*Work at ASU is supported by the U.S. National Science Foundation

56
B. G. Ritchie - MENU 2013 - October 2013 1 *Work at ASU is supported by the U.S. National Science Foundation Barry G. Ritchie* Arizona State University Latest results from FroST at Jefferson Lab

description

Latest results from FroST at Jefferson Lab. Barry G. Ritchie* Arizona State University. *Work at ASU is supported by the U.S. National Science Foundation. Nucleon excited states. As a composite system, the nucleon has a specific spectrum of excitations: the nucleon resonances . - PowerPoint PPT Presentation

Transcript of *Work at ASU is supported by the U.S. National Science Foundation

Page 2: *Work at ASU is supported by the U.S. National Science Foundation

2

Nucleon excited states

γ p → π+ n

B. G. Ritchie - MENU 2013 - October 2013

• As a composite system, the nucleon has a specific spectrum of excitations: the nucleon resonances.

• This nucleon resonance spectrum has many broad overlapping states, making disentangling the spectrum difficult.

Page 3: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 3

The state of our knowledge

22 Δ* states: • 7 with **** • 3 with ***• 7 with **• 5 with *

Nucleon

• Nearly half the states have only fair or poor evidence!

• Most states need more work to learn details

• Are there missing states?26 N* states: • 10 with **** • 5 with ***• 8 with **• 3 with *

Page 4: *Work at ASU is supported by the U.S. National Science Foundation

4

Models predict (lots of)excitations • Many nucleon models have offered

“predictions” for the nucleon resonance spectrum --• constituent quark model• diquark • collective models• instanton-induced interactions• flux-tube models• lattice QCD• (your favorite here) - BUT…

• THE BIG MYSTERY: Most models

predict many more resonance states than have been observed.

B. G. Ritchie - MENU 2013 - October 2013

Page 5: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 5

Example: R.G. Edwards et al. Phys. Rev. D87 054506 (2013)

Example: Lattice QCD results for N* resonances• Noticeable change as the π mass

becomes more realistic

• Number of low-lying states (boxed regions) remains the same for the two π-masses, and generally is the same as NRQMs

• Many of these predicted states are poorly determined or missing.

mπ = 524 MeV

mπ = 391 MeV

Page 6: *Work at ASU is supported by the U.S. National Science Foundation

EXPERIMENT

BARYON MODELS

REACTION MODELAMPLITUDE ANALYSIS

cross sections,spin observables

multipole amplitudes,phase shifts

effective Lagrangians,Isobars, etc…

6

Solving a mystery: “The Case of the Missing Resonances”

LQCD, quark models,etc…

B. G. Ritchie - MENU 2013 - October 2013

Page 8: *Work at ASU is supported by the U.S. National Science Foundation

8

• 8 helicity states: 4 initial, 2 final → 4 2 = 8∙ possible complex amplitudes• Parity reduces these to 4 complex amplitudes Hi (8 W-dependent functions)• Overall phase unobservable → 7 W-dependent functions• Suggests complete determination possible with 7 observables/experiments • HOWEVER, not all possible observables are linearly independent →

a minimum of 8 observables / experiments

Helicity amplitudes for γ + p → p + pseudoscalar

3 12 2

11 22

13 42

H HA

H H

helicity +1 photons (ε+): helicity -1 photons (ε-):31

2 21

4 321

2 12

H HA

H H

,, AeA

→ Parity →

11 12

21 22

A AA

A A

Initial helicity final helicity

B. G. Ritchie - MENU 2013 - October 2013

Page 9: *Work at ASU is supported by the U.S. National Science Foundation

9

Linkage between helicity amplitudes and the observables for single pseudoscalar photoproduction

Differential cross section

Beam polarization S

Target asymmetry T

Recoil polarization P

Double polarization observables

• Need at least 4 of the double observables from at least 2 groups for a “complete experiment”

• π0p, π+ n, and η p will be nearly complete

• K+ Λ will be complete!

Long

itudi

nal t

arge

t

Tran

sver

se ta

rget

Pola

rized

ph

oton

s+

B. G. Ritchie - MENU 2013 - October 2013

Page 11: *Work at ASU is supported by the U.S. National Science Foundation

11B. G. Ritchie - MENU 2013 - October 2013

The detective’s tools:FroST and friends

Page 13: *Work at ASU is supported by the U.S. National Science Foundation

13

Hall B Bremsstrahlung Photon Tagger (not dead yet!)

61 backing counters

B. G. Ritchie - MENU 2013 - October 2013

• Jefferson Lab Hall B bremsstrahlung photon tagger had:• Eγ = 20-95% of E0

• Eγ up to ~5.5 GeV• Circular polarized

photons with longitudinally polarized electrons

• Oriented diamond crystal for linearly polarized photons

Page 14: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 14

• Doped butanol and dynamic nuclear polarization): • Butanol with paramagnetic radical

TEMPO• Polarize unpaired TEMPO electrons to

99.999% with B = 5 T and T = 0.3 K• Transfer electron polarization to free

protons with microwaves at ~140 GHz• Remove microwaves• Cool to T = 30 mK and use B = 0.5 T

holding field• Put target in CLAS and run experiment

Frozen Spin Target - FroST

Page 15: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie – MENU 2013 - Rome15

Transverse polarization – g9b

Longitudinal polarization – g9a

Complete assembly – g9a

Holding coils

Page 16: *Work at ASU is supported by the U.S. National Science Foundation

16

• Frozen spin butanol (C4H9OH)

• Pz ≈ 80%

• Target depolarization: τ ≈100 days

FroST performance

• For g9a (longitudinal orientation) 10% of allocated time was used polarizing target

• For g9b (transverse orientation) 5% of allocated time was used polarizing target

B. G. Ritchie - MENU 2013 - October 2013

Page 17: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 17

FroST’s first clues:Single pion photoproduction

Page 18: *Work at ASU is supported by the U.S. National Science Foundation

18

Isospin combinations for reactions involving π0 and π+

21

321

21

323

21

321

21

3230

,3/2,3/1:

,3/1,3/2:

IIIIn

IIIIp

Δ+ N*

• Differing isospin compositions for N* and Δ+ for the π0 p and π+ n final states

• The π0 p and π+ n final states can help distinguish between the Δ and N*

B. G. Ritchie - MENU 2013 - October 2013

Page 19: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 19

Theoretical analyses In the plots that follow, you will see many curves from:• SAID: A two-stage PWA where

• stage 1 is the fit to data• stage 2 is the extraction of resonance parameters

• BnGa (Bonn-Gatchina): A single stage PWA• MAID: Isobar analysis

Note: The SAID results labeled “new” in this section of the talk include the new Σ data from ASU/CLAS. Later sections of the talk show SAID results that do not have the new Σ data included.

Page 20: *Work at ASU is supported by the U.S. National Science Foundation

20

Observables: T and F

B. G. Ritchie - MENU 2013 - October 2013

Experiment:• g9b: FroST

Configuration:• Circular photon polarization• Transverse target polarization• Unpolarized photon (add circular beams)• No recoil polarization

Reaction: γ p → n π+

Photon beam Target

x y z

Unpolarized 0 T 0

Linearly polarized H (-P) -G

Circularly polarized F 0 -E

Page 21: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 21

T for γ p → n π+

• Early stage results• CLAS results agree well with

previous data

(new)

(new)

(new)

g9b:Michael Dugger

Page 22: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 22

F for γ p → n π+

• Early stage results• Predictions get much worse at

higher energies• SAID13 are predictions based

on preliminary fits to CLAS pion Σ measurements

(new) (new)

(new)

g9b: Michael Dugger

Page 23: *Work at ASU is supported by the U.S. National Science Foundation

23

Observable: E

B. G. Ritchie - MENU 2013 - October 2013

Configuration:• Circular photon polarization• Longitudinal target polarization• No recoil polarization

Reactions: γ p → p π0 and γ p → n π+

Photon beam Target

x y z

Unpolarized 0 T 0

Linearly polarized H (-P) -G

Circularly polarized F 0 -E

Experiment:• g9a: FroST

Page 24: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 24

E for γ p → p π0

• Early stage results

• Predictions better at lower energies

(new)

g9a:

Michael Dugger

Page 25: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 25

E for γ p → n π+

Steffen Strauch

PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARY

PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARY

PRELIMINARY

PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARY PRELIMINARY PRELIMINARY

Predictions worse at higher energies

SAIDSAID (new)MAID

Cos(θπc.m.)

W = 1.25 GeV W = 1.27 GeV

W = 1.29 GeV W = 1.31 GeV W = 1.33 GeV W = 1.35 GeV

W = 1.47 GeVW = 1.45 GeV

W = 1.43 GeVW = 1.41 GeVW = 1.39 GeVW = 1.37 GeV

W = 1.49 GeV W = 1.51 GeV W = 1.53 GeV W = 1.55 GeV W = 1.57 GeV W = 1.59 GeV

W = 1.71 GeVW = 1.69 GeVW = 1.67 GeVW = 1.65 GeVW = 1.63 GeVW = 1.61 GeV

W = 1.73 GeVW = 1.75 GeV W = 1.77 GeV W = 1.81 GeV W = 1.83 GeV W = 1.9 GeV

W = 2.19 GeVW = 2.13 GeVW = 2.07 GeV

W = 2.02 GeVW = 1.98 GeVW = 1.94 GeV

g9a:

Page 26: *Work at ASU is supported by the U.S. National Science Foundation

26

Observable: G Reactions: γ p → n π+

B. G. Ritchie - MENU 2013 - October 2013

Configuration:• Linear photon polarization• Longitudinal target polarization• No recoil polarization

Experiment:• g9a: FroST

Photon beam Target

x y z

Unpolarized 0 T 0

Linearly polarized H (-P) -G

Circularly polarized F 0 -E

Page 27: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 27

G for γ p → n π+g9a:

▬ SAID-- MAID-• Bonn-Gatch

Jo McAndrew

PRELIMINARY PRELIMINARY

PRELIMINARYPRELIMINARY

W=2030-2080 MeV

W=1640-1680 MeV

W=1840-1880 MeV

W=1475-1500 MeV

• Early stage results

• Photon polarizations are approximate

◊ Bussey et al

Page 29: *Work at ASU is supported by the U.S. National Science Foundation

29

“Isospin filters”• Final states of ηp and K+Λ systems have isospin ½ , and limit

one-step excited states of the proton to be isospin ½. • Thus, the final states ηp and K+Λ can serve as isospin filters

to the resonance spectrum.

γ p → π+ n γ p → η p

B. G. Ritchie - MENU 2013 - October 2013

Page 30: *Work at ASU is supported by the U.S. National Science Foundation

30

Observables: T and F

B. G. Ritchie - MENU 2013 - October 2013

Configuration:• Circular photon polarization• Transverse target polarization• Unpolarized photon (add circular beams)• No recoil polarization

Reaction: γ p → η p

Photon beam Target

x y z

Unpolarized 0 T 0

Linearly polarized H (-P) -G

Circularly polarized F 0 -E

Experiment:• g9b: FroST

Page 31: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie – MENU 2013 – Rome 31

T for γ p → η p g9b:Ross Tucker

Page 32: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie – MENU 2013 – Rome 32

F for γ p → η p g9b:Ross Tucker

Page 33: *Work at ASU is supported by the U.S. National Science Foundation

33

Observable: E

B. G. Ritchie - MENU 2013 - October 2013

Configuration:• Circular photon polarization• Longitudinal Target polarization• No recoil polarization

Reaction: γ p → η p

Photon beam Target

x y z

Unpolarized 0 T 0

Linearly polarized H (-P) -G

Circularly polarized F 0 -E

Experiment:• g9a: FROST

Page 34: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 34

E for γ p → h p

• Predictions are generally inconsistent with data at all energies at more forward angles

(new)

g9a:

Igor Senderovich

Page 35: *Work at ASU is supported by the U.S. National Science Foundation

35

Observables: T and F

B. G. Ritchie - MENU 2013 - October 2013

Configuration:• Circular photon polarization• Transverse target polarization• Unpolarized photon (add circular beams)• No recoil polarization

Reaction: γ p → K+L and γ p → K0S

Photon beam Target

x y z

Unpolarized 0 T 0

Linearly polarized H (-P) -G

Circularly polarized F 0 -E

Photon beam Target

x y z

Unpolarized 0 T 0

Linearly polarized H (-P) -G

Circularly polarized F 0 -E

g9b:

Natalie Walford

Page 36: *Work at ASU is supported by the U.S. National Science Foundation

W=1725 MeVEγ=1117 MeV

W=2125 MeVEγ=1938 MeV

W=2025 MeVEγ=1717 MeV

W=1975 MeVEγ=1610 MeV

W=1925 MeVEγ=1506 MeV

W=1875 MeVEγ=1405 MeV

W=1825 MeVEγ=1306 MeV

W=1775 MeVEγ=1210 MeV

W=2275 MeVEγ=2290 MeV

W=2225 MeVEγ=2170 MeV

W=2175 MeVEγ=2053 MeV

W=1675 MeVEγ=1027 MeV

PreliminaryT for γ p → K+L Bonn-Gatchina: blue

kaonMAID: pinkBonn –data - purpleGRAAL data - black

Page 37: *Work at ASU is supported by the U.S. National Science Foundation

W=1725 MeVEγ=1117 MeV

W=2125 MeVEγ=1938 MeV

W=2075 MeVEγ=1826 MeV

W=2025 MeVEγ=1717 MeV

W=1975 MeVEγ=1610 MeV

W=1925 MeVEγ=1506 MeV

W=1875 MeVEγ=1405 MeV

W=1825 MeVEγ=1306 MeV

W=1775 MeVEγ=1210 MeV

W=2275 MeVEγ=2290 MeV

W=2225 MeVEγ=2170 MeV

W=2175 MeVEγ=2053 MeV

PreliminaryT for γ p → K0S Bonn-Gatchina: blue

kaonMAID: pink

Page 38: *Work at ASU is supported by the U.S. National Science Foundation

38

A “complete” set of clues:Self-analyzing reaction K+ Y (hyperon)

• Hyperon weak decay allows extraction of hyperon polarization by looking at the decay distribution of the baryon in the hyperon center of mass system:

cos1)(cos 21

YPI

where I is the decay distribution of the baryon, α is the weak decay asymmetry (αΛ= 0.642 and αΣ0 = -⅓ αΛ), and PY is the hyperon polarization.

• Get recoil polarization information without a recoil polarimeter: the reaction is “self-analyzing”.

• No preliminary results yet, but data will be forthcoming.

B. G. Ritchie - MENU 2013 - October 2013

Page 40: *Work at ASU is supported by the U.S. National Science Foundation

40

Photoproduction of π+ π - p states

• 64 observables• 28 independent relations related to helicity amplitude magnitudes• 21 independent relations related to helicity amplitude phases• Results in 15 independent numbers

Good for discovering resonances that decay into other resonances!

B. G. Ritchie - MENU 2013 - October 2013

Page 41: *Work at ASU is supported by the U.S. National Science Foundation

41

γ p → p π+ π-

B. G. Ritchie - MENU 2013 - October 2013

next slide

unpolarized beam and longitudinal target: δl = Λx = Λy = 0

slide after next

longitudinal beam and longitudinal target: δl ≠ 0, Λx = Λy = 0

Page 42: *Work at ASU is supported by the U.S. National Science Foundation

Spin observable Pz for γ p → p π+ π-

B. G. Ritchie – MENU 2013 – Rome 42

g9a:Sungkyun Park

FSU: Winston Roberts

Fix & Arenhövel

PRELIM

INARY

Page 43: *Work at ASU is supported by the U.S. National Science Foundation

Spin observable Pz for γ p → p π+ π-

B. G. Ritchie – MENU 2013 – Rome 43

Fix & Arenhövel

s

Yuqing Maog9a:

PRELIM

INARY

Page 44: *Work at ASU is supported by the U.S. National Science Foundation

44

FroST results in the full CLAS program for photoproduction from proton

σ Σ T P E F G H Tx Tz Lx Lz Ox Oz Cx Cz

Proton target

pπ0 ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓

nπ+ ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓

pη ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓

pη’ ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓

K+Λ ✔ ✓ ✓ ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✔ ✔

K+Σ0 ✔ ✓ ✓ ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✔ ✔

K0Σ+ ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✔ ✔

✔ - published ✔ - acquired

Not shown in table: ω and ππ photoproduction observables

Preliminary results shown in this talk

Page 45: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 45

Conclusions • Spin observables will

tremendously aid in sleuthing out resonance parameters and finding missing resonances (if they exist)

• Photon experiments in Hall-B with FroST at JLab have acquired hundreds of data points yielding clues to the missing resonances

• For most reaction channels, we will have data sufficient for a nearly complete experiment

Page 46: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 46

Conclusions (cont’d)

• For K Λ and K Σ channels, we will have a complete experiment

• Double-pion observables offer a “next generation” probe of reaction mechanisms and resonances

• Data for some reactions and some observables are nearing the publication stage, but much work remains – STAY ON THE CASE!

Page 47: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 47

Acknowledgements

CLAS Collaboration

Page 49: *Work at ASU is supported by the U.S. National Science Foundation

49

Circ

ular

pol

ariza

tion

Circular polarization from 100% polarized electron beam

• Circular photon beam from longitudinally- polarized electrons

• Incident electron beam polarization

> 85%

2

2

3444

kkkkPP e

Circular beam polarization

k = Eγ/Ee

Coun

ts

H. Olsen and L.C. Maximon, Phys. Rev. 114, 887 (1959) B. G. Ritchie - MENU 2013 - October 2013

Page 50: *Work at ASU is supported by the U.S. National Science Foundation

50

Linearly polarized photons

• Coherent bremsstrahlung from 50-μ oriented diamond

• Two linear polarization states (vertical & horizontal)

• Analytical QED coherent bremsstrahlung calculation fit to actual spectrum (Livingston/Glasgow)

• Vertical 1.3 GeV edge shown

B. G. Ritchie - MENU 2013 - October 2013

Page 51: *Work at ASU is supported by the U.S. National Science Foundation

51

FroST target • Butanol composition: C4H9OH

• C and O are even-even nuclei → No polarization of the bound nucleons

• Carbon target used to represent bound nucleon contribution of butanol

B. G. Ritchie - MENU 2013 - October 2013

Page 52: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 52

Slide from Chris Keith

FroST target

Page 53: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 53

Slide from Chris Keith

FroST target

Page 54: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 54

Slide from Chris Keith

FroST target

Page 55: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 55

Slide from Chris Keith

FroST target

Page 56: *Work at ASU is supported by the U.S. National Science Foundation

B. G. Ritchie - MENU 2013 - October 2013 56

Slide from Chris Keith