Photon-photon collisions at the LHC
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Photon-photon collisions at the LHC Lucian Harland-Lang, University - - PowerPoint PPT Presentation
Photon-photon collisions at the LHC Lucian Harland-Lang, University College London UK HEP forum, Coseners House, 3 Nov 2016 1 Outline Motivation: why study collisions at the LHC? Exclusive production: How do we model
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scattering, axion-like particles and massive resonances.
γγ
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p p p
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S(MZ) ∼ 0.1182 ∼ 1
R
X
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R
X
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MX
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X
Q⊥
x2 x1 Seik Senh
p2 p1
fg(x2, · · · ) fg(x1, · · · )
production via QCD (left) and photon
Q ¯ Q
F(x, ) = @G(x, )/@ log 2
(1 z, ~ k?) (z,~ k?)
V (z, k?) V M = J/ , 0, Υ, Υ0, . . .
~
p p W 2
C-even, couples to gluons Couples to photons C-odd, couples to photons + gluons
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. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
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VETO VETO
LHCb defocussed beams) or can veto on additional charged tracks only (already used to select charged - -by ATLAS/CMS/LHCb).
l+l−, W +W −
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E < √s/2
O(100 m)
O(mm)
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220m 215m 204m !IP5 2 new horizontal cylindrical RPs (1 in LS1) 2 horizontal box-shaped RPs
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~5 cm
the right one??
interactions ( ) is high. What about this BG?
∼ 10 ps
INFN, April 2015
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(GeV)
X
M 500 1000 1500 2000 acceptance(%) 10 20 30 40 50 60 70 80 90 100
215m ⊕ p, z=204m ⊕ JJ ⊕ p → pp
σ d=15 σ d=20
simulation CMS-TOTEM
14 TeV, β*=55 cm
X = ξ1ξ2s
MX
d ∼ 200 m MX & 500 GeV
Detectors at under discussion covers .
d ∼ 400 m ⇒ MX ∼ Mh
X
Q⊥
x2 x1 Seik Senh
p2 p1
fg(x2, · · · ) fg(x1, · · · )
production via QCD (left) and photon
Q ¯ Q
F(x, ) = @G(x, )/@ log 2
(1 z, ~ k?) (z,~ k?)
V (z, k?) V M = J/ , 0, Υ, Υ0, . . .
~
p p W 2
C-even, couples to gluons Couples to photons C-odd, couples to photons + gluons
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X
Q⊥
x2 x1 Seik Senh
p2 p1
fg(x2, · · · ) fg(x1, · · · )
production via QCD (left) and photon
Tg(Q2
⊥, µ2) = exp
µ2
Q2
⊥
dk2
⊥
k2
⊥
αs(k2
⊥)
2π 1−∆
Pqg(z)
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KMR-2001
p p
(GeV)
X
M 500 1000 1500 2000 acceptance(%) 10 20 30 40 50 60 70 80 90 100
215m ⊕ p, z=204m ⊕ JJ ⊕ p → pp
σ d=15 σ d=20
simulation CMS-TOTEM
MX & 200 GeV
*Caveat - this is enhancement in initial state only. Of course depends on coupling to produced state.
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b > R1 + R2
Z4 ∼ 5 × 107
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| (rad)
0.1 0.2 0.3 0.4 0.5 0.6 0.7 /50
2 4 6 8 10 12 14 16 18 20 22 p +
c) p
Data SuperCHIC MC (Normalized to data)
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PHYSICS REPORTS (Section C of Physics Letters) 15, no. 4 (1975) 181—282. NORTH-HOLLAND PUBLISHING COMPANY
THE TWO-PHOTON PARTICLE PRODUCTION MECHANISM. PHYSICAL PROBLEMS. APPLICATIONS. EQUIVALENT PHOTON APPROXIMATION V.M. BUDNEV, I.F. GINZBURG, G.V. MELEDIN and V.G. SERBO
USSR Academy of Science, Siberian Division, Institute for Mathematics, Novosibirsk, USSR Received 25 April 1974 Revised version received 5 July 1974
.4 bstract:
This review deals with the physics of two-photon particle production and its applications. Two main problems are discussed
first, what can one find out from the investigation of the two-photon production of hadrons and how, and second, how can the two-photon production of leptons be used?
The basic method for extracting information on the -y-y h (hadrons) transition
the ee
eeh reaction
is discussed in detail.
γγ → X
Weizsacker and Williams (1935)
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n(xi) = 1 xi α π2 Z d2qi⊥ q2
i⊥ + x2 i m2 p
✓ q2
i⊥
q2
i⊥ + x2 i m2 p
(1 − xi)FE(Q2
i ) + x2 i
2 FM(Q2
i )
◆
dLEPA
γγ
dM 2
X dyX
= 1 s n(x1) n(x2)
γγ → X dσpp→pXp dM 2
XdyX
∼ dLEPA
γγ
dM 2
XdyX
ˆ σ(γγ → X) Not exact equality: see later R
X
G2
E(Q2 i ) = G2 M(Q2 i )
7.78 = 1
i /0.71GeV24
FE/FM
Elastic ⇒ steeply falling
23
Point-like proton
ep
n(xi) = 1 xi α π2 Z d2qi⊥ q2
i⊥ + x2 i m2 p
✓ q2
i⊥
q2
i⊥ + x2 i m2 p
(1 − xi)FE(Q2
i ) + x2 i
2 FM(Q2
i )
◆
24
dσpp→pXp dM 2
XdyX
∼ dLEPA
γγ
dM 2
XdyX
ˆ σ(γγ → X)
γγ R
X
25
pp
γγ
pp X
arXiv:0901.3176
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γγ
b⊥
p p
V.A. Khoze, A.D. Martin, M.G. Ryskin, arXiv:1306.2149
soft ∼ 1
S2
soft ∼ 0.7 − 0.9
small model dep.
b⊥ ∼ 1/p⊥
R
X
Q2 ⌧ 1 GeV2
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EUROPEAN ORGANISATION FOR NUCLEAR RESEARCH (CERN)
Submitted to: Phys. Lett. B. CERN-PH-EP-2015-134 18th August 2015
Measurement of exclusive → `+`− production in proton–proton collisions at √s = 7 TeV with the ATLAS detector
The ATLAS Collaboration Abstract
This Letter reports a measurement of the exclusive ! `+` (` = e, µ) cross-section in proton–proton collisions at a centre-of-mass energy of 7 TeV by the ATLAS experiment at the LHC, based on an integrated luminosity of 4.6 fb1. For the electron or muon pairs satisfying exclusive selection criteria, a fit to the dilepton acoplanarity distribution is used to
Variable Electron channel Muon channel p`
T
> 12 GeV > 10 GeV |⌘`| < 2.4 < 2.4 m`+`− > 24 GeV > 20 GeV
SuperChic
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Variable Electron channel Muon channel p`
T
> 12 GeV > 10 GeV |⌘`| < 2.4 < 2.4 m`+`− > 24 GeV > 20 GeV
e+e−
µ+µ−
µ+µ− e+e− σEPA 0.768 0.479 σEPA · hS2i 0.714 0.441 hS2i 0.93 0.92 ATLAS data 0.628 ± 0.032 ± 0.021 0.428 ± 0.035 ± 0.018
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W +W −
γγ → W +W −
extra dimensions….
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]
[GeV
2
Λ /
W
a
0.0001 0.0002 0.0003 0.0004
]
[GeV
2
Λ /
W C
a
0.0005 0.001 0.0015 Standard Model ATLAS 8 TeV 95% CL contour CMS 7 + 8 TeV 95% CL contour ATLAS 8 TeV 95% CL 1D limits
ATLAS
= 8 TeV, 20.2 fb s
+
W → γ γ = 500 GeV
cutoff
Λ
W → lν
]
[GeV
2
Λ /
W
a
0.0005
]
[GeV
2
Λ /
W C
a
0.001 0.002
Standard model 7 TeV 8 TeV 8 + 7 TeV 8 + 7 TeV 1-D limit CMS
(8 TeV)
(7 TeV) + 19.7 fb
5.1 fb
= 500 GeV
cutoff
Λ
γγ p → p∗
arXiv:1604.04464 arXiv:1607.03745
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γ γ γ γ p,Pb p,Pb p,Pb p,Pb
Synopsis: Spotlight on Photon-Photon Scattering
August 22, 2013 Theory suggests that the Large Hadron Collider might be able to detect for the first time the very weak interaction between two photons.
Wikimedia Commons/Brews oharePbPb
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ATLAS NOTE
ATLAS-CONF-2016-111
26th September 2016
Light-by-light scattering in ultra-peripheral Pb+Pb collisions at √sNN =5.02 TeV with the ATLAS detector at the LHC
The ATLAS Collaboration
be 70 ± 20 (stat.) ± 17 (syst.) nb, nb.
0.06 acoplanarity γ γ 0.01 0.02 0.03 0.04 0.05 0.06 Events / 0.005 2 4 6 8 10 12 14 Preliminary ATLAS = 5.02 TeV
NN
s Pb+Pb < 2 GeV
γ γ T
p = 0
trk
N
b µ Data, 480 MC γ γ → γ γ MC
+
e → γ γ MC γ γ CEP
~ v −c em−fields em−fields ~ v c ~ ~ Pb Pb
L = 480 µb−1
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a Pb Pb Pb Pb γ γ Ze Ze
36 pb1 ATLAS, 3γ 1 n b1 1 n b
OPAL, 3γ
5 20 40 60 80 100 ma (GeV) 105 104 103 1/Λ (GeV1)
ATLAS, 2γ Beam Dump OPAL, 2γ
aF e F coupling
1 00 1 0−1 1 0−2
linear p-p ps = 7 TeV Pb-Pb psNN = 5.5 TeV
La = 1 2(@a)2 − 1 2m2
aa2 − 1
4 a ΛF e F ,
γγ → γγ
10 20 30 40 50
mγγ (GeV)
10−1 100 101 102
√sNN = 5.5 TeV
ma = 15 GeV ma = 40 GeV LBL Fakes Brem
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23
KMR-2001
p p
R
qq (WW...)
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|A+|2 ∼ |p1⊥ · p2⊥|2 ∼ cos2 , |A−|2 ∼ |✏αβµν pα
1pβ 2pµ 1⊥pν 2⊥|2 ∼ sin2
+/−
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0.002 0.004 0.006 0.008 0.5 1 1.5 2 2.5 3
dσ dφ , arbitrary units, 0+
φ
bare screened 0.002 0.004 0.006 0.008 0.5 1 1.5 2 2.5 3
dσ dφ , arbitrary units, 0−
φ
bare screened
40
∼ 11 fb−1
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CERN-PH-LPCC-2015-001 SLAC-PUB-16364 DESY 15-167 September 3 2015
LHC Forward Physics
Editors: N. Cartiglia, C. Royon The LHC Forward Physics Working Group
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Leading lepton vertex z position [cm]
5 10 15 20 25
Δ ToF
0.2 0.4 0.6 0.8 1 Inclusive WW background
simulation CMS-TOTEM
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]
[GeV
2
Λ /
W
a
0.2 0.4 0.6 0.8
10 ×
]
[GeV
2
Λ /
W c
a
0.0005 0.001 0.0015 0.002
=10 ps σ , 13 TeV,
100fb =30 ps σ , 13 TeV,
100fb = 500 GeV
cutoffΛ , 7 TeV,
5fb
simulation CMS-TOTEM
e) µ ( φ Δ 0.5 1 1.5 2 2.5 3
Events / 100fb 10 20 30 40 50
, SM
+
W → γ γ , SM
+
W → γ γ misreconstructed x10
+
τ → γ γ
+
Inclusive W = 0
2
Λ /
W C
, a
GeV
= 5*10
2
Λ /
W
, a
+
W → γ γ
simulation CMS-TOTEM
aW
0 /Λ2 = 2 × 10−6
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R
γ(x1, µ2) γ(x2, µ2)
46
σ per bin [pb] W+W- production at FCC-hh 100 TeV
|η(W±)|<4 Lepton PDF from evolution and initial prior
(apfel_nn23qednlo0118_lept) Tot. qq
ℓ+ℓ-
10-10 10-9 10-8 10-7 10-6 10-5 10-4 10-3 10-2 10-1 100
MadGraph5_aMC@NLO
[%]
Relative contribution
10 100 [%] m(W+W-) [GeV]
PDF uncertainty (68% CL) per channel
1 10 100 5000 7500 10000 12500 15000 17500 20000
m(tt
−0.15 0.15 500 1000 1500 2000 2500 3000 3500 4000
EW/LO QCD; PDF unc.
m(tt
CT14 0.00 CT14 0.14 µ=mt
−0.15 0.15 500 1000 1500 2000 2500 3000 3500 4000
EW/LO QCD; PDF unc.
tt
tt
arXiv:1606.01915
arXiv:1607.01831
γγ
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quark and gluons. Freely parametrise and fit to DIS and some LHC data. Uncertainties (so far) remain large.
W, Z
γ(x, Q0)
photon emission from quarks. Compare/fit to ZEUS isolated photon DIS.
x*PDF x Q = 3.2 GeV CT0.00 CT0.14 MRST0 MRST1 NNPDF23 0.02 0.04 0.06 0.08 0.1 10-5 10-4 10-3 10-2 10-1
arXiv:1509.02905
reveals apparently large uncertainties. However: have we included all
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p p
R
X
49
DGLAP evolution
p
(Low scale) ‘incoherent’ emission.
Elastic emission
p p
≡
X
50
γ(x, µ2) = γ(x, Q2
0) +
Z µ2
Q2
α(Q2) 2π dQ2 Q2 Z 1
x
dz z ✓ Pγγ(z)γ(x z , Q2) + X
q
e2
qPγq(z)q(x
z , Q2) + Pγg(z)g(x z , Q2) ◆ ,
γ(x, Q2
0) = γcoh(x, Q2 0) + γincoh(x, Q2 0) ,
γevol
Q0 ∼ 1 GeV
A.D. Martin, M.G. Ryskin, arXiv:1406.2118
R
X
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high mass, semi-exclusive processes, and diphoton resonance production.
LHL, V.A. Khoze, M.G. Ryskin, arXiv:1601.03372, 1601.07187, 1607.4635
RIP
understood coherent emission ( ).
quarks (with well constrained PDFs).
Q2 . 1 GeV2 Q2 & 1 GeV2
production, while taking simple model for (low scale) incoherent. Sufficient to give some fairly dramatic results w.r.t. previous studies.
p p p
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10−6 10−4 10−2 100 102 104 100 1000
dL d ln M2
X , √s = 13 TeV
MX [GeV]
γγ - this work γγ - NNPDF gg qq qq 10−6 10−4 10−2 100 102 104 100 1000 10000
dL d ln M2
X , √s = 100 TeV
MX [GeV]
γγ - this work γγ - NNPDF gg qq qq
arXiv:1607.04635
q, g
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0.0001 0.001 0.01 0.1 1 10 100 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5
dσ/Mll [fb/TeV], √s = 13 TeV Mll [TeV]
γγ - NNPDF γγ - this work DY 1e-05 0.0001 0.001 0.01 0.1 1 6 8 10 12 14 16 18 20
dσ/Mll [fb/TeV], √s = 100 TeV Mll [TeV]
γγ - NNPDF γγ - this work DY
arXiv:1607.04635
Mll γγ γγ . 10%
54
0.01 0.1 1 10 100 1000 10000 100000 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5
dσ/MW W [fb/TeV], √s = 13 TeV MW W [TeV]
γγ - NNPDF γγ - this work QCD 0.01 0.1 1 10 100 6 8 10 12 14 16 18 20
dσ/MW W [fb/TeV], √s = 100 TeV MW W [TeV]
γγ - NNPDF γγ - this work QCD
W +W −
arXiv:1607.04635
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0.8 0.85 0.9 0.95 1 1.05 0.2 0.4 0.6 0.8 1 GE/Gstd.dipole (b)
A1 Collaboration, arXiv:1307.6227
p p
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CERN-TH/2016-155
How bright is the proton? A precise determination of the photon PDF
Aneesh Manohar,1, 2 Paolo Nason,3 Gavin P. Salam,2, ∗ and Giulia Zanderighi2, 4
1Department of Physics, University of California at San Diego, La Jolla, CA 92093, USA 2CERN, Theoretical Physics Department, CH-1211 Geneva 23, Switzerland 3INFN, Sezione di Milano Bicocca, 20126 Milan, Italy 4Rudolf Peierls Centre for Theoretical Physics, 1 Keble Road, University of Oxford, UK
proton neutral lepton l (massless) heavy neutral lepton L (mass M)
ν Lµν(k, q)]
Wµν(p, q)
STEP 1
work out a cross section (exact) in terms of F2 and FL struct. fns.
hadronic tensor, known in terms of F2 and FL
xfγ/p(x, µ2) = 1 2πα(µ2) Z 1
x
dz z ( Z
µ2 1−z x2m2 p 1−z
dQ2 Q2 α2(Q2) " zpγq(z) + 2x2m2
p
Q2 ! F2(x/z, Q2) z2FL ⇣x z , Q2⌘ # α2(µ2)z2F2 ⇣x z , µ2⌘ ) , (6)
F2 FL LUXqed
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10−6 10−4 10−2 100 102 104 106 108 100 1000
dL d ln M2
X , √s = 13 TeV
MX [GeV]
γγ - this work γγ - NNPDF γγ - LUXqed gg qq qq 10−8 10−6 10−4 10−2 100 102 104 106 108 100 1000 10000
dL d ln M2
X , √s = 100 TeV
MX [GeV]
γγ - this work γγ - NNPDF γγ - LUXqed gg qq qq
See backup for more details
γγ MX Q2
58
yLRG yX yq yp
| {z }
δ
CERN-EP/2016-073 2016/09/09
CMS-FSQ-13-008
Evidence for exclusive γγ ! W+W production and constraints on anomalous quartic gauge couplings in pp collisions at ps = 7 and 8 TeV
The CMS Collaboration⇤
EUROPEAN ORGANISATION FOR NUCLEAR RESEARCH (CERN)
DOI: 10.1103/PhysRevD.94.032011 CERN-EP-2016-123 September 6, 2016
Measurement of exclusive γγ → W+W− production and search for exclusive Higgs boson production in pp collisions at √s = 8 TeV using the ATLAS detector
59
p → pγ
γγ γγ sγγ γγ
60
γ(x, µ2) = γ(x, Q2
0) +
Z µ2
Q2
α(Q2) 2π dQ2 Q2 Z 1
x
dz z ✓ Pγγ(z)γ(x z , Q2) + X
q
e2
qPγq(z)q(x
z , Q2) + Pγg(z)g(x z , Q2) ◆ , Pγγ
61
NLO in QCD
Pγγ(z) ∼ δ(1 − z)
62
γ(x, µ2) = γ(x, Q2
0) Sγ(Q2 0, µ2) +
Z µ2
Q2
α(Q2) 2π dQ2 Q2 Z 1
x
dz z ✓ X
q
e2
qPγq(z)q(x
z , Q2) + Pγg(z)g(x z , Q2) ◆ Sγ(Q2, µ2) ,
z ◆ ≡ γin(x, µ2) + γevol(x, µ2)
γin(x, µ2) Q2 < Q2
0 ∼ 1 GeV2
γevol(x, µ2)
Sγ(Q2
0, µ2) = exp
−1 2 Z µ2
Q2
dQ2 Q2 α(Q2) 2π Z 1 dz X
a=q, l
Paγ(z) !
Q2 µ2 Sγ(Q2
0, µ2)
µ
63
10
10
10 1 )
2
(x,Q γ x 0.02 0.04 0.06 0.08 0.1 ATLAS ATLAS
2
GeV
4
= 10
2
Q
NNPDF2.3qed 68% CL NNPDF2.3qed + ATLAS high-mass DY data MRST2004qed, current quark mass MRST2004qed, constituent quark mass CT14qed 68% CL
0.5 1 0.01 0.1 1e-05 0.0001 0.001 0.01 0.1 xγ(x, µ = 100 GeV)
x
coh. incoh. evol. Tot. NNPDF3.0
Mll < 1500 GeV
x x ↓
64
Q2
Q2 < Q2 Q2 > Q2
∼ 1 GeV2
Q2 > Q2
xfγ/p(x, µ2) = 1 2πα(µ2) Z 1
x
dz z ( Z
µ2 1−z x2m2 p 1−z
dQ2 Q2 α2(Q2) " zpγq(z) + 2x2m2
p
Q2 ! F2(x/z, Q2) z2FL ⇣x z , Q2⌘ # α2(µ2)z2F2 ⇣x z , µ2⌘ ) , (6)
ln µ2/Q2
Q2 m2
p
xfγ/p(x, µ2) → x Z 1
x
dz z Z µ2
Q2
dQ2 Q2 α(Q2) 2π α(Q2) α(µ2) pγq(z) X e2
q q
⇣x z , Q2⌘ ,
αS
LL Cutoff
65
Sγ(Q2
0, µ2) = exp
−1 2 Z µ2
Q2
dQ2 Q2 α(Q2) 2π Z 1 dz X
a=q, l
Paγ(z) !
xfγ/p(x, µ2) = x Z 1
x
dz z Z µ2
Q2
dQ2 Q2 α(Q2) 2π α(Q2) α(µ2) Pγq(z) X e2
q q
⇣x z , Q2⌘ , Pγγ
γ(x, µ2) = γ(x, Q2
0) Sγ(Q2 0, µ2) +
Z µ2
Q2
α(Q2) 2π dQ2 Q2 Z 1
x
dz z ✓ X
q
e2
qPγq(z)q(x
z , Q2) + Pγg(z)g(x z , Q2) ◆ Sγ(Q2, µ2) ,
α(Q2)/α(µ2)
α
Sγ(Q2, µ2) = α(Q2) α(µ2) + O(α) Q2 > Q2
γ
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0.005 0.01 0.015 0.02 0.025 0.0001 0.001 0.01 0.1
xγ(x, Q2
0 = 2 GeV2)
x
Radiative ansatz Low Q2 < Q2
0 continuum
Resonance contribution Resonance + Continuum 1e-05 0.0001 0.001 0.01 0.0001 0.001 0.01 0.1
xγ(x, Q2
0 = 2 GeV2)
x
Radiative ansatz Low Q2 < Q2
0 continuum
Resonance contribution Resonance + Continuum
and similar in shape.
at higher .
‘Christy-Bosted’ fit
W 2 ∼ Q2/x
x ∼ Q0
Q2
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0.6 0.8 1 1.2 1.4 0.0001 0.001 0.01 0.1
xγHKR/xγLUX , µ = 100 GeV x
HKR HKR (incoh. LUX)
µ = 100 GeV
γincoh = 0 x x ↑
O(%)
68
0.6 0.8 1 1.2 1.4 0.0001 0.001 0.01 0.1
xγHKR/xγLUX , µ = 100 GeV x
HKR HKR (incoh. LUX)
Q2
γ(x, Q2
0)