Studying the gluon and charm content of the deuteron Nodoka - - PowerPoint PPT Presentation

studying the gluon and charm content of the deuteron
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Studying the gluon and charm content of the deuteron Nodoka - - PowerPoint PPT Presentation

3mm JSPS16-17_01_.indd 1 2016/12/01 8:36:38 Studying the gluon and charm content of the deuteron Nodoka Yamanaka (IPN Orsay) In collaboration with 2018/05/15 S. J. Brodsky (SLAC), K. Y.-J. Chiu (SLAC),


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SLIDE 1

Studying the gluon and charm content of the deuteron

2018/05/15 Light-Cone2018 Jefferson Lab

Nodoka Yamanaka (IPN Orsay)

背厚3mm

JSPS16-17_01_表紙(英).indd 1 2016/12/01 8:36:38

In collaboration with

  • S. J. Brodsky (SLAC), K. Y.-J. Chiu (SLAC),

and J.-P. Lansberg (IPN Orsay)

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SLIDE 2

Introduction

Why the deuteron?

The simplest nucleus Well-known in nuclear physics ⇒ Quantify nuclear effect Minimal nuclear effect ⇒ Extract neutron PDF E.g. : used in the EMC ratio Build a base to extend to heavier nuclei The gluon and charm content of the deuteron may be studied with future fixed-target experiments at the LHC (c.f AFTER@LHC) Gluon PDF of 4He for cosmic ray reaction with interstellar matter Required from astrophysics: Charm PDF of atmospheric nuclei (14N,16O) for the study

  • f high energy (prompt) neutrino

In particular, the high-x region PDF near the endpoint is predicted in perturbative QCD : e.g. gluon PDF in deuteron Gd(x) ∝ (2 − x)11

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SLIDE 3

Kinematic coverage of bottomonium prod. at AFTER@LHC

(Fixed target mode of LHCb)

x1 << x2 x1 x2 Hadron center-of-mass Target rest frame x1 x2

θ semi-large

Let us estimate up to which x LHCb can cover with Upsilon production off pp Production threshold at CM: Kinematics of Upsilon production:

Can access up to “x” = 1.4 with LHCb in the fixed-target mode

LHCb rapidity coverage: [2,5]Lab frame = [-2.8,0.2]c.m.s.

(√s = 115GeV for fixed-target)

x1,2 = mb¯

b

√s e±yc.m.s.

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x1x2s = m2

b¯ b

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SLIDE 4

Prospects for astrophysics (2 important cases)

Interstellar reactions Atmospheric neutrinos productions

PAMELA, AMS-02, DAMPE, … Cosmic ray sources

  • f high energy protons

(acceleration, dark matter,…)

p

4He

Primary CR Secondary CR

NASA, AMS-02

In high energy reactions, low-x is important

14N

High energy cosmic protons from space Hard reactions with interstellar matter (mostly p and 4He)

D Λc

Atmospheric nuclei Charmed hadrons Prompt neutrinos IceCube

High energy hadrons are produced from high-x charm quarks

⇒ Gluons !

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SLIDE 5

Chiral effective field theory description of nuclear PDF

(a) (b)

Leading contribution to nuclear PDF in chiral EFT :

hxnig|A = hxnig[A + hA|αn(N †N)2|Ai]

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Impulse approximation

J.-W. Chen and W. Detmold, PLB625 (2005) 165

(b) : Nucleon-nucleon correlation effect : subleading in chiral EFT (a) : Impulse approximation ⇒ Leading effect in chiral EFT (≒ velocity expansion) connected to quark EMC effect, but unknown for gluons Long-range correlation (pion-exchange current) : O(v3) effect ⇒ Small Moments of the PDF can be expanded in terms of the nucleon velocity:

hxnig|A = vA,µ0 · · · vA,µnhA|Oµ0···µn

g

|Ai

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  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

  • L. B. Weinstein et al., PRL 106, 052301 (2011)

J.-W. Chen et al., PRL 119, 262502 (2017) J.-W. Chen and W. Detmold, PLB625 (2005) 165

Short-range correlation :

slide-6
SLIDE 6

Nonrelativistic deuteron wavefunction

Calculate deuteron wave function in nonrelativistic nuclear physics . We use the phenomenological nuclear force Av18.

0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 1 2 3 4 5 6

ψ(r) r(fm)

S-wave D-wave

Radial wavefunction of deuteron

We solve the Schroedinger equation with the Gaussian expansion method

  • R. B. Wiring et al., Phys. Rev. D 51, 38 (1995).
  • E. Hiyama et al., Prog. Part. Nucl. Phys. 51, 223 (2003).
  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

Basis of wavefunction is a superposition of Gaussians: Φnlm(r) = Nnlrle−νnr2Ylm(ˆ r)

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With sufficient number of basis functions (n), the Schroedinger eq. can be solved with high precision (10-10)

Solve Schroedinger eq. by variational principle, numerical diagonalization of Hamiltonian

(truncate with finite n)

slide-7
SLIDE 7

Conversion from rest-frame to light-front-frame

0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 1 2 3 4 5 6

ψ(r) r(fm)

S-wave D-wave

⇒ Here we use the Recipe of Terentev

  • M. V. Terentev, Sov. J. Nucl. Phys. 24 (1976) 106. [Yad. Fiz.24,207(1976)]
  • H. Merabet et al, Phys. Lett. B 307, 177 (1993)

P . Hoyer and S. Peigne, Phys. Rev. D 61, 031501 (2000)

  • J. Hufner, Yu. P

. Ivanov, B. Z. Kopeliovich, Phys. Rev. D 62, 094022 (2000)

  • B. Kopeliovich, A. Tarasov, J. Hufner, Nucl. Phys. A 696, 669 (2001)

Radial WF Cylindrical WF (momentum-space)

0.001 0.002 0.003 0.004 0.005 0.006 0.007 0.008 0.009 0.01 50 100 150 200 250 300 350 400

P(pz) pz(MeV)

Deuteron Deuteron (S-wave only) Heavy nucleus 2 4 6 8 10 0.5 1 1.5 2

NN/A(z) z

Deuteron Heavy nucleus

FT

LF distribution of nucleon

Fold with nucleon PDF (GRV98, CJ15)

PDF of deuteron

ψ(p⊥, z) = r ∂pz(p⊥, z) ∂z ψ(p⊥, pz)

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pz = (z − 1) s m2

N + p2 ⊥

z(2 − z)

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  • M. Glueck, E. Reya, and A.Vogt, Eur. Phys. J. C 5, 461 (1998)
  • A. Accardi et al., Phys. Rev. D 93, 114017 (2016)
  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

Project the wavefunction to the z-axis and Fourier transform Conversion from rest- to light-front-frame is ambiguous (not a Lorentz boost) Convert pz to momentum fraction

slide-8
SLIDE 8

Region of applicability

Our framework is based on velocity expansion : nucleon should be nonrelativistic 0-th moment of PDF cancels, 1st moment is small

10-2 10-1 100 0.5 1 1.5 2

< v2> (x) x

Nucleon < v2> (GRV98, µF=1GeV)

We expect our framework to be applicable for 0 < x < 1.1 and to break down for x > 1.5 since <v2> > 1

Let us take <v2> < 0.3 to be conservative

Velocity distribution of nucleon in terms of gluon x

  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

To examine the validity, we inspect the average velocity in function of x (gluon) We solve <v2> in the function of x Strict limit of applicability (v < 1) : x < 1.5

  • A. S. Rinat and M. F

. Taragin, PRC 72, 065209 (2005)

The important corrections start from O(v2)

slide-9
SLIDE 9

Result (gluon PDF)

Gluon PDF:

10-5 10-4 10-3 10-2 10-1 100 101 102 103

G(x)

Gd(x) (GRV98, µF=1GeV) Gp(x) (GRV98, µF=1GeV)

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

Gd(x)/2Gp(x) x

Ratio deuteron/proton

We use GRV98 for proton PDF (behaves well near x=1)

  • M. Glueck et al., Eur. Phys. J. C 5, 461 (1998).
  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

slide-10
SLIDE 10

Result (gluon PDF)

Gluon PDF:

10-5 10-4 10-3 10-2 10-1 100 101 102 103

G(x)

Gd(x) (GRV98, µF=1GeV) Gp(x) (GRV98, µF=1GeV)

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

Gd(x)/2Gp(x) x

Ratio deuteron/proton

Fermi motion

We use GRV98 for proton PDF (behaves well near x=1)

  • M. Glueck et al., Eur. Phys. J. C 5, 461 (1998).
  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

slide-11
SLIDE 11

Result (gluon PDF)

Gluon PDF:

10-5 10-4 10-3 10-2 10-1 100 101 102 103

G(x)

Gd(x) (GRV98, µF=1GeV) Gp(x) (GRV98, µF=1GeV)

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

Gd(x)/2Gp(x) x

Ratio deuteron/proton

Fermi motion

We use GRV98 for proton PDF (behaves well near x=1)

Small EMC effect?

  • M. Glueck et al., Eur. Phys. J. C 5, 461 (1998).
  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

slide-12
SLIDE 12

Result (gluon PDF)

Gluon PDF:

10-5 10-4 10-3 10-2 10-1 100 101 102 103

G(x)

Gd(x) (GRV98, µF=1GeV) Gp(x) (GRV98, µF=1GeV)

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

Gd(x)/2Gp(x) x

Ratio deuteron/proton

Fermi motion

We use GRV98 for proton PDF (behaves well near x=1)

Small EMC effect? Antishadowing?

  • M. Glueck et al., Eur. Phys. J. C 5, 461 (1998).
  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

slide-13
SLIDE 13

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV)

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (CJ15)

Result (charm PDF)

Charm: We use CJ15 for proton PDF (charm PDF available)

  • A. Accardi et al., Phys. Rev. D 93, 114017 (2016).
  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

slide-14
SLIDE 14

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV)

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (CJ15)

Result (charm PDF)

Charm:

Fermi motion

We use CJ15 for proton PDF (charm PDF available)

  • A. Accardi et al., Phys. Rev. D 93, 114017 (2016).
  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

slide-15
SLIDE 15

Intrinsic charm

u u d c ¯ c

Gluon splitting:

Distribution similar to gluon PDF (3 diagrams)

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV)

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (CJ15)

Charm:

slide-16
SLIDE 16

Intrinsic charm

u u d c ¯ c

Gluon splitting:

Distribution similar to gluon PDF (3 diagrams)

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV)

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (CJ15)

u u d c ¯ c

Intrinsic charm:

More important than gluon splitting at large x (3 diagrams)

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV) Intrinsic charm PDF of proton folded by deuteron Intrinsic charm PDF in proton

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (intrinsic) Ratio deuteron/proton (CJ15)

  • S. J. Brodsky, P

. Hoyer, C. Peterson, N. Sakai, PLB93 (1980) 451.

Charm:

slide-17
SLIDE 17

Intrinsic charm

u u d c ¯ c

Gluon splitting:

Distribution similar to gluon PDF (3 diagrams)

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV)

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (CJ15)

u u d c ¯ c d d u u d d d u u c ¯ c (a) (b)

Hidden color configuration of deuteron:

Further enhanced at large x compared to the intrinsic charm nucleon PDF but may be enhanced by combinatoric factors (compare the number of diagrams) Normalization not known, This enhancement is potentially important in astrophysics!

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV) Intrinsic charm PDF of proton folded by deuteron Intrinsic charm PDF in proton Intrinsic charm PDF in deuteron

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (intrinsic) Ratio deuteron/proton (CJ15)

(15 diagrams) (20 diagrams)

Hidden color conf.

  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

u u d c ¯ c

Intrinsic charm:

More important than gluon splitting at large x (3 diagrams)

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV) Intrinsic charm PDF of proton folded by deuteron Intrinsic charm PDF in proton

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (intrinsic) Ratio deuteron/proton (CJ15)

  • S. J. Brodsky, P

. Hoyer, C. Peterson, N. Sakai, PLB93 (1980) 451.

Charm:

slide-18
SLIDE 18

Intrinsic charm

u u d c ¯ c

Gluon splitting:

Distribution similar to gluon PDF (3 diagrams)

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV)

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (CJ15)

u u d c ¯ c d d u u d d d u u c ¯ c (a) (b)

Hidden color configuration of deuteron:

Further enhanced at large x compared to the intrinsic charm nucleon PDF but may be enhanced by combinatoric factors (compare the number of diagrams) Normalization not known, This enhancement is potentially important in astrophysics!

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV) Intrinsic charm PDF of proton folded by deuteron Intrinsic charm PDF in proton Intrinsic charm PDF in deuteron

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (intrinsic) Ratio deuteron/proton (CJ15)

(15 diagrams) (20 diagrams)

Hidden color conf.

  • S. J. Brodsky, K.Y

.J. Chiu, J.P . Lansberg, NY , arXiv:1805.03173 [hep-ph]

u u d c ¯ c

Intrinsic charm:

More important than gluon splitting at large x (3 diagrams)

10-10 10-8 10-6 10-4 10-2 100 102 104

fc(x)

Charm PDF in deuteron (CJ15, µF=3GeV) Charm PDF in proton (CJ15, µF=3GeV) Intrinsic charm PDF of proton folded by deuteron Intrinsic charm PDF in proton

0.9 0.95 1 1.05 1.1 0.2 0.4 0.6 0.8 1

fc/d(x)/2fc/N(x) x

Ratio deuteron/proton (intrinsic) Ratio deuteron/proton (CJ15)

  • S. J. Brodsky, P

. Hoyer, C. Peterson, N. Sakai, PLB93 (1980) 451.

Charm:

slide-19
SLIDE 19
  • We have studied the gluon and charm PDF of the

deuteron with nonrelativisitic inputs.

  • Chiral EFT suggests the validity of our nonrelativistic

framework in the region 0 < x < 1.1.

  • The gluon PDF of the deuteron shows Fermi motion at

x > 0.6, and a small EMC effect at x~0.4.

  • Hidden color may enhance the charm PDF of deuteron

in the high-x region : may be important in astrophysics. Summary

Future subjects:

  • Studies of NN correlation required for quantitative

analysis.

  • Normalization of hidden color states to be fixed.
  • Extension to heavier nuclei is on-going : stay tuned.
slide-20
SLIDE 20

Backup

slide-21
SLIDE 21

1st moments of nuclear PDF

  • A. S. Rinat and M. F

. Taragin, Phys. Rev. C 72, 065209 (2005).

Deuteron Difference between PDF of single nucleon and nuclear PDF (per nucleon) The 1st moments are much smaller than 1