physics - stanford universityk i? physics do es not dep end on buras et al " 0 k " k im v...
TRANSCRIPT
PHYSICS BEYOND �PT
A. Pich
IFIC, Univ. Valencia { CSIC
� F�(t): F. Guerrero, A.P., PLB 412 (1997) 382
F. Guerrero, PRD 57 (1998) 4136
D. G�omez{Dumm, A.P., J. Portol�es, PRD 62(2000) 054014
� F ��
S(t): E. Pallante, A.P., hep-ph/0007208
� "0=": E. Pallante, A.P., PRL 84 (2000) 2568;
E. Pallante, A.P., hep-ph/0007208
E. Pallante, A.P., I. Scimemi, IFIC/00-31
G. Ecker etal., PLB 477 (2000) 88
� FK�
S(t) ; ms: M. Jamin, J.A. Oller, A.P., hep-ph/0006045
M. Jamin, J.A. Oller, A.P., IFIC/00-32
� KL ! �+��: D. G�omez{Dumm, A.P., PRL 80 (1998) 4633
EVOLUTION FROM MW TO MK
Scale Fields E�. Theory
MW
W;Z; ; g
�; �; e; �i
t; b; c; s; d; u
Standard Model
<�mc
; g ; �; e; �i
s; d; uL(nf=3)
QCD , L�S=1;2e�
MK
; �; e; �i
�;K; �ChPT
?
?
OPE
NC !1
�PT
Chiral Symmetry: [M � diag(mu;md;ms) = 0]
LQCD := i �qL/DqL+ i �qR/DqR ; qT = (u; d; s)
qL;R ! gL;R qL;R ; gL;R 2 SU(3)L;R
SU(3)L SU(3)R ! SU(3)V + 8 0� Goldstones
h�qjLqiRi U = exp
�ip2�=f
�; U ! gR U g
yL
� =
0BBB@q
12�0+
q16� �+ K+
�� �q
12�0+
q16� K0
K� �K0 �q
23�
1CCCA
Low{Energy Expansion: (p2n ; mnq ) L =
PnL2n
L2 = f2
4 hD�UyD�U + 2B0
�UyM+MyU
�i
= D��+D��
� �M2��+��+ � � �
+ 16f2
��+
$D� �
�� �
�+$D ���
�+ � � �
M2�
mu+md=
M2
K0
ms+md=
M2
K+
ms+mu= B0 = �h�qqi
f2
O(p4) �PT
i) L4 at tree level (Gasser{Leutwyler)
L4 = L1 hD�UyD�Ui2 + L2 hD�U
yD�Ui hD�UyD�Ui+ L3 hD�U
yD�UD�UyD�Ui + L4 hD�U
yD�Ui hUy�+ �yUi+ L5 hD�U
yD�U�Uy�+ �yU
�i + L6 hUy�+ �yUi2
+ L7 hUy�� �yUi2 + L8 h�yU�yU + Uy�Uy�i� i L9 hF ��
RD�UD�U
y+ F��
LD�U
yD�Ui + L10 hUyF ��
RUFL��i
F��
J� @�J� � @�J� � i[J�; J�] ; J� = l�; r� ; � � 2B0M
ii) L2 at one loop (Unitarity)
T4 � p4na log(p2=�2) + b(�)
o
� Chiral Logarithms unambiguously predicted
� Li's �xed by QCD dynamics
Reabsorb one{loop divergences Lri(�)
iii) Wess{Zumino{Witten term (chiral anomaly)
�0 ! ; � ! ; � ! �� ; � � �
O(p4) �PT COUPLINGS
i Lri(M�)� 103 Source �i
1 0:4� 0:3 Ke4, �� ! �� 3=32
2 1:4� 0:3 Ke4, �� ! �� 3=16
3 �3:5� 1:1 Ke4, �� ! �� 0
4 �0:3� 0:5 Zweig rule 1=8
5 1:4� 0:5 FK : F� 3=8
6 �0:2� 0:3 Zweig rule 11=144
7 �0:4� 0:2 Gell-Mann{Okubo, L5;8 0
8 0:9� 0:3 MK0 �MK+, L5, 5=48
(ms � m̂) : (md �mu)
9 6:9� 0:7 hr2i�V 1=4
10 �5:5� 0:7 � ! e� �1=4
Li = Lr
i(�) + �i
�D�4
32�2
n2
D�4 + E � log (4�) � 1o
Lr
i(�2) = Lr
i(�1) +
�i
(4�)2log
��1
�2
�
�� � 4�f� � 1:2 GeV Li � f2�=4
�2�� 2� 10�3
Li'S
FRO
M
RESO
NANCE
EXCHANGE
i
Lr i(M�)
V
A
S
S1
�1
Total
Totalb)
1
0:4�0:3
0:6
0
�0:2
0:2
0
0:6
0:9
2
1:4�0:3
1:2
0
0
0
0
1:2
1:8
3
�3:5�1:1
�3:6
0
0:6
0
0
�3:0
�4:9
4
�0:3�0:5
0
0
�0:5
0:5
0
0:0
0:0
5
1:4�0:5
0
0
1:4a)
0
0
1:4
1:4
6
�0:2�0:3
0
0
�0:3
0:3
0
0:0
0:0
7
�0:4�0:2
0
0
0
0
�0:3
�0:3
�0:3
8
0:9�0:3
0
0
0:9a)
0
0
0:9
0:9
9
6:9�0:7
6:9a)
0
0
0
0
6:9
7:3
10
�5:5�0:7
�10:0
4:0
0
0
0
�6:0
�5:5
a)
Input
b)
LV 1
=
LV 2=2=
�LV 3=6=
LV 9=8=
�L
V
+A
10
=6=
f2 �=(16M2 V)
PION FORM FACTOR
h�0��j�d �uj0i �p2 F�(s)
�p�� � p�0
��
� O(p4) �PT:
F�(s) = 1+2Lr
9(�)
f2�s� s
96�2f2�A
�M2
�s;M2
�
�2
�
A(x; y) � log y+8x� 53+ �3
xlog
��x+1�x�1
�; �x �
p1� 4x
� NC !1: (1 Resonance only)
�
�
�
�
�
+
�
�
�
F�(s) = 1+FVGV
f2�
sM2
��s=
M2�
M2��s
(lims!1 F�(s) = 0)
� O(p4) �PT + NC !1:
F�(s) =M2
�
M2��s
� s96�2f2�
A
�M2
�s;M2
�
�2
�
� Omn�es Summation:
F�(s) =M2
�
M2��s
exp
�� s96�2f2�
A
�M2
�s ;
M2�
M2�
��
Omn�es Problem
ImAIJ(s+ i�) =
1
2
Xn
h(��)IJ jT yjni hnjOji(q)i
ImAIJ =
�ImAI
J
�2�
= e�i�IJ sin �IJ A
IJ = ei�
IJ sin �IJ A
I�J
= sin �IJ jAIJ j = tan �IJ ReA
IJ
AI
J(s) =
n�1Xk=0
(s� s0)k
k!
dkAI
J
dsk
����s=s0
+(s� s0)n
�
Z 1
4M2
�
dz
(z � s0)ntan �I
J(z)ReAI
J(z)
z � s� i�
AIJ(s) = exp
8<:n�1Xk=0
(s� s0)k
k!
dk
dsklog
nAIJ(s)
o���s=s0
+(s� s0)
n
�
Z 14M2
�
dz
(z � s0)n
�IJ(z)
z � s� i�
)
� I;J(s; s0) AIJ(s0)
� Rho Width: Dyson Summation
(a) (b)
(c) (d) (e)
F�(s) � M2�
M2��s�iM���(s)
��(s) = �(s� 4M2�) �
3�
M� s
96�f2�
��(s) = 144 MeV [exp: (150:7� 1:1) MeV]
�11(s) = arctan
�M� ��(s)Ms
��s
�� s �3�
96�f2�+ � � �
F�(s) =M2
�
M2��s�iM���(s)
exp
�� s96�2f2�
Re
�A
�M2
�s;M2
�
M2�
���
0.5 1 1.5
√s (GeV)
−1
0
1
log
|FV|2
CLEO−II dataALEPH dataFit (Mρ = 0.776 GeV)
Guerrero and Pich (Mρ = 0.776 GeV)
τ decay data vs theory
−0.5 0 0.5 1 1.5
s/ √(|s|) (GeV)
−0.5
0
0.5
1
1.5
log
|FV
|2
Fit τ data (Mρ = 0.776 GeV)
Guerrero and Pich (Mρ = 0.776 GeV)
e+ e
− data vs theory (fit to τ decay data)
SCALAR FORM FACTOR
h�i(p0)j�uu+ �ddj�k(p)i � �ik F�S (t)
F�S (t) = F�
S (0)n1+ g(t) +O(p4)
o
g(t) =t
f2
��1�M2
�
2t
��J��(t) +
1
4�JKK(t) +
M2�
18t�J��(t)
+ 4(Lr
5+ 2Lr
4)(�) +5
4(4�)2
�ln
�2
M2�
� 1
�� 1
4(4�)2lnM2
K
M2�
�
�JPP(t) = 1(4�)2
n2� �P ln
��P+1�P�1
�o; �P �
q1� 4M2
P
t
F�S (t) =0(t; t0)F
�S (t0)�0(t; t0)F
�S (0) f1+ g(t0)g
t0 g(t0) <0(M2K; t0) jF �
S(M2
K)=F �
S(0)j
0 0 1.45 1.45
M2�
0.042 1.40 1.46
2M2�
0.091 1.34 1.46
3M2�
0.15 1.26 1.45
4M2�
0.26 1.11 1.40
M2K
0:54� 0:46 i � 1 1.61
jF�S (M
2K)=F
�S (0)j = 1:55� 0:10
�+� �T(KL ! �+��)T(KS ! �+��)
� "K + "0K
�00 �T(KL ! �0�0)
T(KS ! �0�0)� "K � 2"0K
"K = (2:280� 0:013)� 10�3 ei�"K
�"K = (43:47� 0:51)�
Re
"0K"K
!� 1
6
8<:1�
����� �00�+�
�����29=; = (19:3� 2:4)� 10�4
DIRECT CP VIOLATION
104Re("0K="K) = 33� 11 NA31 (1988)
32� 30 E731 (1988)
20� 7 NA31 (1993)
7:4� 5:9 E731 (1993)
28:0� 4:1 KTeV (1999)
14:0� 4:3 NA48 (1999{2000)
K ! 2� ISOSPIN AMPLITUDES
j��i : J = 0 , CP = + , I = 0 ; 2 (Bose)
A[K0! �+��] � A0 ei �0+
1p2A2 e
i �2
A[K0! �0�0] � A0 ei �0 �
p2A2 e
i �2
A[K+! �+�0] � 3
2A2 e
i �2
�I = 1=2 Rule :
! � Re (A2)Re (A0)
� 122
Strong Final State Interactions :
�0 � �2 = 45� � 6�
"0K = �ip2ei (�
2��0) !�Im (A0)Re (A0)
� Im (A2)Re (A2)
�
SHORT DISTANCES
L�S=1eff =� GFp
2Vud V
�us
Pi Ci(�) Qi(�)
Q1 =�s�u�
�V�A
�u�d�
�V�A
Q2 = (su)V�A (ud)V�A
Q3;5 = (sd)V�AP
q(qq)V�A
Q4;6 =�s�d�
�V�A
Pq(q�q�)V�A
Q7;9 = 32(sd)V�A
Pqeq (qq)V�A
Q8;10 = 32
�s�d�
�V�A
Pqeq(q�q�)V�A
q > � : Ci(�) = zi(�)� yi(�)�Vtd V
�ts=Vud V
�us
�O(�n
stn) , O(�n+1
stn) , [t � log (M=m)] (Munich / Rome)
q < � : h��jQi(�)jKi ?
Physics does not depend on �
Buras et al
"0K"K
� Im�V �tsVtd
� hP (1=2) � P (3=2)
i
P (1=2) = rXi
yi(�) hQi(�)i0 (1�IB)
P (3=2) =r
!
Xi
yi(�) hQi(�)i2
Experiment: r =GF !
2j"jRe (A0)
! =Re (A2)Re (A0)
� 122 ; Re(A0) = 3:37� 10�7 GeV
Theory: hQi(�)i � hQiivs Bi(�)
"0K"K
��110MeVms(2GeV)
�2 �B(1=2)6 (1�IB)� 0:4B
(3=2)8
�
B(1=2)6 = 1:0� 0:3 ; B
(3=2)8 = 0:8� 0:2
IB � �+�0 = 0:25� 0:08 0:16
�0{� MIXING (Ecker et al)
�0 � �3+ "�0� �8 A0 �! AIB2 / "�0� A0
A(K0 ! �0�0) � A(K0 ! �3�3) + 2 "�0�A(K0 ! �8�3)
IB =Im (AIB
2)
! Im (A0)=
2p2 "
�0�
3p3!
O(p2) CHPT: m̂ � (mu +md)=2
"(2)�0�
=
p3 (md�mu)4 (ms�m̂) IB � 0:13
O(p4) CHPT: "�0� = "(2)�0�
+ "(4)�0�
IB � �+�0 = 0:16� 0:03
"(4)�0�
="(2)�0�
/ f(3L7+ L8(�)) + � logsg
�0: "(4)�0�(L7)="
(2)�0�
= 1:10 ; a0: "(4)�0�(L8)="
(2)�0�
= �0:83
RECENT
THEO
RETICAL
ESTIM
ATES
Group
B(1=2)
6
B(3=2)
8
"0 K="K
�104
Munich
1:0�0:3
0:8�0:2
9:2+6:8
�4:0
(G)
1:4!32:7
(S)
Rome
1:0�1:0
0:71�0:13
8:1+10:3
�9:5
(G)
�13!37
(S)
Trieste
1:3
0:84
22�8
(G)
9!48
(S)
Dortmund
1:50!1:62
B(1=2)
6
=1:72
6:8!63:9
(S)
Dubna{DESY
1:0
1:0
�3:2!3:3
(S)
Granada{Lund
2:5�0:4
1:35�0:20
34�18
Montpellier
2:99�0:34
1:70�0:39
25:5�8:4
Taipei
1:5
1:5
7!16
Valencia
1.55
0.92
17�6
O(GF p2) �PT
L�S=12 =
nG8 f
4 h�L�L�i+G27 f
4
�L�23L
�
11+2
3L�21L
�
13
�
+ e2f6GEW h�UyQUio
GR �� GFp2VudV �usgR ; � � �(6�i7)=2 ; L� = �iUyD�U
A0 =p2f�
��G8+
1
9G27
�(M2
K �M2� )�
2
3f2�e
2GEW
�
A2 =2
9f�n5G27 (M
2K �M2
� )� 3f2�e2GEW
o
�0 = �2 = 0
h�(K ! 2�) + �I
iExp
: g8 � 5:1 ; jg27=g8j � 1=18
NC !1: g8 =�35C2 � 2
5C1+ C4
��16L5
�h�i(�)
f3�
�2C6(�)
g27 =35(C2+ C1) ; e2 gEW =�3
�h�i(�)
f3�
�2C8(�)
- Equivalent to standard calculations of Bi
- � dependence only captured for Q6;8
- Good estimate of Im (gI) . Large1NC
corrections
to Re (gI) (Pich { de Rafael '91)
1{Loop �PT
(Kambor et al '90)
� Large enhancement of A0 (� 40{50%)
� �I 6= 0 (still �0 < �0exp)
� Loop correction dominated by infrared
log (M�) terms from �{� loops (FSI)
� O(p4) local terms �xed at NC !1� Not included in Lattice { 1=NC estimates
(�I = 0 at NC !1)
Overlooked in Standard predictions of "0="
Higher Orders ?
FINAL STATE INTERACTIONS
Watson Theorem: AI � A[K ! (��)I ] � AI ei�I
SU(3): AI = (M2K �M2
� ) aI
Omn�es: aI(M2K) = I(M
2K; s0) aI(s0)
I(s; s0) � exp
((s� s0)
�
Zdz
(z � s0)
�I(z)
(z � s� i�)
)
� ei�I(s) <I(s; s0)
� �I(s) = �I(s)j�� below inelastic threshold
� Arbitrary number of subtractions
(n)I(s; s0) = exp
�Pn(s; s0) +
(s� s0)n
�
Zdz
(z � s0)n�I(z)
(z � s� i�)
�
� All{order resummation of infrared chiral logs (same 8n)
� Polynomial ambiguity ) Short{distance information
<0 = 1:55� 0:10 ; <2 = 0:92� 0:03
K ! 2�
AI � A[K ! (��)I ] � AI ei�I = (M2
K �M2�) aI e
i�I
aI(s) = aI(0)n1+ gI(s) +O(p4)
o
g(s) =s
f2
��1� M2
�
2s
��J��(s) +
1
4�JKK(s) +
M2�
18s�J��(s)
+ 4(Lr
5+2Lr
4)(�) +5
4(4�)2
�ln
�2
M2�
� 1
�� 1
4(4�)2lnM2
K
M2�
�
g(8)0 (s) =
s
f2
��1� M2
�
2s
��J��(s) �
1
4
�1�
M2K
s
��JKK(s) +
M2�
18s�J��(s)
+ C85(�) +
3
4(4�)2
�ln
�2
M2�
� 1
�+
1
4(4�)2lnM2
K
M2�
�
g(27)0 (s) =
s
f2
��1� M2
�
2s
��J��(s) �
3
2
�1�
M2K
s
��JKK(s)�
M2�
2s�J��(s)
+ C275 (�)� 1
2(4�)2
�ln
�2
M2�
� 1
�+
3
2(4�)2lnM2
K
M2�
�
g2(s) =s
f2
��12
�1� 2M2
�
s
��J��(s)
+ �C275 (�)� 1
2(4�)2
�ln
�2
M2�
� 1
��
INCLUDING FSI
"0K"K
��110MeVms(2GeV)
�2 �B(1=2)6 (1�IB)� 0:4B
(3=2)8
�
� B(1=2)6
����NC!1
� B(3=2)8
����NC!1
� 1
� B(1=2)6 � B
(1=2)6
����NC!1
� <0 � 1:55
� B(3=2)8 � B
(3=2)8
����NC!1
� <2 � 0:92
� IB � 0:16�<2=<0 � 0:09
(Wolfe{Maltman: 0:08� 0:05)
"0
"= (17� 6)� 10�4
SUMMARY
� �PT � Low{Energy Symmetry Constraints
- Known infrared logarithms
- Unknown chiral couplings
Short Distances
� 1=NC: QCD Matching
Resonance Exchanges
� Omn�es: FSI (elastic unitarity)
Exponentiation of chiral logarithms
� Unitarity: Coupled channels
� Many applications:
- Estimates of chiral couplings
- Hadronic Form Factors / Matrix Elements
- "0="- ms
- KL ! �+��