Neutral Current Weak Form Factors & Neutrino Scattering
Raza Sabbir Sufian
USQCD All Hands’ Meeting 2018
Neutral Current Weak Form Factors & Neutrino Scattering Raza - - PowerPoint PPT Presentation
Neutral Current Weak Form Factors & Neutrino Scattering Raza Sabbir Sufian USQCD All Hands Meeting 2018 Neutrino-Nucleon Neutral Current Elastic Scattering ( q 1 , 1 ) ( q 2 , 2 ) + p + p Z 0 ( q ) + p +
USQCD All Hands’ Meeting 2018
Matrix element in V-A structure of leptonic current
ν + p → ν + p ¯ ν + p → ¯ ν + p,
M = i 2 p 2GF ¯ ν(q2)γµ(1 γ5)ν(q1) | {z }
leptonic current
hN(p2)|Jµ
Z|N(p1)i
| {z }
hadronic current
.
Z0(q) ν(q1, σ1) ν(q2, σ2) N(p1, κ1) N(p2, κ2)
hN(p2)| Jµ
Z |N(p1)i = ¯
u(p2)[F Z
1 (Q2) + F Z 2 (Q2)iσµνqν
2MN + F Z
A (Q2)γµγ5]u(p1)
d dQ2 G2
F
2 Q2 E2
W 4E=Mp ;
A 1
4fGZ A21FZ 1 2 FZ 2 214FZ 1 FZ 2 g;
B 1
4GZ AFZ 1 FZ 2 ;
C 1 64 GZ
A2 FZ 1 2 FZ 2 2:
Neutral Weak Dirac & Pauli FFs Weak axial FF
F Z,p
1,2 =
✓1 2 sin2 θW ◆ (F p
1,2(Q2) F n 1,2(Q2)) sin2 θW(F p 1,2 + F n 1,2) F s 1,2
2
Ye, Arrington, Hill, Lee
RSS, Yang, Alexandru, Draper, Liang, Liu
PL B 777 (2018) 8-15 PRL 118, 042001 (2017)
Strange EMFF from Lattice QCD
Physical point 4 lattice spacings 3 volumes
PRD 95, 014011(2017) RSS, de Teramond, Brodsky, Dosch, Deur
Strange EMFF Nucleon EMFF (total)
PRL 2018 de Teramond, Liu, RSS, Brodsky, Dosch, Deur
ffiffiffi
PRD 96, 093007 (2017) RSS
Radiative corrections for e-p scattering
GZ,p(n)
E,M (Q2) = 1
4 (1−4 sin2 ✓W )(1+Rp(n)
V
)Gγ,p(n)
E,M (Q2)
−(1+Rn(p)
V
)Gγ,n(p)
E,M (Q2)− Gs E,M(Q2)
*Use MiniBooNE data (0.27 < Q2 < 0.65 GeV2)
Reason 1: Uncertainty in GsE,M becomes very large and values consistent with zero
Reason 2: Nuclear effect can be large for at low Q2
C ~ 1
GZA (0) = - 0.751 (56) Mdipole = 0.95(6) GeV
dσ dQ2 From MiniBooNE Experiment
)(F p
1,2
− F n
1,2)}
From Experiment
1,2
From Lattice QCD
In preparation with Keh-Fei Liu & David Richards
(??)
(0))Gs E,M(
(0))Gs E,M(
X
BNL E734 data was NOT used in the analysis Nuclear effects Pauli blocking & nuclear shadowing at Q2 < 0.15 GeV2
GZ
A 1 2GCC A Gs A;
Gs
A(0)
GZ
A(0) = −0.751(56)
GCC
A (0) = 1.2723(23)
MiniBooNE, PRD 82 (2010) Gs
A(0) = 0.08(26)
BNL E734, PRC 48 (1993)
0.1 0.2 0.3 0.4 0.5 mπ (GeV) −0.18 −0.16 −0.14 −0.12 −0.10 −0.08 −0.06 −0.04 −0.02 0.00 gs
A
QCDSF Engelhardt ETMC CSSM and QCDSF/UKQCD LHPC χQCD Phenomenology (JAM15) Phenomenology (JAM17) Phenomenology (NNPDFpol1.1)
From Jeremy Green’s Talk
Gs
A(0) = - 0.21(10)
Precise estimate of NC weak axial form factor GZA
Strange quark contribution cannot be ignored
Reconstruction of (anti)neutrino- nucleon diff. cross sections with correct prediction of GZA and lattice input of GsE,M
Lattice QCD calculation of GsA in the continuum and infinite volume limit with controlled systematic uncertainties required
Many models of meson-baryon fluctuations to study s(x)-s(x) asymmetry
In Preparation
EPJ Web Conf. 66 (2014) 06018
0.2 0.4 0.6 0.8 1 0.2 0.4 0.6 0.8 1
0.5
0.5
s A
G
0.2 0.4 0.6 0.8 1 0.2 0.4 0.6 0.8 1
0.2 0.4
0.2 0.4
s M
G
)
2(GeV
2Q 0.2 0.4 0.6 0.8 1 0.2 0.4 0.6 0.8 1
0.2
0.2
s E
G
Pate, et al
TABLE II. Two solutions for the strange form factors at Q2 0:5 GeV2 produced from the E734 and HAPPEX data. Solution 1 Solution 2 Gs
E
0:02 0:09 0:37 0:04 Gs
M
0:00 0:21 0:87 0:11 Gs
A
0:09 0:05 0:28 0:10
[13] S.F. Pate, Phys. Rev. Lett. 92, 082002 (2004), [14] D. Armstrong, R. McKeown, Ann.Rev.Nucl.P
Q2 = 0.5 GeV2
Ap
PV = − GF Q2
4 √ 2πα 1 [(Gp
E)2 + τ(Gp M)2]
× {((Gp
E)2 + τ(Gp M)2)(1 − 4 sin2 θW )(1 + Rp V )
− (Gp
EGn E + τGp MGn M)(1 + Rn V )
− (Gp
EGs E + τGp MGs M)(1 + R(0) V )
− ′(1 − 4sin2θW )Gp
MGe A} ,
(2 with τ = Q2 4M 2
p
, =
2 −1 , ′ =
RT =1
A
RT =0
A
R(0)
A
−0.172 −0.253 −0.551 many-quark −0.086(0.34) 0.014(0.19) N/A total −0.258(0.34) −0.239(0.20) −0.55(0.55)
0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8
0.5
Ge,(T =1)
A
Q2 (Ge V/ c
2)
G0 A4 Zhu et al. SAMPLE
Particle Lifetime (ns) Decay mode Branching ratio (%) π+ 26.03 µ+ + νµ 99.9877 e+ + νe 0.0123 K+ 12.385 µ+ + νµ 63.44 π0 + e+ + νe 4.98 π0 + µ+ + νµ 3.32 K0
L
51.6 π− + e+ + νe 20.333 π+ + e− + νe 20.197 π− + µ+ + νµ 13.551 π+ + µ− + νµ 13.469 µ+ 2197.03 e+ + νe + νµ 100.0
νµ + n → µ− + p , ¯ νµ + p → µ+ + n , νe + n → e− + p , ¯ νe + p → e+ + n .
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