andard - kek · neutrino beams s tef ano f or te u niversit ... ost-lhc construction windo w ma y...

65
TESTS OF THE STANDARD MODEL WITH NEUTRINO BEAMS STEFANO FORTE UNIVERSIT ` A DI MILANO J-PARC WORKSHOP KEK, TSUKUBA,NOVEMBER 30, 2005

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Page 1: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

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NO

J-PA

RC

WO

RK

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K,T

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KU

BA,N

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EM

BE

R30,2005

Page 2: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

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Page 3: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

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EU

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ET!..

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0.9

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Page 4: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

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INO

BE

AM

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EU

TR

INO

SIN

TE

RA

CT

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AK

LY.

..D

ISX-S

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T.:

σW σγ∼

GFQ

2

8πα

M2 W

Q2+M

2 W

≈5·1

0−

5Q

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eV2

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2 W)

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ED

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IGTA

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OR

US

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Kg

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18

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6D

ISE

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NTS/Y

R

=20÷

400

GeV

NM

C:

5K

g,∼

0.9

m3,∼

106

EV/Y

R

Page 5: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

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Page 6: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

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Page 7: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p
Page 8: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

TH

ES

UPE

RB

EA

M&β

BE

AM

:

Bet

aB

eam

(P.Z

ucch

elli:

Phy

s.Le

tt.B

532:

166,

2002

)

M.L

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aB

eam

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illar

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epte

mbe

r24

2004

.9

Page 9: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

TH

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EA

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AM

:

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aB

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ucch

elli:

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s.Le

tt.B

532:

166,

2002

)

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indr

oos

etal

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epte

mbe

r24

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Page 10: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

FLU

XE

SA

ND

SPE

CTR

A:

FR

OM

LOW

EN

ER

GY.

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Flux

es

0

500

1000

1500

2000

2500

3000

3500

4000

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x 10

7 00.

20.

40.

60.

81

Eν (G

eV)

ν/m2/20 meV

SPL

νµ

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Bet

aν−

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Bet

e (N

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CC

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0

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81

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eV)

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10.

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=60

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Page 11: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

...T

OH

IGH

EN

ER

GY

FLU

XE

S

β=

100

3He

Fre

jus Eν (

GeV

)

ν/m2/20 MeV/yr

0

1000

2000

3000

4000

5000

6000

7000

8000

x 1

07

00.2

0.4

0.6

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1

SP

L ν

µ

SP

L ν−

µ

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a

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e6)

Bet

a ν

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e18)

β=

350

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11.

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dΦ�dEΝHm-2GeV-1yr-1L

Γ He=

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Γ Ne=

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Nu

Fact

front-

end

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MPA

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fluxes

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tance

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6−

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ith

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r

Page 12: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

WH

YN

EU

TR

INO

S?:

TH

EY

PR

OB

EE

LEC

TR

OW

EA

KC

OU

PLI

NG

S...

elas

ticν

-fer

mio

nsc

atte

rin

g

dσ dy

(νf→νf

)=G

2 FQ

2

πy

[ g2 L

+g

2 R(1−y)2] ;

Q2≡−

(kν−k′ ν)

2,

y≡

pf·qν

pf·kν

...S

PIN

...

RE

AC

TIO

Ng L

g R

νµe−→νµe−

(NC

)−

1 2+

sin

2θ W

sin

2θ W

νµe−→µ−νe

(CC

)1

0

νu→νu

(NC

)1 2−

2 3si

n2θ W

2 3si

n2θ W

νd→νd

(NC

)−

1 2+

1 3si

n2θ W

1 3si

n2θ W

νed→e−u

(CC

)1

0

AN

DF

LAV

OU

R!

Page 13: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

WH

YN

EU

TR

INO

S?:

TH

EY

PR

OB

EE

LEC

TR

OW

EA

KC

OU

PLI

NG

S...

elas

ticν

-fer

mio

nsc

atte

rin

g

dσ dy

(νf→νf

)=G

2 FQ

2

πy

[ g2 L

+g

2 R(1−y)2] ;

Q2≡−

(kν−k′ ν)

2,

y≡

pf·qν

pf·kν

...S

PIN

...

RE

AC

TIO

Ng L

g R

νµe−→νµe−

(NC

)−

1 2+

sin

2θ W

sin

2θ W

νµe−→µ−νe

(CC

)1

0

νu→νu

(NC

)1 2−

2 3si

n2θ W

2 3si

n2θ W

νd→νd

(NC

)−

1 2+

1 3si

n2θ W

1 3si

n2θ W

νed→e−u

(CC

)1

0

AN

DF

LAV

OU

R!

Page 14: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

WH

YN

EU

TR

INO

S?:

TH

EY

PR

OB

EE

LEC

TR

OW

EA

KC

OU

PLI

NG

S...

elas

ticν

-fer

mio

nsc

atte

rin

g

dσ dy

(νf→νf

)=G

2 FQ

2

πy

[ g2 L

+g

2 R(1−y)2] ;

Q2≡−

(kν−k′ ν)

2,

y≡

pf·qν

pf·kν

...S

PIN

...

RE

AC

TIO

Ng L

g R

νµe−→νµe−

(NC

)−

1 2+

sin

2θ W

sin

2θ W

νµe−→µ−νe

(CC

)1

0

νu→νu

(NC

)1 2−

2 3si

n2θ W

2 3si

n2θ W

νd→νd

(NC

)−

1 2+

1 3si

n2θ W

1 3si

n2θ W

νed→e−u

(CC

)1

0

AN

DF

LAV

OU

R!

Page 15: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

WH

YN

EU

TR

INO

S?:

TH

EY

PR

OB

EE

LEC

TR

OW

EA

KC

OU

PLI

NG

S...

elas

ticν

-fer

mio

nsc

atte

rin

g

dσ dy

(νf→νf

)=G

2 FQ

2

πy

[ g2 L

+g

2 R(1−y)2] ;

Q2≡−

(kν−k′ ν)

2,

y≡

pf·qν

pf·kν

...S

PIN

...

RE

AC

TIO

Ng L

g R

νµe−→νµe−

(NC

)−

1 2+

sin

2θ W

sin

2θ W

νµe−→µ−νe

(CC

)1

0

νu→νu

(NC

)1 2−

2 3si

n2θ W

2 3si

n2θ W

νd→νd

(NC

)−

1 2+

1 3si

n2θ W

1 3si

n2θ W

νed→e−u

(CC

)1

0

AN

DF

LAV

OU

R!

Page 16: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

NE

UTR

INO

-HA

DR

ON

INTE

RA

CTIO

NS

DE

EP-I

NE

LAS

TIC

SC

ATTE

RIN

G:.

..

−Q

2

p

γ∗ ,W∗ ,Z∗

X

Lep

ton

fract

ional

ener

gy

loss

:y

=p·qp·k

;

Bjo

rken

x:x

=Q

2

2p·q

lepto

n-n

ucl

eon

CM

ener

gy:s

=Q

2

xy

;

vir

tual

boso

n-n

ucl

eon

CM

ener

gyW

2=Q

21−xx

;

d2σλpλ`(x,y,Q

2)

dxdy

=G

2 F

(1+Q

2/m

2 W)2Q

2

xy

{[ −

λ`y

( 1−y 2

) xF

3(x,Q

2)

+(1−y)F

2(x,Q

2)

+y

2xF

1(x,Q

2)]−

2λp

[ −λ`y(2−y)xg1(x,Q

2)−

(1−y)g

4(x,Q

2)−y

2xg5(x,Q

2)]}

λl→

lepto

nhel

icit

y

λp→

pro

ton

hel

icit

y

PA

RIT

YC

ON

S.

PA

RIT

YV

IOL.

UN

PO

L.F

1,F

2F

3

PO

L.g1

g4,g5

Page 17: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

PA

RTO

ND

ISTR

IBU

TIO

NS

STR

UC

TU

RE

FU

NC

TIO

N=H

AR

DC

OE

FF.⊗

PA

RTO

ND

ISTN.

FN

C2

(x,Q

2)

=x∑ flav.i

e2 i(qi

+q i

)+αs

[Ci[αs]⊗

(qi

+q i

)+Cg[αs]⊗g]

q iqu

ark

,q i

anti

qu

ark

,g

glu

on

LEA

DIN

GP

AR

TO

NC

ON

TE

NT

(up

toO

[αs]

corr

ecti

ons)

q i≡q↑↑i

+q↑↓i

∆q i≡q↑↑i−q↑↓i

NC

F1γ,Z

=∑

ie2 i

(qi

+q i

)g 1γ,Z

=∑

ie2 i

(∆q i

+∆q i

)

CC

FW

+

1=u

+d

+s

+c

gW

+

1=

∆u

+∆d

+∆s

+∆c

CC

−FW

+

3/2

=u−d−s

+c

gW

+

5=

∆u−

∆d−

∆s

+∆c

F2

=2xF

1g 4

=2xg 5

W+→

W−⇒

u↔d,c↔s;

more

com

bin

ati

on

su

sin

gIs

osp

in:p→n⇒

u↔d

Page 18: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

ELA

STIC

&Q

UA

SI-

ELA

STIC

SC

ATTE

RIN

GPO

INTLI

KE

CR

OS

SS

EC

TIO

NS

CO

RR

EC

TE

DB

YFO

RM

FA

CTO

RS:

neg

lect

ing

term

sO

(Mn/E

),fo

rth

ee.

m.

curr

ent

〈p′ |jµ|p〉=

u(p′ )γµu

(p)G

M(Q

2)

+u

(p′ )u

(p)( p

µ+p′µ

2m

) GE

(Q2);

axia

lcu

rren

t⇒

GA

;d

efin

ean

alo

gou

sly

stra

nge

form

fact

ors

from

stra

nge

curr

ent

[ dσ

dy

NC

ν

+dσ

dy

NC

ν

] p

=G

2 FMnEν

1 4

[ 2(1−y

+y

2)][ (G

A−Gs A

)2+( G

p M(1−

4si

n2θW

)−Gn M−Gs M

) 2]

[ dσ

dy

NC

ν

−dσ

dy

NC

ν

] p

=G

2 FMnEν

1 2(2−y)[ G

p M(1−

4si

n2θW

)−Gn M−Gs M

] (GA

+Gs A

)

[ dσ

dy

NC

ν

+dσ

dy

NC

ν

] n

=G

2 FMnEν

14[ 2

(1−y

+y

2)][ (G

A+Gs A

)2+( G

n M(1−

4si

n2θW

)−Gp M−Gs M

) 2]

[ dσ

dy

NC

ν

−dσ

dy

NC

ν

] n

=G

2 FMnEν

−1 2

(2−y)[ G

n M(1−

4si

n2θW

)−Gp M−Gs M

] (GA

+Gs A

)

[ dσ

dy

CC

ν

+dσ

dy

CC

ν

]=

G2 FMnEν

[ 2(1−y

+y

2)][ G

2 A−

(Gp M−Gn M

)2]

[ dσ

dy

CC

ν

−dσ

dy

CC

ν

]=

G2 FMnEν

2(2−y)(Gp M−Gn M

)GA

M→

nu

cleo

nm

ass

;fo

rmfa

ctors

dep

end

onQ

2=

2Mn(E

n−Mn)

(nu

cl.

rest

fram

e)

NO

TE

NO

DE

P.O

NGE

,E

NTE

RS

TH

RO

UG

HO

(Mn/E

)TE

RM

S

Page 19: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

AN

EX

AM

PLE

....

Page 20: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

TH

EN

UT

EV

AN

OM

ALY

PW

RA

TIO

:D

ATA...

Nu

TeV

2001

sin

2θ W

(OS

)=

0.22

72±

0.00

13(s

tat)±

0.00

09(s

yst

0.00

02(M

t,M

H)

Glo

bal

Fit

2003

sin

2θ W

(OS

)=

0.22

29±

0.00

04

...V

S.

TH

EO

RY

R−

=σNC

(ν)−σNC

(ν)

σCC

(ν)−σCC

(ν)

=( 1 2−

sin

2θ W

)

+2

[ (u−u

)−

(d−d)

u−u

+d−d−

s−s

u−u

+d−d

] ×[ (

1 2−

7 6si

n2θ W

)

+4 9

αs

( 1 2−

sin

2θ W

)+O

(α2 s)]

+O

(δ(u−d)2,δs

2)

U,D

...D

EN

OTE

MO

ME

NTU

MF

RA

CTIO

NS

CA

RR

IED

BY

CO

RR

ES

P.Q

UA

RK

FLA

VO

RS

•IS

OS

PIN

VIO

LATIO

N→

corr

n.

for

non

-iso

scala

rta

rget

incl

ud

ed,

bu

tn

otup6=dn

•S

TR

AN

GE

AS

YM

.→

stra

ngen

ess

mu

stva

nis

h,

bu

tn

ot

vale

nce

mom

.fr

act

.!

•Q

CD

CO

RR

EC

TIO

NS→

tiny

(on

lyen

ter

thro

ugh

sym

.vio

lati

ng

term

s)

s−s≈

0.0

04

(OR

2%

ISO

SPIN

VLN

.)E

NO

UG

HTO

RE

MO

VE

AN

OM

ALY:

CA

NW

ETE

ST

IT?

Page 21: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

TH

EN

UT

EV

AN

OM

ALY

PW

RA

TIO

:D

ATA...

Nu

TeV

2001

sin

2θ W

(OS

)=

0.22

72±

0.00

13(s

tat)±

0.00

09(s

yst

0.00

02(M

t,M

H)

Glo

bal

Fit

2003

sin

2θ W

(OS

)=

0.22

29±

0.00

04

...V

S.

TH

EO

RY

R−

=σNC

(ν)−σNC

(ν)

σCC

(ν)−σCC

(ν)

=( 1 2−

sin

2θ W

)+

2

[ (u−u

)−

(d−d)

u−u

+d−d

−s−s

u−u

+d−d

] ×

[

( 1 2−

7 6si

n2θ W

)

+4 9

αs

( 1 2−

sin

2θ W

)+O

(α2 s)]

+O

(δ(u−d)2

,δs

2

)

U,D

...D

EN

OTE

MO

ME

NTU

MF

RA

CTIO

NS

CA

RR

IED

BY

CO

RR

ES

P.Q

UA

RK

FLA

VO

RS

•IS

OS

PIN

VIO

LATIO

N→

corr

n.

for

non

-iso

scala

rta

rget

incl

ud

ed,

bu

tn

otup6=dn

•S

TR

AN

GE

AS

YM

.→

stra

ngen

ess

mu

stva

nis

h,

bu

tn

ot

vale

nce

mom

.fr

act

.!

•Q

CD

CO

RR

EC

TIO

NS→

tiny

(on

lyen

ter

thro

ugh

sym

.vio

lati

ng

term

s)

s−s≈

0.0

04

(OR

2%

ISO

SPIN

VLN

.)E

NO

UG

HTO

RE

MO

VE

AN

OM

ALY:

CA

NW

ETE

ST

IT?

Page 22: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

TH

EN

UT

EV

AN

OM

ALY

PW

RA

TIO

:D

ATA...

Nu

TeV

2001

sin

2θ W

(OS

)=

0.22

72±

0.00

13(s

tat)±

0.00

09(s

yst

0.00

02(M

t,M

H)

Glo

bal

Fit

2003

sin

2θ W

(OS

)=

0.22

29±

0.00

04

...V

S.

TH

EO

RY

R−

=σNC

(ν)−σNC

(ν)

σCC

(ν)−σCC

(ν)

=( 1 2−

sin

2θ W

)+

2

[ (u−u

)−

(d−d)

u−u

+d−d−

s−s

u−u

+d−d

] ×

[

( 1 2−

7 6si

n2θ W

)

+4 9

αs

( 1 2−

sin

2θ W

)+O

(α2 s)]

+O

(δ(u−d)2,δs

2)

U,D

...D

EN

OTE

MO

ME

NTU

MF

RA

CTIO

NS

CA

RR

IED

BY

CO

RR

ES

P.Q

UA

RK

FLA

VO

RS

•IS

OS

PIN

VIO

LATIO

N→

corr

n.

for

non

-iso

scala

rta

rget

incl

ud

ed,

bu

tn

otup6=dn

•S

TR

AN

GE

AS

YM

.→

stra

ngen

ess

mu

stva

nis

h,

bu

tn

ot

vale

nce

mom

.fr

act

.!

•Q

CD

CO

RR

EC

TIO

NS→

tiny

(on

lyen

ter

thro

ugh

sym

.vio

lati

ng

term

s)

s−s≈

0.0

04

(OR

2%

ISO

SPIN

VLN

.)E

NO

UG

HTO

RE

MO

VE

AN

OM

ALY:

CA

NW

ETE

ST

IT?

Page 23: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

TH

EN

UT

EV

AN

OM

ALY

PW

RA

TIO

:D

ATA...

Nu

TeV

2001

sin

2θ W

(OS

)=

0.22

72±

0.00

13(s

tat)±

0.00

09(s

yst

0.00

02(M

t,M

H)

Glo

bal

Fit

2003

sin

2θ W

(OS

)=

0.22

29±

0.00

04

...V

S.

TH

EO

RY

R−

=σNC

(ν)−σNC

(ν)

σCC

(ν)−σCC

(ν)

=( 1 2−

sin

2θ W

)+

2

[ (u−u

)−

(d−d)

u−u

+d−d−

s−s

u−u

+d−d

] ×[ (

1 2−

7 6si

n2θ W

)

+4 9

αs

( 1 2−

sin

2θ W

)+O

(α2 s)]

+O

(δ(u−d)2,δs

2)

U,D

...D

EN

OTE

MO

ME

NTU

MF

RA

CTIO

NS

CA

RR

IED

BY

CO

RR

ES

P.Q

UA

RK

FLA

VO

RS

•IS

OS

PIN

VIO

LATIO

N→

corr

n.

for

non

-iso

scala

rta

rget

incl

ud

ed,

bu

tn

otup6=dn

•S

TR

AN

GE

AS

YM

.→

stra

ngen

ess

mu

stva

nis

h,

bu

tn

ot

vale

nce

mom

.fr

act

.!

•Q

CD

CO

RR

EC

TIO

NS→

tiny

(on

lyen

ter

thro

ugh

sym

.vio

lati

ng

term

s)

s−s≈

0.0

04

(OR

2%

ISO

SPIN

VLN

.)E

NO

UG

HTO

RE

MO

VE

AN

OM

ALY:

CA

NW

ETE

ST

IT?

Page 24: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

TH

EN

UT

EV

AN

OM

ALY

PW

RA

TIO

:D

ATA...

Nu

TeV

2001

sin

2θ W

(OS

)=

0.22

72±

0.00

13(s

tat)±

0.00

09(s

yst

0.00

02(M

t,M

H)

Glo

bal

Fit

2003

sin

2θ W

(OS

)=

0.22

29±

0.00

04

...V

S.

TH

EO

RY

R−

=σNC

(ν)−σNC

(ν)

σCC

(ν)−σCC

(ν)

=( 1 2−

sin

2θ W

)+

2

[ (u−u

)−

(d−d)

u−u

+d−d−

s−s

u−u

+d−d

] ×[ (

1 2−

7 6si

n2θ W

)

+4 9

αs

( 1 2−

sin

2θ W

)+O

(α2 s)]

+O

(δ(u−d)2,δs

2)

U,D

...D

EN

OTE

MO

ME

NTU

MF

RA

CTIO

NS

CA

RR

IED

BY

CO

RR

ES

P.Q

UA

RK

FLA

VO

RS

•IS

OS

PIN

VIO

LATIO

N→

corr

n.

for

non

-iso

scala

rta

rget

incl

ud

ed,

bu

tn

otup6=dn

•S

TR

AN

GE

AS

YM

.→

stra

ngen

ess

mu

stva

nis

h,

bu

tn

ot

vale

nce

mom

.fr

act

.!

•Q

CD

CO

RR

EC

TIO

NS→

tiny

(on

lyen

ter

thro

ugh

sym

.vio

lati

ng

term

s)

s−s≈

0.0

04

(OR

2%

ISO

SPIN

VLN

.)E

NO

UG

HTO

RE

MO

VE

AN

OM

ALY:

CA

NW

ETE

ST

IT?

Page 25: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

DIS

EN

TA

NG

LIN

GS

TR

AN

GE

NE

SS

CH

AR

MIS

CO

PIO

US

LY

PR

OD

UC

ED

INW

++s→c

easi

lyta

gged

thro

ugh

dim

uon

sign

al,

2nd

mu

onfr

omsu

bse

qu

entc

dec

ay

⇒A

CC

UR

ATE

EX

TR

AC

TIO

NO

FTH

ES

TR

AN

GE

DIS

TR

IBU

TIO

N

-0.0

020

0.00

2

0.00

4

0.00

6

0.00

8

0.01

00.

20.

40.

60.

8a)Q2 =2

0GeV

2

x

xs-xs-

0

0.51

1.52

2.53

3.54

4.55

0.2

0.4

0.6

b) x

s/s-

CC

FR

fit2

BPZ

NuT

eV

x(s−

s)s(

x)/s

(x)

−−

NuT

eVBPZ

CC

FR

/NUT

EVs−s

DE

TE

RM

INA

TIO

N

5000ν

&1500ν

DIM

UO

NE

VE

NT

SA

MPLE

:

AS

SU

ME

DPA

RM

.:s(x

)=κu

(x)+d(x

)2

(1−x

NE

GA

TIV

Es−s

AT

SM

ALLx

⇒M

OM

.F

RA

CT.s−s

=−

0.0

03±

0.0

01

NUT

EV

AN

OM

ALY

WO

RS

E!

HO

WE

VE

R,B

PZ

GLO

BA

LFIT

TO

NE

UTR

INO

INC

LUS

IVE

DIS

(Baro

ne

etal

2003)⇒

PO

SIT

IVE

(TIN

Y)

AS

YM

ME

TR

Y

Page 26: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

DIS

EN

TA

NG

LIN

GS

TR

AN

GE

NE

SS

CH

AR

MIS

CO

PIO

US

LY

PR

OD

UC

ED

INW

++s→c

easi

lyta

gged

thro

ugh

dim

uon

sign

al,

2nd

mu

onfr

omsu

bse

qu

entc

dec

ay

⇒A

CC

UR

ATE

EX

TR

AC

TIO

NO

FTH

ES

TR

AN

GE

DIS

TR

IBU

TIO

N

-0.0

020

0.00

2

0.00

4

0.00

6

0.00

8

0.01

00.

20.

40.

60.

8a)Q2 =2

0GeV

2

x

xs-xs-

0

0.51

1.52

2.53

3.54

4.55

0.2

0.4

0.6

b) x

s/s-

CC

FR

fit2

BPZ

NuT

eV

x(s−

s)s(

x)/s

(x)

−−

NuT

eVBPZ

CC

FR

/NUT

EVs−s

DE

TE

RM

INA

TIO

N

5000ν

&1500ν

DIM

UO

NE

VE

NT

SA

MPLE

:

AS

SU

ME

DPA

RM

.:s(x

)=κu

(x)+d(x

)2

(1−x

NE

GA

TIV

Es−s

AT

SM

ALLx

⇒M

OM

.F

RA

CT.s−s

=−

0.0

03±

0.0

01

NUT

EV

AN

OM

ALY

WO

RS

E!

HO

WE

VE

R,B

PZ

GLO

BA

LFIT

TO

NE

UTR

INO

INC

LUS

IVE

DIS

(Baro

ne

etal

2003)⇒

PO

SIT

IVE

(TIN

Y)

AS

YM

ME

TR

Y

Page 27: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

DIS

EN

TA

NG

LIN

GS

TR

AN

GE

NE

SS

CH

AR

MIS

CO

PIO

US

LY

PR

OD

UC

ED

INW

++s→c

easi

lyta

gged

thro

ugh

dim

uon

sign

al,

2nd

mu

onfr

omsu

bse

qu

entc

dec

ay

⇒A

CC

UR

ATE

EX

TR

AC

TIO

NO

FTH

ES

TR

AN

GE

DIS

TR

IBU

TIO

N

-0.0

020

0.00

2

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Page 28: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

CO

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Page 29: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

CO

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Page 30: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

MO

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Page 31: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

ELE

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Page 32: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

sin

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(νe−→νe−

)=

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π

[ g2 L

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y≡Ee/E

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+B

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)−

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sin

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sin

2θ W

0.0

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(NC

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77

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sin

2θ W

0.5

51

νee−→νee−

(NC

+CC

)si

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1 2+

sin

2θ W

0.2

31

Page 33: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

sin

2θ W

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ALL

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N:

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tic/

DIS∼me/m

p

dσ dy

(νe−→νe−

)=

2G2 FmeEν

π

[ g2 L

+g

2 R(1−y)2] ;

y≡Ee/E

ν

AT

NU

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EX

PE

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107

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ton

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etec

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yr.

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b−

1);

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TE:σ∝Eν

sin

2θ W

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INE

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RO

Mg A

,g V

(ORg L

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):R

EA

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g Rg

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1 3g

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(NC

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sin

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sin

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0.0

91

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77

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sin

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0.5

51

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+CC

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31

Page 34: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

CU

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02468101214161820

05

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µ- bea

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Page 35: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

LOW

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GY

(?)

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RO

SS

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CTIO

NA

GA

IN

dσ dy

(νe−→νe−

)=

2G

2 FmeEν

π

[ g2 L

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2 R(1−y)2]

⇒LO

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Page 36: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

TH

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EU

TR

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Page 37: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

sin

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+

=σNC

(νµ)

+σNC

(νe)

σCC

(νµ)

+σCC

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=σNC

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)−σNC

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Page 38: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

sin

2θ W

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SS

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PE

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FA

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)+

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Page 39: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

sin

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Page 40: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

sin

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un

det

erm

ined

)–E< ∼Mn⇒

ALL

XS

EC

TS

LIN

EA

RLY

IND

EP.

,B

UT

EIG

HT

FO

RM

FA

CTO

RS→

NE

ED

TO

INPU

TTH

RE

EFO

RM

FA

CTO

RS

•W

ITHν,ν

BE

AM

S&

NU

CLE

ON

TA

RG

ETS,(O

NLYp,

ISO

SC

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RN

UC

LEI,.

..)

FO

UR

IND

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CR

OS

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ED

TO

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TS

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AN

GE

FO

RM

FA

CTO

RGs A

Page 41: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

sin

2θ W

FR

OM

ELA

STIC

SC

ATTE

RIN

GO

FF

NU

CLE

ON

S

•(Q

UA

SI)E

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TICν-N

UC

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NC

RO

SS

SE

CTIO

NS

DE

PE

ND

ON

FIV

EIN

DE

P.FO

RM

FA

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RS

(Gp M

,Gn M

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,Gs M

,Gs A

)+

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p E,Gn E

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ETS,

SIX

IND

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CR

OS

SS

EC

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NS

–E>>Mn⇒

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SE

CTS

AR

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AR

LY

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EN

T→

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ND

ETE

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NG

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n2θ W

&FO

UR

OU

TO

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(ali

nea

rco

mb

inat

ion

ofth

eth

ree

mag

net

icf.

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un

det

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ALL

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EC

TS

LIN

EA

RLY

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EP.

,B

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FO

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FA

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BE

AM

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Page 42: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

BE

AM

OPTIO

NS

AN

DQ

UA

NTIT

ATIV

EE

STIM

ATE

S(P

.F

erra

rio,

S.F

.)

•TW

OE

XTR

EM

EE

NE

RG

YS

CE

NA

RIO

S:

β60→〈E

ν〉≈

200

MEV

(LO

WE

NE

RG

Y)

β1500→〈E

ν〉≈

5G

EV

(HIG

HE

NE

RG

Y)

•C

OM

PU

TE

RA

TE

SO

N4.4

MTO

NW

ATE

RA

T130

KM

:Φν∼

Φν∼

10

11/(m

2yr)

–at

low

ener

gy,∼

1.5×

10

5C

and

as

manyν

even

ts;∼

1.6

10

4N

Cpro

tonν

and∼

halfν

even

ts,∼

1.3

10

4N

Cneu

tronν

and∼

halfν

even

ts

–at

hig

hen

ergy,∼

10

6C

and

as

manyν

even

ts;∼

1.5

10

5N

Cpro

tonν

and

as

manyν

even

ts,∼

1.3

10

5N

Cneu

tronν

and

as

manyν

even

ts

•B

INE

VE

NTS

W.

XS

EC

TA

PPR

OX

CO

NS

TA

NT

INB

IN:

AN

G.

RE

SO

LUTIO

N∆θ∼

5◦

NO

TEy

DE

PE

ND

EN

CE

DR

IVE

NB

YF

OR

MFA

CTO

RTH

RO

UG

HQ

2=

2Mp(yEν−Mp)

–at

low

ener

gy,

rate

unif

orm

lydis

trib

ute

din∼

20

bin

sof

0.0

03<Q

2<

0.1

GeV

2

–at

hig

hen

ergy,

rate

conce

ntr

ate

din

firs

ttw

oout

of∼

20

bin

sQ

2< ∼

1G

eV2

•E

RR

OR

ON

sin

2θ W

:LO

WE

NE

RG

Y:δ

=∼

10−

3(W

ITH

P/N

SE

PA

RA

TIO

N);

δ=∼

10−

2(W

ITH

OU

TP/N

SE

PA

RA

TIO

N)

HIG

HE

NE

RG

Y:δ

=∼

10−

3(W

ITH

OR

WIT

HO

UT

P/N

SE

PA

RA

TIO

N)

–no

signifi

cant

gain

from

p/n

at

hig

hen

ergy:

dep

.of

xse

ctonGs A

ver

yw

eak

–no

signifi

cant

gain

from

hig

hen

ergy:

incr

ease

dxse

ctin

low

-yw

her

edep

on

sin

2θ W

wea

k

Page 43: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

BE

AM

OPTIO

NS

AN

DQ

UA

NTIT

ATIV

EE

STIM

ATE

S(P

.F

erra

rio,

S.F

.)

•TW

OE

XTR

EM

EE

NE

RG

YS

CE

NA

RIO

S:

β60→〈E

ν〉≈

200

MEV

(LO

WE

NE

RG

Y)

β1500→〈E

ν〉≈

5G

EV

(HIG

HE

NE

RG

Y)

•C

OM

PU

TE

RA

TE

SO

N4.4

MTO

NW

ATE

RA

T130

KM

:Φν∼

Φν∼

10

11/(m

2yr)

–at

low

ener

gy,∼

1.5×

10

5C

and

as

manyν

even

ts;∼

1.6

10

4N

Cpro

tonν

and∼

halfν

even

ts,∼

1.3

10

4N

Cneu

tronν

and∼

halfν

even

ts

–at

hig

hen

ergy,∼

10

6C

and

as

manyν

even

ts;∼

1.5

10

5N

Cpro

tonν

and

as

manyν

even

ts,∼

1.3

10

5N

Cneu

tronν

and

as

manyν

even

ts

•B

INE

VE

NTS

W.

XS

EC

TA

PPR

OX

CO

NS

TA

NT

INB

IN:

AN

G.

RE

SO

LUTIO

N∆θ∼

5◦

NO

TEy

DE

PE

ND

EN

CE

DR

IVE

NB

YF

OR

MFA

CTO

RTH

RO

UG

HQ

2=

2Mp(yEν−Mp)

–at

low

ener

gy,

rate

unif

orm

lydis

trib

ute

din∼

20

bin

sof

0.0

03<Q

2<

0.1

GeV

2

–at

hig

hen

ergy,

rate

conce

ntr

ate

din

firs

ttw

oout

of∼

20

bin

sQ

2< ∼

1G

eV2

•E

RR

OR

ON

sin

2θ W

:LO

WE

NE

RG

Y:δ

=∼

10−

3(W

ITH

P/N

SE

PA

RA

TIO

N);

δ=∼

10−

2(W

ITH

OU

TP/N

SE

PA

RA

TIO

N)

HIG

HE

NE

RG

Y:δ

=∼

10−

3(W

ITH

OR

WIT

HO

UT

P/N

SE

PA

RA

TIO

N)

–no

signifi

cant

gain

from

p/n

at

hig

hen

ergy:

dep

.of

xse

ctonGs A

ver

yw

eak

–no

signifi

cant

gain

from

hig

hen

ergy:

incr

ease

dxse

ctin

low

-yw

her

edep

on

sin

2θ W

wea

k

Page 44: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

BE

AM

OPTIO

NS

AN

DQ

UA

NTIT

ATIV

EE

STIM

ATE

S(P

.F

erra

rio,

S.F

.)

•TW

OE

XTR

EM

EE

NE

RG

YS

CE

NA

RIO

S:

β60→〈E

ν〉≈

200

MEV

(LO

WE

NE

RG

Y)

β1500→〈E

ν〉≈

5G

EV

(HIG

HE

NE

RG

Y)

•C

OM

PU

TE

RA

TE

SO

N4.4

MTO

NW

ATE

RA

T130

KM

:Φν∼

Φν∼

10

11/(m

2yr)

–at

low

ener

gy,∼

1.5×

10

5C

and

as

manyν

even

ts;∼

1.6

10

4N

Cpro

tonν

and∼

halfν

even

ts,∼

1.3

10

4N

Cneu

tronν

and∼

halfν

even

ts

–at

hig

hen

ergy,∼

10

6C

and

as

manyν

even

ts;∼

1.5

10

5N

Cpro

tonν

and

as

manyν

even

ts,∼

1.3

10

5N

Cneu

tronν

and

as

manyν

even

ts

•B

INE

VE

NTS

W.

XS

EC

TA

PPR

OX

CO

NS

TA

NT

INB

IN:

AN

G.

RE

SO

LUTIO

N∆θ∼

5◦

NO

TEy

DE

PE

ND

EN

CE

DR

IVE

NB

YF

OR

MFA

CTO

RTH

RO

UG

HQ

2=

2Mp(yEν−Mp)

–at

low

ener

gy,

rate

unif

orm

lydis

trib

ute

din∼

20

bin

sof

0.0

03<Q

2<

0.1

GeV

2

–at

hig

hen

ergy,

rate

conce

ntr

ate

din

firs

ttw

oout

of∼

20

bin

sQ

2< ∼

1G

eV2

•E

RR

OR

ON

sin

2θ W

:LO

WE

NE

RG

Y:δ

=∼

10−

3(W

ITH

P/N

SE

PA

RA

TIO

N);

δ=∼

10−

2(W

ITH

OU

TP/N

SE

PA

RA

TIO

N)

HIG

HE

NE

RG

Y:δ

=∼

10−

3(W

ITH

OR

WIT

HO

UT

P/N

SE

PA

RA

TIO

N)

–no

signifi

cant

gain

from

p/n

at

hig

hen

ergy:

dep

.of

xse

ctonGs A

ver

yw

eak

–no

signifi

cant

gain

from

hig

hen

ergy:

incr

ease

dxse

ctin

low

-yw

her

edep

on

sin

2θ W

wea

k

Page 45: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

BE

AM

OPTIO

NS

AN

DQ

UA

NTIT

ATIV

EE

STIM

ATE

S(P

.F

erra

rio,

S.F

.)

•TW

OE

XTR

EM

EE

NE

RG

YS

CE

NA

RIO

S:

β60→〈E

ν〉≈

200

MEV

(LO

WE

NE

RG

Y)

β1500→〈E

ν〉≈

5G

EV

(HIG

HE

NE

RG

Y)

•C

OM

PU

TE

RA

TE

SO

N4.4

MTO

NW

ATE

RA

T130

KM

:Φν∼

Φν∼

10

11/(m

2yr)

–at

low

ener

gy,∼

1.5×

10

5C

and

as

manyν

even

ts;∼

1.6

10

4N

Cpro

tonν

and∼

halfν

even

ts,∼

1.3

10

4N

Cneu

tronν

and∼

halfν

even

ts

–at

hig

hen

ergy,∼

10

6C

and

as

manyν

even

ts;∼

1.5

10

5N

Cpro

tonν

and

as

manyν

even

ts,∼

1.3

10

5N

Cneu

tronν

and

as

manyν

even

ts

•B

INE

VE

NTS

W.

XS

EC

TA

PPR

OX

CO

NS

TA

NT

INB

IN:

AN

G.

RE

SO

LUTIO

N∆θ∼

5◦

NO

TEy

DE

PE

ND

EN

CE

DR

IVE

NB

YF

OR

MFA

CTO

RTH

RO

UG

HQ

2=

2Mp(yEν−Mp)

–at

low

ener

gy,

rate

unif

orm

lydis

trib

ute

din∼

20

bin

sof

0.0

03<Q

2<

0.1

GeV

2

–at

hig

hen

ergy,

rate

conce

ntr

ate

din

firs

ttw

oout

of∼

20

bin

sQ

2< ∼

1G

eV2

•E

RR

OR

ON

sin

2θ W

:LO

WE

NE

RG

Y:δ

=∼

10−

3(W

ITH

P/N

SE

PA

RA

TIO

N);

δ=∼

10−

2(W

ITH

OU

TP/N

SE

PA

RA

TIO

N)

HIG

HE

NE

RG

Y:δ

=∼

10−

3(W

ITH

OR

WIT

HO

UT

P/N

SE

PA

RA

TIO

N)

–no

signifi

cant

gain

from

p/n

at

hig

hen

ergy:

dep

.of

xse

ctonGs A

ver

yw

eak

–no

signifi

cant

gain

from

hig

hen

ergy:

incr

ease

dxse

ctin

low

-yw

her

edep

on

sin

2θ W

wea

k

Page 46: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

DE

TE

CTIO

NC

ON

STR

AIN

TS

(V.

Anto

nel

li,

G.

Batt

isto

ni,

S.F

.)

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WA

TE

RC

ER

EN

KO

V,

NE

ED

p E>

0.7

5F

OR

RE

CO

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OTO

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p>

1.1

GEV

;C

AN

NO

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CO

ILIN

GN

EU

TR

ON

•IN

LIQ

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AR,

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300

MEV

(E−m> ∼

50

MEV

)IN

OR

DE

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HAV

ER

EA

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NA

BLE

PR

OTO

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NO

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ON

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SE

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TS

CA

NN

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TE

CT

RE

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ILIN

GN

EU

TR

ON

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RH

APS

NE

UTR

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TE

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NPO

SS

IBLE

TH

RO

UG

HR

EC

OIL

AF

TE

RD

EU

TE

RIU

MB

RE

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UP

(SN

O)?

•Q

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TIC

CO

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ER

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AX

IMIZ

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FF

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CY→

HIG

HE

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Y

⇒O

PTIM

AL

EN

ER

GY

AR

OU

ND

1G

EV

Page 47: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

DE

TE

CTIO

NC

ON

STR

AIN

TS

(V.

Anto

nel

li,

G.

Batt

isto

ni,

S.F

.)

•IN

WA

TE

RC

ER

EN

KO

V,

NE

ED

p E>

0.7

5F

OR

RE

CO

ILIN

GPR

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1.1

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AN

NO

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CO

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GN

EU

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300

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MEV

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OR

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ER

EA

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BLE

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NO

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TE

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TE

RD

EU

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MB

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(SN

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TIC

CO

NTR

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AX

IMIZ

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FF

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CY→

HIG

HE

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Y

⇒O

PTIM

AL

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AR

OU

ND

1G

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Page 48: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

DE

TE

CTIO

NC

ON

STR

AIN

TS

(V.

Anto

nel

li,

G.

Batt

isto

ni,

S.F

.)

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WA

TE

RC

ER

EN

KO

V,

NE

ED

p E>

0.7

5F

OR

RE

CO

ILIN

GPR

OTO

N⇒

p>

1.1

GEV

;C

AN

NO

TD

ETE

CT

RE

CO

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GN

EU

TR

ON

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LIQ

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AR,

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300

MEV

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50

MEV

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HAV

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EA

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NO

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Page 49: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p
Page 50: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p
Page 51: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

sin

2θ W

AT

LOW

EN

ER

GY:

(TE

NTA

TIV

E)

QU

AN

TIT

ATIV

EC

ON

CLU

SIO

NS

•M

EA

SU

RE

ME

NT

WIT

HW

ATE

RC

ER

EN

KO

V&

PR

ES

EN

TTE

CH

NO

LOG

YN

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RE

ALI

STIC

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EA

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ME

NT

WIT

HPR

ES

EN

TIC

AR

US

TE

CH

NO

LOG

YFE

AS

IBLE

–C

UTpp> ∼

300

MEV

IMPLI

ESQ

2> ∼

0.1

GEV

2

⇒LO

SS

OF

2/3

OF

XS

EC

TIN

FIR

ST

BIN

,A

BO

UT

25%

OF

TO

TA

L

–A

TFA

RD

ETE

CTO

R,

ME

AS

UR

EM

EN

TO

NLY

CO

MPE

TIT

IVE

WIT

HLA

RG

EV

OLU

ME

(5M

TO

NTO

RE

AC

H5×

10−

3A

CC

UR

AC

Y)

–A

TN

EA

RD

ETE

CTO

RM

EA

SU

RE

ME

NT

ALR

EA

DY

CO

MPE

TIT

IVE

WIT

HS

MA

LLV

OLU

ME

(500

TO

NTO

RE

AC

H5×

10−

4A

CC

UR

AC

Y)

•S

NO

TE

CH

NO

LOG

YM

IGH

TE

NA

BLE

LOW

-EN

ER

GY

ME

AS

UR

EM

EN

T,

MU

ST

BE

INV

ES

TIG

ATE

D

Page 52: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

sin

2θ W

AT

LOW

EN

ER

GY:

(TE

NTA

TIV

E)

QU

AN

TIT

ATIV

EC

ON

CLU

SIO

NS

•M

EA

SU

RE

ME

NT

WIT

HW

ATE

RC

ER

EN

KO

V&

PR

ES

EN

TTE

CH

NO

LOG

YN

OT

RE

ALI

STIC

•M

EA

SU

RE

ME

NT

WIT

HPR

ES

EN

TIC

AR

US

TE

CH

NO

LOG

YFE

AS

IBLE

–C

UTpp> ∼

300

MEV

IMPLI

ESQ

2> ∼

0.1

GEV

2

⇒LO

SS

OF

2/3

OF

XS

EC

TIN

FIR

ST

BIN

,A

BO

UT

25%

OF

TO

TA

L

–A

TFA

RD

ETE

CTO

R,

ME

AS

UR

EM

EN

TO

NLY

CO

MPE

TIT

IVE

WIT

HLA

RG

EV

OLU

ME

(5M

TO

NTO

RE

AC

H5×

10−

3A

CC

UR

AC

Y)

–A

TN

EA

RD

ETE

CTO

RM

EA

SU

RE

ME

NT

ALR

EA

DY

CO

MPE

TIT

IVE

WIT

HS

MA

LLV

OLU

ME

(500

TO

NTO

RE

AC

H5×

10−

4A

CC

UR

AC

Y)

•S

NO

TE

CH

NO

LOG

YM

IGH

TE

NA

BLE

LOW

-EN

ER

GY

ME

AS

UR

EM

EN

T,

MU

ST

BE

INV

ES

TIG

ATE

D

Page 53: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

sin

2θ W

AT

LOW

EN

ER

GY:

(TE

NTA

TIV

E)

QU

AN

TIT

ATIV

EC

ON

CLU

SIO

NS

•M

EA

SU

RE

ME

NT

WIT

HW

ATE

RC

ER

EN

KO

V&

PR

ES

EN

TTE

CH

NO

LOG

YN

OT

RE

ALI

STIC

•M

EA

SU

RE

ME

NT

WIT

HPR

ES

EN

TIC

AR

US

TE

CH

NO

LOG

YFE

AS

IBLE

–C

UTpp> ∼

300

MEV

IMPLI

ESQ

2> ∼

0.1

GEV

2

⇒LO

SS

OF

2/3

OF

XS

EC

TIN

FIR

ST

BIN

,A

BO

UT

25%

OF

TO

TA

L

–A

TFA

RD

ETE

CTO

R,

ME

AS

UR

EM

EN

TO

NLY

CO

MPE

TIT

IVE

WIT

HLA

RG

EV

OLU

ME

(5M

TO

NTO

RE

AC

H5×

10−

3A

CC

UR

AC

Y)

–A

TN

EA

RD

ETE

CTO

RM

EA

SU

RE

ME

NT

ALR

EA

DY

CO

MPE

TIT

IVE

WIT

HS

MA

LLV

OLU

ME

(500

TO

NTO

RE

AC

H5×

10−

4A

CC

UR

AC

Y)

•S

NO

TE

CH

NO

LOG

YM

IGH

TE

NA

BLE

LOW

-EN

ER

GY

ME

AS

UR

EM

EN

T,

MU

ST

BE

INV

ES

TIG

ATE

D

Page 54: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

STR

ON

GIN

TE

RA

CTIO

NS

Page 55: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

FLA

VO

UR

SE

PA

RA

TIO

NA

TTH

EN

EU

TR

INO

FA

CTO

RY

•N

EU

TR

INO

BE

AM

ISW

IDE

BA

ND→

CA

ND

ETE

RM

INE

ALLFi,g i

FR

OM

y=Q

2/(

2xmpEν)

DE

PE

ND

EN

CE

OF

(E.G

.)

d2σ↑λ`

dxdy−d

2σ↓λ`

dxdy

=G

2 F

(1+Q

2/m

2 W)2Q

2

xy

[ λ`y(2−y)xg 1

(x,Q

2)

+(1−y)g

4(x,Q

2)

+y

2xg 5

(x,Q

2)]

•C

AN

DIS

EN

TA

NG

LEIN

DIV

IDU

AL

PD

FS

BY

LIN

EA

RC

OM

BIN

ATIO

N:

AT

LO

1 2

( gW−

1−gW−

5

)=

∆u

+∆c;

1 2

( gW

+

1+gW

+

5

)=

∆u

+∆c

1 2

( gW

+

1−gW

+

5

)=

∆d+

∆s;

1 2

( gW−

1+gW−

5

)=

∆d+

∆s

∆c,

∆c,

∆s,

∆s

only

pre

sent

abov

ech

arm

thre

shol

d

Page 56: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

STR

UC

TU

RE

FU

NC

TIO

NS

AT

TH

FA

CTO

RY:

UN

PO

LAR

IZE

D...

EV

EN

TR

ATE

S(D

EFA

ULT

BE

AM

AN

DD

ETE

CTO

R)

EX

PE

CTE

DS

TA

T.E

RR

OR

S

KIN

EM

ATIC

CO

VE

RA

GE

AN

DA

CC

UR

AC

YR

ATH

ER

BE

TTE

RTH

AN

CU

RR

EN

TC

HA

RG

ED

LEPTO

NE

XPE

RIM

EN

TS

(E.G

.N

MC

)

Page 57: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

...A

ND

PO

LAR

IZE

D

PR

ES

EN

TA

BS

OLU

TEν

FA

CT

ER

RS.

STA

TIS

TIC

AL

AC

CU

RA

CY

AB

OU

TO

NE

OR

DE

RO

FM

AG

NIT

UD

EB

ETTE

RTH

AN

CU

RR

EN

TPO

LAR

IZE

DC

HA

RG

ED

-LE

PTO

NE

XPE

RIM

EN

TS!

Page 58: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

PO

LAR

IZE

DD

ISA

TAν

FA

CT

(S.F

.,M

.L.M

angano,

G.R

idolfi

)

LIG

HT

FLA

VO

UR

SE

PA

RA

TIO

N:

•P

RE

SE

NT:

TR

IPLE

Ta

3=

1.1

0.0

4;

NO

INF

OO

N∆q−

∆q

•ν–F

AC

T.:a

3=

1.1

07±

0.0

06;

∆(u−u

)=

0.7

64±

0.0

06;

∆(d−d)

=−

0.3

20±

0.0

08;

ISTH

EG

LUO

NC

ON

TR

IBU

TIO

N“L

AR

GE”?

(w.r

.to

qu

ark

)IS

TH

ES

CA

LE–I

NVA

RIA

NT

QU

AR

K“S

MA

LL”?

(w.r

.to

oct

et)

•P

RE

SE

NT:

GLU

ON:

∆g(1,1

GeV

2)

=0.8±

0.2

;S

CA

LE–I

NV.

QU

AR

K∆

Σ(1

)=

0.3

0.0

3;

OC

TE

Ta

8=

0.6±

30%

(?)

•ν–F

AC

T.:

“AN

OM

ALY”

∆g

=0.9±

0.1

;∆

Σ=

0.3

0.0

1;a

8=

0.5

0.0

1‘I N

STA

NTO

N”

∆g

=0.2±

0.1

;∆

Σ=

0.3

0.0

1;a

8=

0.5

0.0

1

ISTH

ES

TR

AN

GE

NE

SS

“VA

LEN

CE

LIK

E”?

•P

RE

SE

NT:

NO

INF

OR

MA

TIO

NO

NVA

LEN

CE–S

EA

SE

PA

RA

TIO

N

•ν–F

AC

T.:

‘INS

TA

NTO

N”

[∆s−

∆s]

(1,1

GeV

2)

=−

0.0

07±

0.0

07;

‘SK

YR

MIO

N”

[∆s−

∆s]

(1,1

GeV

2)

=−

0.1

06±

0.0

08;

CA

NE

AS

ILY

TE

LLS

CE

NA

RIO

SFR

OM

EA

CH

OTH

ER

BU

TE

RR

OR

ON

SIN

GLE

TD

RIV

EN

BY

SYS

TE

RR

OR

ON

GLU

ON:

ON

LY

OB

STA

CLE

TO

FU

LLS

PIN

STR

UC

TU

RE

IS∆g!

Page 59: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

TH

EPR

OTO

NS

PIN

STR

UC

TU

RE

FR

OM

LOW

-EN

ER

GY

DA

TA

AX

IAL

CH

AR

GE

SF

RO

ME

LAS

TICν-p

SC

ATTE

RIN

G(K

apla

n&

Manohar,

1988):

〈p′ |js 5µ|p〉=

u(p′ )γµγ

5u

(p)G

s A(Q

2);

Gs A

(0)

=∆s

•C

AN

DE

TE

RM

INE

∆s

FR

OM

FO

RW

AR

DS

TR

AN

GE

AX

IAL

FO

RM

FA

CTO

R

•D

ETE

RM

INE

FO

RM

FA

CTO

RA

TS

MA

LLQ

2&

EX

TR

APO

LATE

TOQ

2=

0

•C

OR

RE

CTIO

NS

FR

OM

HIG

HE

RD

IME

NS

ION

AL

OPE

RA

TO

RS

KN

OW

N&

SM

ALL

•C

AN

EX

TR

AC

TGA

FR

OM

UN

PO

LAR

IZE

DX

SE

CT,

BU

TW

.LA

RG

EE

RR

OR

PO

LAR

IZE

DE

LAS

TIC

CA

SE

WO

RTH

INV

ES

TIG

ATIN

G

Page 60: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

CO

NC

LUS

ION

S

•N

EU

TR

INO

SC

ATTTE

RIN

GE

XPE

RIM

EN

TS

HAV

EB

EE

N

CR

UC

IAL

INE

STA

BLI

SH

ING

TH

ES

TA

ND

AR

DM

OD

EL

•A

TPR

ES

EN

T,TH

EY

STR

ETC

HTH

EB

OU

ND

AR

IES

OF

TH

ES

TA

ND

AR

DM

OD

EL

•N

EW

PH

YS

ICS

ISB

EH

IND

TH

EC

OR

NE

R

Page 61: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

CO

NC

LUS

ION

S

•N

EU

TR

INO

SC

ATTTE

RIN

GE

XPE

RIM

EN

TS

HAV

EB

EE

N

CR

UC

IAL

INE

STA

BLI

SH

ING

TH

ES

TA

ND

AR

DM

OD

EL

•A

TPR

ES

EN

T,TH

EY

STR

ETC

HTH

EB

OU

ND

AR

IES

OF

TH

ES

TA

ND

AR

DM

OD

EL

•N

EW

PH

YS

ICS

ISB

EH

IND

TH

EC

OR

NE

R

Page 62: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

CO

NC

LUS

ION

S

•N

EU

TR

INO

SC

ATTTE

RIN

GE

XPE

RIM

EN

TS

HAV

EB

EE

N

CR

UC

IAL

INE

STA

BLI

SH

ING

TH

ES

TA

ND

AR

DM

OD

EL

•A

TPR

ES

EN

T,TH

EY

STR

ETC

HTH

EB

OU

ND

AR

IES

OF

TH

ES

TA

ND

AR

DM

OD

EL

•N

EW

PH

YS

ICS

ISB

EH

IND

TH

EC

OR

NE

R

Page 63: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

CA

NM

EA

SU

RE

AC

CU

RA

TE

LY

SH

APE

OF

LIG

HT

FLA

VO

RS

BU

TN

OT

STR

AN

GE

NE

SS

OR

CH

AR

M

UN

LES

STH

EG

LUO

NIS

KN

OW

N

(CO

MPA

SS

,R

HIC

!)

0

0.1

0.2

0.3

0.4

0.5 10

-310

-210

-1

x

-0.2

5

-0.2

-0.1

5

-0.1

-0.0

50

0.050.1

0.15

10-3

10-2

10-1

x

-0.5

-0.2

50

0.250.5

0.751

1.251.5

1.752 10

-310

-210

-1

x

-0.0

4

-0.0

3

-0.0

2

-0.0

10

0.01

0.02

10-3

10-2

10-1

x

BLU

MLE

IN&

BO

TTC

HE

R,2003

νFA

CT

PA

RTO

NS

&D

ATA

gW−

1−gW−

5∼

∆u

+∆c−αs

∆g

gW

+

1−gW

+

5∼

∆d

+∆s−αs

∆g

Page 64: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

•C

HA

RM

FA

CTO

RY

PH

YS

ICS:

CH

AR

MPR

OD

UC

ED

INW

++s→c

easi

lyta

gged

thro

ugh

dim

uon

sign

al,

2n

dm

uon

from

sub

sequ

entc

dec

ay⇒

STR

AN

GE

QU

AR

K

•Λ

PO

LAR

IZA

TIO

NIN

TH

EC

UR

RE

NT

FR

AG

ME

NTA

TIO

NR

EG

ION⇒

FR

AG

ME

NTA

TIO

N

FU

NC

TIO

NS

•ν–I

ND

UC

ED

EX

CLU

SIV

EDs

PR

OD

UC

TIO

N⇒

GE

NE

RA

LIZ

ED

PA

RTO

ND

ISTR

IBU

TIO

NS

Page 65: ANDARD - KEK · NEUTRINO BEAMS S TEF ANO F OR TE U NIVERSIT ... ost-LHC construction windo w ma y exist for a facilit y to b e sited at CERN {CERN should arrange for budget and p

AN

EX

AM

PLE

:PO

LAR

IZE

DS

TR

AN

GE

NE

SS

-0.0

10

0.01

10-2

10-1

1

µ2 = 2

2 G

eV2

c)

ξ∆ s

( ξ

, µ2 )

-0.0

10

0.01

10-2

10-1

1

µ2 = 1

3 G

eV2

-0.0

10

0.01

10-2

10-1

1

µ2 = 8

GeV

2

-0.0

10

0.01

10-2

10-1

1

µ2 = 5

GeV

2

-0.0

10

0.01

10-2

10-1

1 ξ

µ2 = 3

.5 G

eV2

Str

an

ge

dis

tn.

at

LO

dir

ectl

yd

eter

min

edby

tagged

–ch

arm

stru

ctu

refu

nct

ion

:

gW

+

1,c

(x,Q

2)

=|Vcs|2

∆s(ξ,µ

2 c)

+|Vcd|2

∆d(ξ,µ

2 c);

ξ=x

(1+m

2 c/Q

2);µ

2 c=Q

2+m

2 c

Sta

tist

ical

erro

rssm

all

;h

owev

erla

rge

erro

rin

-

du

ced

by

QC

Dco

rrn

s.d

ue

tou

nce

rtain

tyon

glu

on

EX

CE

LLE

NT

DE

TE

RM

INA

TIO

NO

FS

HA

PE

IFG

LUO

N

KN

OW

N(C

OM

PA

SS

,R

HIC

...)