onstru™ted energy sp e™trum of # 9s with noEos™ill—tion —nd with

" os™ill—tionF yne ™—n see the signi™—nt distortion in the sp e™trum in the ™—se of a) b)

c) d)

pigure ITX „he exp e™ted energy distri˜ution of # —t ƒup erEu—miok—nde re™onE

"

stru™ted from single ring "Elike eventsF „he histogr—ms show the d—t— without

os™ill—tionF „he ™rosses shows the d—t— in the ™—se of # # os™ill—tion with

" (

P

P P P P Q P

sin P a I —nd —A with m aIH e† D ˜A with m aS IH e† D ™A with

P Q P P Q P

m aQ IH e† D dA with m aP IH e† F 0

)) 10 2 (eV 2 m

∆ -1 99% C.L.

10 90% C.L. log( σ 3

-2 10

-3 10

-4 10 0 0.2 0.4 0.6 0.8 1 2

sin 2θ

P

P

pigure IUX „he sensitivity plot in @m Dsin P A sp—™e for # dis—pp e—r—n™e se—r™h

"

PH

with IH €y„ ˜y using the neutrino energy sp e™trum —n—lysisF i—™h ™ontour —t

WH 7 gFvFDWW 7 gFvF —nd Q ' level is shownF elso shown —re the —llowed region

from u—miok—nde —nd ƒup erEu—miok—nde resultsF

P

os™ill—tion with m suggested ˜y —tmospheri™ neutrino d—t—F „he sensitivity for

P

the # dis—pp e—r—n™e me—surement is plotted in pigure IUF „he region where m

"

P

Q P

is gre—ter th—n Q  IH e† —nd sin P is gre—ter th—n HFT ™—n ˜ e explored ˜y

this exp erimentF

„he ™onstru™tion of the new neutrino ˜ e—mline h—s ˜ een st—rted in IWWTF „he

inst—ll—tion of the front dete™tor will ˜ e st—rted from yg„D IWWVF „he rst neuE

trino ˜ e—m will ˜ e extr—™ted from t—nDIWWWF „he physi™s run will ˜ e st—rted eprD

IWWW —nd ™ontinues for P$Q ye—rsF st will give — ™on™lusive result for the os™ill—tion

p—r—meter —nd mo desF

S gon™lusion

ƒup erEu—miok—nde is the l—rgest underground w—ter gerenkov dete™tor dedi™—ted

to the dete™tion of neutrinos —nd proton de™—ysF ƒup erEu—miok—nde h—s ˜ een

™ontinuously running from epril ID IWWT —nd ™olle™ts mu™h gre—ter st—tisti™s of

neutrino d—t— th—n h—s ˜ een —™hieved so f—r ˜y —ny underground neutrino exp erE

imentF

„he prelimin—ry results in sol—r neutrino —re rep orted ˜—sed on QUR liveEd—ys

d—t—F „he o˜served ux of sol—r neutrinos is —pp—rently sm—ller th—n the exp e™t—E

tion of ƒƒwD —nd ™onsistent to the previous result of u—miok—ndeF „he h—yGxight

dieren™e is ™onsistent to zero within errorF „his result p—rti—lly ex™ludes the lower

P

m region in the l—rgeE—ngle solution of wƒ‡F „he o˜served energy sp e™trum

of d—t—Gƒƒw is not signi™—ntly distorted with ™urrent errors though — t with —

P

distorted sp e™trum gives ˜ etter 1 th—n ™omp—rison to the undistorted sh—p eF

„he prelimin—ry results in —tmospheri™ neutrinos —re presented ˜—sed on RIR

liveEd—ys d—t—F „he dou˜le r—tios —re me—sured ˜ oth in the su˜Eqe† s—mple —nd

the multiEqe† s—mpleF foth —re —pp—rently sm—ller th—n unity —nd ™onsistent

with the previous u—miok—nde resultF woreoverD — l—rge de™it of upgoing # is

"

o˜served in multiEqe† s—mpleF „hose —nom—lies —re h—rd to expl—in ˜y st—nd—rd

physi™s —nd ™ould ˜ e eviden™e of neutrino os™ill—tionsF „he prelimin—ry results

in upw—rdEgoingEthrough muons ˜—sed on QTP d—ys d—t— —re —lso rep ortedF „he

o˜served zenith —ngle distri˜ution is still ™onsistent with the exp e™t—tion within

errorsF roweverD it is —lso ™onsistent with # 3 # os™ill—tion with the p—r—meters

" x

suggested ˜y the —tmospheri™ resultF wu™h more st—tisti™s —re needed to give— de™isive —nswer for neutrino os™ill—tionsF

„he p—r—meter region suggested ˜y —tmospheri™ neutrino result will ˜ e exE

plored ˜y the long ˜—seline exp eriment using — high intensity # ˜ e—m from uiuE

"

€ƒ st—rting in IWWWF ‡e m—y ™onrm # 3 # os™ill—tions ˜y dete™ting — p ossi˜le

" x

distortion of the # energy sp e™trum —t ƒup erEu—miok—ndeF st is ex™iting th—t osE

"

P

P Q

™ill—tions with the p—r—meters @m Dsin P A$ @S  IH DIAD whi™h —re —llowed ˜y

˜ oth the u—miok—nde —nd the ƒup erEu—miok—nde —tmospheri™ neutrino resultsD

™—use l—rge distortion of the # energy sp e™trumF rop efullyDwem—y determine

"

the mo de —nd p—r—meter of neutrino os™ill—tions —nd op en — new eld of neutrino

physi™sF

‚eferen™es

‘I“ „he ƒup erEu—miok—nde ™oll—˜ or—tionD snstitute for gosmi™ ‚—y ‚ese—r™h

@sg‚‚AD niversityof„okyoD qifu niversityD x—tion—l v—˜ or—tory for righ

inergy €hysi™s @uiuAD uo˜ e niversityD wiy—gi niversity of idu™—tionD xiE

ig—t— niversityD ys—k— niversityD„ok—i niversityD„okyo snstitute of „e™hE

nologyD„ohoku niversityD foston niversityD fro okh—ven x—tion—l v—˜ or—E

toryD niversity of g—liforni—D srvineD g—liforni— ƒt—te niversityD hominguez

rillsD qeorge w—son niversityD niversityofr—w—iiD vos el—mos x—tion—l

v—˜ or—toryD vouisi—n— ƒt—te niversityD niversity of w—ryl—ndD ƒt—te niE

versity of xew ‰ork —t ƒtony fro okD niversityof‡—rs—wD niversityof

‡—shingtonF

‘P“ ƒeeD for ex—mpleD tFxFf—h™—ll —nd wFrF€insonne—ultD ‚evF wo dF €hysF TU

@IWWSA UVIF

‘Q“ uFv—ndeD to ˜ e pu˜lished in x eutr ino WTD €ro ™eedings of the IUth sntern—E

tion—l gonferen™e on xeutrino €hysi™s —nd estrophysi™sD relsinkiD pinl—ndD

tune IWWTF ƒee —lso fF„Fglevel—nd et —lFD xu™lF €hysF f @€ro ™F ƒupplFA QV

@IWWSA RUF

‘R“ ‰Fpukud— et —lFD €hysF ‚evF vettF UU @IWWTA ITVQF

‘S“ tFxFe˜ dur—shitov et —lFD €hysF ‚evF vettF UU @IWWTA RUHVF

‘T“ ‡Fr—mp el et —lFD €hysF vettF f QVV @IWWTA QVRF

‘U“ „he ƒup erEu—miok—nde ™oll—˜ or—tionD dr—ft in prep—r—tionF

‘V“ ƒeeD for ex—mpleD xFr—t— —nd €Fv—ng—™kerD €reprint veƒƒxƒEeƒ„ WUGPW

@w—yIWWUAD —nd referen™es thereinF

‘W“ ƒF€Fwikheyev —nd eF‰uFƒmirnovD ƒovF tF xu™lF €hysF RP @IWVSA WIQY

vF‡olfensteinD €hysF ‚evF h IU @IWUVA PQTWY i˜idF PH @IWUWA PTQRF

‘IH“ fe™kerEƒzendy et —lFD €hysF ‚evF h RT @IWWPA QUPHF

‘II“ ‚Fgl—rk et —lFD to ˜ e pu˜lished in €hys ‚evF vettF ‚Fgl—rkD priv—te ™ommuE

ni™—tion for the @"aeA a@"aeA v—lueF

d—t— wg

‘IP“ ‰Fpukud— et —lFD €hysF vettF f QQS @IWWRA PQUF

‘IQ“ wFegliett— et —lFD iurophysF vettF VD @IWVWA TIIF

‘IR“ uFh—um et —lFD F €hysF g TT @IWWSA RIUF

‘IS“ ‡F‡FwFellison et —lFD €hysF vettF f QWI @IWWUA RWIF wFgFqo o dm—nnD for

the ƒoud—nEP ™oll—˜ or—tionD t—lk presented —t ƒixth gonferen™e on the snterE

se™tions of €—rti™le —nd xu™le—r €hysi™sD wont—n—D ƒeD w—yEtuneD IWWUF

‘IT“ fF e™hk—r et—lFD xu™lF €hysF f RQR @IWWSASHQF

‘IU“ qF ƒF †idy—kin et—lFD ƒovF €hysF ti„€ UID RPR @IWWHAY ti„€ vettF SWD QWH

@IWWRAF

‘IV“ gho oz ™oll—˜ or—tionD preprint hepEexGWUIIHHHP @S xov IWWUA

‘IW“ ‡F pr—ti et—lFD €hysF ‚evF h RV @IWWQA IIRHF

‘PH“ ‚F fe™kerEƒzendy et—lFD €hysF ‚evF vettF TW @IWWPA IHIHF

‘PI“ uFxishik—w— sxƒE‚epFEWPRD @IWWPAF