Determination of the - and '-nucleus optical potential Mariana - - PowerPoint PPT Presentation

determination of the and nucleus optical potential
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Determination of the - and '-nucleus optical potential Mariana - - PowerPoint PPT Presentation

Determination of the - and '-nucleus optical potential Mariana Nanova for the CBELSA/TAPS Collaboration Outline: motivation exp. approaches to study the in-medium properties of mesons experimental results on the real and


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Mariana Nanova for the CBELSA/TAPS Collaboration

*funded by the DFG within SFB/TR16

Outline: ◆ motivation ◆ exp. approaches to study the in-medium properties of mesons ◆ experimental results on the real and imaginary part of the ω- and η’-nucleus optical potential ◆ summary & outlook

MESON2016 Cracow, 2th - 7th June 2016

Determination of the ω- and η'-nucleus optical potential

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2

if the QCD ground state changes in a medium ⇒ properties of hadrons (“excited states”) are also expected to change

baryons and mesons

◆ QCD vacuum as a Bose-Einstein condensate of qq ◆ all states (particles) are created out of the vacuum state (“excitations of the QCD-vacuum”) ◆ the ground-state structure influences the particle properties

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widespread theoretical and experimental activities to search for in-medium modifications of hadrons how do the hadron properties (mass, width) change in a dense nuclear medium ??

hadrons in the medium

G.E.Brown and M. Rho, PRL 66 (1991) 2720

m? m ≈ < ¯ qq >? < ¯ qq >0 ≈ 0.8(ρ ≈ ρ0)

“Brown-Rho Scaling”

T.Hatsuda and S. Lee, PRC 46 (1992) R34

m

V

mV = (1 − α ρ ρ0 ); α ≈ 0.18

QCD sum rule approach: drop of ρ, ω mass by about 15% at ρ=ρ0

  • V. Bernard and U.-G. Meißner,

NPA 489 (1988) 647

pioneering papers:

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4

  • V. Bernard and U.-G. Meissner,
  • Phys. Rev.D 38 (1988) 1551

almost no dependence of η’ mass on density

  • S. Bass and A. Thomas,

PLB 634 (2006) 368

Δmη’ (ρ0)≈−40 MeV for θηη’ = −200 Δmη’ (ρ0)≈−150 MeV Δmη (ρ0) ≈ +20 MeV

  • H. Nagahiro et. al,
  • Phys. Rev. C 74 (2006) 045203

SU(2) SU(3)

  • S. Sakai and D. Jido

PRC 88 (2013) 064906

Δmη’ (ρ0)≈−80 MeV NJL-model NJL-model linear σ model QMC-model

hadronic models: predictions for η’ in-medium mass

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5

hadronic models: predictions for ω-spectral functions

  • F. Klingl et al.,

NPA 610 (1997) 297; NPA 650 (1999) 299

◆ lowering of in-medium mass ◆ broadening of resonance

with increasing nuclear density Re(U) ≠0; Im(U) ≠0

  • M. Lutz et al.,

NPA 706 (2002) 437

splitting into ω-like and N*N-1 mode due to coupling to nucleon resonances

P . Mühlich et al., NPA 780 (2006) 187

spectral function for ω meson at rest: almost no mass shift; strong in-medium broadening Re(U) ≈0; Im(U) large

experimental task: search for {

}

mass shift ? broadening? structures?

  • f hadronic spectral functions
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meson-nucleus optical potential U(r) = V (r) + iW(r)

mass and lifetime (width) may be changed in the medium

V (r) = ∆m(ρ0) · ρ(r)

ρ0

real part in-medium mass modification

W(r) = −Γ0/2 · ρ(r)

ρ0

= − 1

2 · ~c · ρ(r) · σinel · β

imaginary part in-medium width, absorption inelastic cross section lifetime shortened

  • H. Nagahiro an S. Hirenzaki,

PRL 94 (2005) 232503

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experimental approaches to determine the meson-nucleus optical potential U(r) = V (r) + iW(r) V (r) = ∆m(ρ0) · ρ(r)

ρ0

real part

W(r) = −Γ0/2 · ρ(r)

ρ0

= − 1

2 · ~c · ρ(r) · σinel · β

imaginary part

◆ transparency ratio measurement

TA = σγA→η0X A · σγN→η0X

  • D. Cabrera et al., NPA 733 (2004)130

◆ line shape analysis ◆ excitation function ◆ momentum distribution ◆ meson-nucleus bound states

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CBELSA/TAPS experiment

MiniTAPS Crystal Barrel photon beam

Eγ=0.7-3.1 GeV

Forward Plug

solid target: 12C

and 93Nb

Eγ=0.7 - 3.1 GeV

1320 CsI 216 BaF2

4π photon detector: ideally suited for identification of multi-photon final states

η’→π0π0η→6γ

BR 8.5%

ω→π0γ→ 3γ BR 8.2%

≈ 3% σm m

η’→π0π0η→6γ

]

2

[MeV/c

η π π

M 850 900 950 1000 1050 1100 1150 )]

2

[1/(6 MeV/c

η π π

N 200 400 600 800 1000 1200 1400 1600 1800 3177 counts

Nb

2

0.3 MeV/c ± =11.8 σ

2

0.5 MeV/c ± m=957.6

≈ 1% σm m

]

2

[MeV/c

γ π

M 600 650 700 750 800 850 900 950 )]

2

[1/(4 MeV/c

γ π

N

3

10

4

10 64456 counts

C

2

0.3 MeV/c ± =25.8 σ

2

0.4 MeV/c ± m=792.5

ω→π0γ→ 3γ

≈ 3% σm m

64456 counts 3177 counts

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The real part of the meson-nucleus

  • ptical potential
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  • J. Weil, U. Mosel and
  • V. Metag, PLB 723 (2013 ) 120

the real part of the ω-nucleus potential

ω→π0γ

sensitive to nuclear density at production point and not at decay point

γ+93Nb→π0γ+X Eγ=0.9-1.3 GeV

π0γ momentum distribution

◆ momentum distribution of the meson: in case of dropping mass - when leaving the nucleus hadron has to become on-shell; mass generated at the expense of kinetic energy ➯ downward shift of momentum distribution

10

➯ cross section enhancement

π0γ excitation function

◆ measurement of the excitation function

  • f the meson

in case of dropping mass - higher meson yield for given √s because of increased phase space due to lowering of the production threshold

Eγthr

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Eγthr

excitation function for ω photoproduction off C comparison with GiBUU calculation

CB/TAPS @ MAMI

  • V. Metag et al., PPNP

, 67 (2012) 530

data not consistent with strong mass shift scenario (Δm/m≈-16%)

vacuum collisional broadening(CB) CB+mass shift (-16%) mass shift (-16%)

  • M. Thiel et al., EPJA 49 (2013) 132

momentum distribution V(ρ=ρ0) = −(42±17(stat)±20(syst)) MeV

[GeV]

γ

E 0.9 1 1.1 1.2 1.3 1.4 b] µ /A [ σ

  • 2

10

  • 1

10

Carbon

★CB/TAPS@MAMI

  • CBELSA/TAPS

GiBUU

collisional broad. and mass shift V = 0 MeV V = -20 MeV V = -40 MeV V = -55 MeV V = -94 MeV V = -125 MeV

Carbon

excitation function

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data: M. Nanova et al., PLB 727 (2013) 417

data disfavour strong mass shifts

Eγ[MeV] ση’ [µb]

V(ρ=ρ0) = 0 MeV V(ρ=ρ0) = -75 MeV V(ρ=ρ0) = -100 MeV V(ρ=ρ0) = -150 MeV V(ρ=ρ0) = -50 MeV V(ρ=ρ0) = -25 MeV

Eγ[MeV] ση’ [µb]

σtot C data σdiff Eγthr

10

  • 1

1 10 1000 1500 2000 2500

Vη’(ρ=ρ0) = −(40±6) MeV

ση’N=11 mb

CBELSA/TAPS @ ELSA

pη’ [GeV/c ] dση’/dpη’ [µb/GeV/c]

C data Eγ=1500-2200 MeV V(ρ=ρ0) = 0 MeV V(ρ=ρ0) = -75 MeV V(ρ=ρ0) = -25 MeV V(ρ=ρ0) = -100 MeV V(ρ=ρ0) = -150 MeV V(ρ=ρ0) = -50 MeV

10

  • 1

1 0.25 0.5 0.75 1 1.25 1.5 1.75 2

Vη’(pη’≈1.1 GeV/c;ρ=ρ0) = −(32±11) MeV

ση’N=11 mb

excitation function and momentum distribution for η' photoproduction off C

calc.: E. Paryev, J. Phys. G 40 (2013) 025201

γ C →η’X

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excitation function and momentum distribution for η' photoproduction off Nb

CBELSA/TAPS @ ELSA

[GeV/c]

' η

p

0.5 1 1.5 2 2.5

b/GeV/c] µ / [

' η

/dp σ d

1 10

Nb =1.3 - 2.6 GeV

γ

E

= 14 mb

inel ' η

σ ) = 0 MeV ρ = ρ V( ) = - 25 MeV ρ = ρ V( ) = - 50 MeV ρ = ρ V( ) = - 75 MeV ρ = ρ V( ) = -100 MeV ρ = ρ V( ) = -150 MeV ρ = ρ V(

P R E L I M I N A R Y

Vη'(pη'≈1.14 GeV/c;ρ=ρ0) = −(41±22) MeV

  • M. Nanova et al., submitted to PRC for publication

[GeV]

γ

E

1 1.5 2 2.5

b] µ [

' η

σ

1 10

Nb

tot

σ

diff

σ

= 14 mb

inel ' η

σ ) = 0 MeV ρ = ρ V( ) = - 25 MeV ρ = ρ V( ) = - 50 MeV ρ = ρ V( ) = - 75 MeV ρ = ρ V( ) = -100 MeV ρ = ρ V( ) = -150 MeV ρ = ρ V(

' thr η γ

E

P R E L I M I N A R Y

Vη'(ρ=ρ0) = −(46±15) MeV

data disfavour strong mass shifts γ Nb →η’X

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real part of ω-nucleus potential from ω kinetic energy

10≤θp≤110

the higher the attraction the lower the kinetic energy of the ω meson

γ ω p

Eγ=1.25-3.1 GeV CBELSA/TAPS @ ELSA

  • 782 [MeV]

γ π

E 20 30 40 50 60 70 80 90 [nb/MeV/sr] Ω d

kin

/dE

γ π

σ

2

d 1.4 1.5 1.6 1.7 1.8 1.9 2 2.1 2.2

) , W (V

  • (156,70) MeV
  • (100,70) MeV
  • ( 50,70) MeV
  • ( 0,70) MeV
  • (-20,70) MeV
  • (-50,70) MeV
  • H. Nagahiro, priv. com.
  • 782 [MeV]
  • E
  • 300 -200 -100

100 200 300 400 [nb/MeV/sr]

  • d

kin

/dE

  • 2

d

  • 0.5

0.5 1 1.5

Carbon

  • S. Friedrich et al., PLB 736 (2014) 26

Ekin=(60.5±7)MeV

Vω(pω≈300 MeV/c; ρ=ρ0) = −(15±35) MeV

potential depth [MeV]

  • 150
  • 100
  • 50

50 peak position [MeV] 30 40 50 60 70 80 90

d)

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compilation of results for the real part of the ω- and η’-nucleus optical potential

Vη’A(ρ=ρ0) =

−(40±8(stat)±15(syst)) MeV VωA(ρ=ρ0) = −(29±19(stat)±20(syst)) MeV

ω η’

[MeV]

'A η

V 80 − 60 − 40 − 20 −

excitation function

  • mom. distribution

weighted average C Nb

[MeV]

'A η

V 80 − 60 − 40 − 20 − 20

excitation function

kin

peak E average C

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The imaginary part of the meson-nucleus

  • ptical potential: momentum dependence
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[MeV/c]

ω

p 500 1000 1500 2000 2500 b/(GeV/c)] µ /A [

ω

/dp σ d 0.5 1 1.5 2 2.5

Nb C

momentum differential cross section for ω, η’ produced off C, Nb

ω η’

γ C,Nb → ωX

Eγ = 1.2- 2.9 GeV

TNb/C (pm) = 12 ⦁σγNb→mX (pm) 93 ⦁σγC→mX (pm)

m

momentum differential cross sections ⇒

P R E L I M I N A R Y

[MeV/c]

' η

p 500 1000 1500 2000 2500 b/(GeV/c)] µ /A [

' η

/dp σ d 0.05 0.1 0.15 0.2 0.25

Nb C

P R E L I M I N A R Y

γ C,Nb →η’X

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ω η’

momentum dependence of transparency ratio for ω, η’

absorption of η’ mesons much weaker than for ω mesons !!

TNb/C (pm) = 12 ⦁σγNb→mX(pm) 93 ⦁σγC→mX (pm)

m

  • M. Kotulla et al., PRL 100 (2008) 192302

bbbbbbbbbbbb

  • M. Nanova et al., PLB 710 (2012) 600

blablabla

TNb/C ≈ 0.7-0.8

η’

TNb/C ≈ 0.4-0.6

ω

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imaginary part of the potential for ω, η’

Glauber model: high energy Eikonal approximation TNb/C (pm)

⇒ Γ0 (ρ=ρ0) (pm) = - 2 Im U0 (pm)

m m m

ω η’

  • M. Nanova et al., PLB 710 (2012) 600

Im U0(ρ=ρ0,pω=0) = −(30±10) MeV

ω

◆ extrapolation to production threshold: ◆ extension to higher energies allows for dispersion relation analysis,

providing link between real and imaginary part of potential

  • M. Kotulla et al., PRL 114 (2015) 199903

PRELIMINARY

[MeV]

thr

s

  • ω

s 200 400 600 800 1000 1200 1400 1600 ) [MeV]

ω

  • (Im U

20 40 60 80 100 120

PRL 114 (2015) 199903 this experiment

PRELIMINARY

Im U0(ρ=ρ0,pη’=0) = −(10±3) MeV

η’

[MeV]

thr

s

  • '

η

s 200 400 600 800 1000 1200 1400 ) [MeV]

' η

  • (Im U

5 10 15 20 25 30 35 40 45

PLB 710 (2012) 600 this experiment

blablabla blablabla

  • S. Friedrich et al., submitted to EPJA for publication
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compilation of results for real and imaginary part of the ω, η’ -nucleus optical potential

UωA(ρ=ρ0)= −((29±19(stat)±20(syst) + i(30±10)) MeV Uη’A(ρ=ρ0)= −((40±8(stat)±15(syst) + i(10±3)) MeV

ω not a good candidate to search for meson-nucleus bound states!

⎮Im U ⎮≈⎮Re U⎮; ➯

first (indirect) observation of in-medium mass shift of η’ at ρ=ρ0 and T=0 in good agreement with QMC model predictions (S. Bass et al. , PLB 634 (2006) 368)

η’ promising

candidate to search for mesic states ⎮Re U⎮ >>⎮Im U⎮; ➯

ω η’

potential depth [MeV] 10 20 30 40 50 imaginary part [MeV] 10 20 30 40 50 60

ω ' η

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  • utlook: search for η’-mesic states in photo-nuclear reactions

12C(γ,p) η’X @ 1.5-2.8 GeV

Δp/p ≈ 1-2 %

B1: BGO-OD@ELSA

BGO-OD ideally suited for exclusive measurement

approved proposal: ELSA/3-2012-BGO

η’

γ

p

formation and decay of η’-mesic state

N

η

LEPS2@SPring-8

12C(γ,p) η’X @ 1.5-2.4 GeV

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,)

missing mass spectrometry: Δmm =2.5 MeV/c2

12C target

S2 S4 2.5 GeV protons 2 . 7

  • 2

. 9 G e V / c d e u t e r

  • n

s ( p r

  • t
  • n

s ) MWDC aerogel Cerenkov aerogel Cerenkov p/d separation by aerogel Cerenkov TOF S2-S4 (diff.≈20 ns) plastic scintillators

search for η’-mesic states in hadronic reactions FRS@GSI:

12C(p,d)η’⦻11C

  • K. Itahashi et al., PETP 128 (2012) 601
  • H. Nagahiro et al., PRC 87 (2013) 045201

particle identification by time-of-flight

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Summary & Outlook

how do the hadron properties (mass, width) change in a dense nuclear medium ?? ◆ all mesons are broadened; their lifetime is shortened through inelastic collisions Γω(ρ=ρ0; p=0) ≈ 60 MeV; Γη’(ρ=ρ0; p=0) ≈ 15 MeV; ◆ large mass modifications Δm > 100 MeV (as predicted by some calculations) have not been observed ◆ for the η’ meson an in-medium mass drop of Δm (ρ=ρ0) ≈ −40 MeV has been determined ◆ the η’ meson is a good candidate for forming meson-nucleus bound states since Im U << Re U ◆ search for η’ mesic states ongoing ◆ in-medium effects described within meson-nucleus optical

meson properties do change in a strongly interacting medium !!

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BACKUP

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[MeV]

ω

Γ 50 100 150 200 250 300 350 400

ω Nb/C

T 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

= 200 MeV/c

ω

p = 400 MeV/c

ω

p = 600 MeV/c

ω

p = 800 MeV/c

ω

p = 1000 MeV/c

ω

p = 1200 MeV/c

ω

p = 1600 MeV/c

ω

p = 2400 MeV/c

ω

p

ω

[MeV]

' η

Γ 50 100 150 200 250 300 350 400

' η Nb/C

T 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

= 275 MeV/c

' η

p = 525 MeV/c

' η

p = 750 MeV/c

' η

p = 1075 MeV/c

' η

p = 1225 MeV/c

' η

p = 1525 MeV/c

' η

p = 1825 MeV/c

' η

p = 2275 MeV/c

' η

p

' η

in-medium width from transparency ratio

Glauber model in high energy eikonal approximation TNb/C(p) ⟷ Γ0(p)

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26

[MeV/c]

' η

p 500 1000 1500 2000 [MeV]

' η

Γ 10 20 30 40 50 60 70 80 90

PLB 710 (2012) 600 this experiment

momentum dependence of ω, η’ in-medium width

P . Mühlich et al.,NPA 780 (2006) 187

  • O. Buss et al., Phys. Rep. 512 (2012) 1

[MeV/c]

ω

p 500 1000 1500 2000 [MeV]

ω

Γ 50 100 150 200 250

PRL 114 (2015) 199903 this experiment

GiBUU

  • A. Ramos et al., EPJA 49 (2013)148
  • D. Cabrera and R. Rapp, PLB 729 (2014)67
  • S. Friedrich
  • M. Kotulla et al., PRL 114 (2015) 199903
  • M. Nanova et al., PLB 710 (2012) 600
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27

[MeV/c]

' η

p 500 1000 1500 2000 [mb]

' η inel

σ 5 10 15 20 25 30 35 40

PLB 710 (2012) 600 this experiment

[MeV/c]

ω

p 500 1000 1500 2000 [mb]

ω inel

σ 50 100 150 200

PRL 114 (2015) 199903 this experiment

inelastic absorption cross section σinel

a=0.0±6.2 b=31±4 a=8.1±9.5 b=6.8±9.8

⟨σinel(p)⟩ = (14±3) mb

  • E. Oset and A. Ramos, PLB 704 (2012) 334
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if self-energy Σ of the meson is an analytic function then imaginary and real part related up to a constant by: work in progress (Horst Lenske (B7)) + const

Dispersion relation analysis