Form Factors with Electrons and Positrons Factors with Electrons and Positrons HUGS2013, JLab, May...

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Form Factors with Electrons and Positrons HUGS2013, JLab, May 28 – June 14, 2013 Michael Kohl Hampton University, Hampton, VA 23668 Jefferson Laboratory, Newport News, VA 23606 Part 2: Proton form factor measurements

Transcript of Form Factors with Electrons and Positrons Factors with Electrons and Positrons HUGS2013, JLab, May...

Page 1: Form Factors with Electrons and Positrons Factors with Electrons and Positrons HUGS2013, JLab, May 28 – June 14, 2013 ... Bohr, Sommerfeld: Atomic shell model " ... “In a given

Form Factors with Electrons and Positrons

HUGS2013, JLab, May 28 – June 14, 2013

Michael Kohl

Hampton University, Hampton, VA 23668 Jefferson Laboratory, Newport News, VA 23606

Part 2: Proton form factor measurements

Page 2: Form Factors with Electrons and Positrons Factors with Electrons and Positrons HUGS2013, JLab, May 28 – June 14, 2013 ... Bohr, Sommerfeld: Atomic shell model " ... “In a given

General scattering A + B → C + D 2

  Fermi’s Golden Rule

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Lorentz invariants 3

Energy transfer

Bjorken scaling var.

Inelasticity

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LAB frame kinematics 4

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LAB frame kinematics 5

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LAB frame kinematics 6

,

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CM frame kinematics 7

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CM frame kinematics 8

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Lepton-lepton scattering 9

  Lepton-lepton scattering (Feynman, Dirac):

  Unpolarized scattering cross section:

  The matrix element accounts for the strength of the interaction α = 2πe2/hc = 1/137, higher orders suppressed by powers of α

One-photon exchange approximation (Born approximation)

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Lepton-lepton scattering 10

  Matrix element: average over initial, sum over final spins

(ERL)

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Lepton-lepton scattering 11

  Matrix element: average over initial, sum over final spins

  Dirac cross section (pointlike spin-1/2 target)

(ERL)

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Lepton-lepton scattering 12

  Matrix element: average over initial, sum over final spins

  Dirac cross section (pointlike spin-1/2 target)

  Mott cross section (pointlike spin-0 target)

(ERL)

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Lepton-nucleon scattering 13

  Lepton-nucleon scattering:

  Lepton-lepton scattering:

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Lepton-nucleon scattering 14

  Lepton-nucleon scattering:

  Nucleon vertex factor (current)

Dirac (F1) and Pauli (F2) “form factors”

  Lepton-lepton scattering:

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Lepton-nucleon scattering 15

  Lepton-nucleon scattering:

  Nucleon vertex factor (current)

  Differential (Rosenbluth) cross section

Dirac (F1) and Pauli (F2) “form factors”

  Lepton-lepton scattering:

Rosenbluth formula

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Elastic cross section affected by structure 16

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Sachs form factors 17

Rosenbluth formula

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Sachs form factors 18

  Sachs form factors can be obtained from Dirac and Pauli form factors

and vice versa

Rosenbluth formula

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Sachs form factors 19

  Sachs form factors can be obtained from Dirac and Pauli form factors

and vice versa

Rosenbluth formula

  Normalization at Q2 = 0

Proton

Neutron

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Sachs form factors 20

  With Sachs form factors the Rosenbluth formula becomes simpler

Only squares of Sachs form factors occur

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Sachs form factors 21

  With Sachs form factors the Rosenbluth formula becomes simpler

  Introducing the “virtual photon polarization”

Forward angle: θ = 0ο ε = 1 Backward angle: θ = 180ο ε = 0

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Sachs form factors 22

  With Sachs form factors the Rosenbluth formula becomes simpler

  Introducing the “virtual photon polarization”

  Obtain simple expression for a “reduced cross section”

Forward angle: θ = 0ο ε = 1 Backward angle: θ = 180ο ε = 0

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"   In One-photon exchange, form factors are related to radiatively corrected elastic electron-proton scattering cross section

Rosenbluth method

τGM2

GE2

θ=180o θ=0o

 Determine |GE|, |GM|,

|GE/GM|

σred = εGE2 + τGM

2

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Fourier transform 24

  The Sachs form factors can be interpreted as spatial charge and magnetization density distributions in the Breit frame obtained via Fourier transforms

  However, the effect of recoil prohibits the interpretation as rest frame distributions!

  Breit frame: defined as frame in which no energy is transferred (ν=0):

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Spatial distributions in the Breit frame

Proton Neutron

Up

Down C. Crawford et al. PRC 82 (2010) 045211 Proton

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Spatial distributions in transverse plane 26

Charge density ρ(b) in the transverse plane of the infinite momentum frame is a 2D Fourier transform of F1

The transverse coordinates are not affected by the Lorentz boost Lorentz contraction Pancake

G.A. Miller, Phys. Rev. Lett. 99, 112001 (2007)

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Multipole expansion and charge radius 27

  The proton charge radius is obtained as the slope of electric form factor at Q2 = 0

  Likewise for the magnetic radius

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Radiative corrections 28

  Feynman rule: higher-order diagrams contribute to same final state   Suppressed by powers of α – corrections of order % to tens of %

L. W. Mo and Y. S. Tsai, Rev. Mod. Phys. 41, 205 (1969) L. C. Maximon and J. A. Tjon, Phys. Rev. C 62, 054320 (2000) M. Vanderhaeghen et al. Phys. Rev. C 62, 025501 (2001)

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Radiative corrections 29

  Mainz VCS

E = 705 MeV

θ = 40o

Bethe-Heitler (e)

Born (p)

Angular distribution of the emitted photon

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Radiative corrections 30

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Radiative corrections 31

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Radiative corrections 32

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How radiative corrections matter at high Q2 33

Q2 = 1.75, 3.25 and 5 (GeV/c)2

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Proton electric and magnetic form factors GE and GM

  Unpolarized and polarized methods   Traditional and new techniques   Overview of experimental data

High Q2: Energy frontier   Proton form factor ratio   Transition to pQCD   Two-photon exchange: GE(Q2) uncertain

Low Q2: Precision frontier   Pion cloud effect   Deviations from dipole form   The Proton Radius Puzzle: 7σ discrepancy

A. Thomas, W. Weise, The Structure of the Nucleon (2001)

Motivation 34

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"   In One-photon exchange, form factors are related to radiatively corrected elastic electron-proton scattering cross section

Form factors from Rosenbluth method

τGM2

GE2

θ=180o θ=0o

 Determine |GE|, |GM|,

|GE/GM|

σred = εGE2 + τGM

2

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GpE and Gp

M from unpolarized data 36

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GpE and Gp

M from unpolarized data 37

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GpE and Gp

M from unpolarized data

"   charge and magnetization density (Breit fr.)

"   Dipole form factor

"   within 10% for Q2 < 10 (GeV/c)2

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GpE and Gp

M from unpolarized data

"   charge and magnetization density (Breit fr.)

"   Dipole form factor

"   within 10% for Q2 < 10 (GeV/c)2

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High Q2: GE uncertain

Low Q2: GM uncertain

σred = εGE2 + τGM

2

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How radiative corrections matter … 40

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Rosenbluth data and form factor scaling 41

Early Rosenbluth data from 1970’s from DESY and Bonn showed onset of for decline of GE faster than standard dipole

However, data from SLAC favored scaling (Litt 1970, Walker 1994, Andivahis 1994)

Scaling confirmed at JLab by Christy 2004 and Qattan 2005

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Rosenbluth data and form factor scaling 42

Early Rosenbluth data from 1970’s from DESY and Bonn showed onset of for decline of GE faster than standard dipole

However, data from SLAC favored scaling (Litt 1970, Walker 1994, Andivahis 1994)

Scaling confirmed at JLab by Christy 2004 and Qattan 2005

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The amazing result:

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Concept of spin and polarization

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"   Early QM: energy quantized → Planck: black-body radiation, Einstein: photo-electric effect

"   Orbital angular momentum quantized Bohr, Sommerfeld: Atomic shell model

"   Correspondence principle QM observables have classical analogon for N→∞ or ħ→0

Quantum mechanics without spin? 44

Page 45: Form Factors with Electrons and Positrons Factors with Electrons and Positrons HUGS2013, JLab, May 28 – June 14, 2013 ... Bohr, Sommerfeld: Atomic shell model " ... “In a given

"   Early QM: energy quantized → Planck: black-body radiation, Einstein: photo-electric effect

"   Orbital angular momentum quantized Bohr, Sommerfeld: Atomic shell model

"   Correspondence principle QM observables have classical analogon for N→∞ or ħ→0

"   But incomplete! Existing puzzles of the "   Zeeman effect (1896) "   Fine structure and hyperfine structure (Goudsmit+Uhlenbeck 1925) "   Stability of atoms (Pauli 1924, Dirac 1928)

explained by concept of electron spin ½

Quantum mechanics without spin? 45

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Stern-Gerlach Experiment (1922)

•  Stern and Gerlach 1922: Ag atoms through a non-uniform magnetic field

•  Phipps and Taylor 1927: same observation with H atoms (L=0!)

The beam split in two. This marked the discovery of the electron spin. A new type of internal angular momentum, with a quantum number that can take on only two values, s=½, ms=±½

Spin is fundamentally different from orbital momentum! No classical analogon!

Discovery of electron spin

Source Magnetic field gradient Screen

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  From spectra of complex atoms, Wolfgang Pauli (1925) deduced a new rule:

“In a given atom, no two electrons* can be in the same quantum state, i.e. they cannot have the same set of quantum numbers n, l, ml , ms”

  → every “atomic orbital with n,l,ml” can hold 2 electrons: (↑↓)   Systems of bosons have symmetric, fermions have antisymmetric

wave function   → Fermi and Bose statistics   → explains stability of atoms

“Pauli Exclusion Principle”

*Note: More generally, no two identical fermions (any particle with spin of ħ/2, 3ħ/2, etc.) can be in the same quantum state.

Pauli exclusion principle 47

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Orbital motion and magnetic moment

• Magnetic moment proportional to angular momentum remains true with relativity and QM.

• Orbital angular momentum and magnetic moment: g = 1

• Classical ring current

• Angular momentum

•  Torque causing precession

• Magneton:

=magnetic moment of a uniformly charged sphere with

• Magnetic moment

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  Magnetic moment proportional to spin

  The ratio of magnetic moment to “spin” involves a “g” factor   Electron gs~2   Proton gs~5.59   Neutron gs~3.83

  Electron gs=2 predicted by Dirac Eq.! spin is a property of spacetime

  Spin precession: Larmor frequency

  → Spin manipulation through magnetic interaction

Spin and magnetic moment

Deviation from 2 is “anomalous” }

MRI

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Spin ½ and polarization

  Single spin “measurement”: choose quantization axis (e.g. magnetic field) with arbitrary but fixed orientation

→ s=½, ms=±½

  N “measurements” (ensemble of spins):

Probability p(ms) to find ms → “Polarization”

  Spin asymmetry A = (N+ − N−) / (N+ + N−)

  Polarization vector can be controlled externally “Spin orientation” is “jargon”

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Polarimetry

left right

Spin-zero nucleus

 Electron polarization measured with Compton (eγ) or Moller (ee) scattering

 Muon polarization from angular distribution of decay µ→eνν

 Strong LS interaction energy allows hadron polarization measurements with large analyzing powers

Intensity

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Lepton-nucleon scattering 52

  Lepton-nucleon scattering:

  Nucleon vertex factor (current)

Dirac (F1) and Pauli (F2) “form factors”

  Lepton-lepton scattering:

  Spin dependent, polarized cross section: no more averaging over initial and summing over final spins in the matrix element