Study of Neutron-Proton Correlations via �Two-Nucleon Removal Reactions
Outline:
heavy-ion target
4. Ongoing analysis of np-removal data with proton target
5. Summary
n
p
n
p
T = 0
T = 1
Hongna Liu, Beijing Normal University
IWND2026, Shanxi, China, Aug. 21-25, 2026
2
Independent Particle Model
Shell structure & Magic numbers
(Mayer & Jensen
1963 Nobel Prize)
Woods-Saxson+ Spin-Orbital Interaction
Mean Field
Correlations
Important ingredient:np Correlations
Neutron-Proton Correlations
4 types of Nucleonic pairs
Well defined from the
isospin symmetry
pp
nn
np
np
T = 1, S = 0
T = 0, S = 1
Isoscalar
Isovector
(deutron-like)
A lot of uncertainties
Neutron-Proton Correlations
Isoscalar (T=0, S=1) np pair
(deuteron-like)
🡪 new phase of nuclear matter
(e, eꞌp) reactions
R. Subedi et al., Science 320, 1476(2008)
12C( e, eꞌ pN )
@4.627GeV JLAB
IPM
SRC
S. Paschalis et al., PLB 800, 135110 (2020) .
L. Lapikas et al., NPA 553, 297c(1993).
30%~40%压低
M. Duer, et al., Nature 560, 7720 (2018) .
In Stable nuclei:
Mean-filed contribution: ~60%-70%
SRC contribution:22%±8% LRC:14%±10%
np Dominance in SRC correlations
🡺T = 0 np tensor
interaction
O. Hen et al., Science (2014),
Neutron-Proton Correlations
J. Engel et al.,.Phys. Lett.B 389, 211(1996).
T = 1 components
Nature, 654, 619(2026)
Stronger high-momentum enhancement
n & p in the same valence shell
N = Z system is good to study np correlations
(e,e’pN)
6 protons
8 protons
Shell evolution
0s1/2
0p3/2
0p1/2
1s1/2
0d5/2
0d3/2
1p3/2
0f7/2
1p1/2
0f5/2
0g9/2
2
8
20
28
16
34
32
8
20
28
New magic num.
0d3/2
6
Neutron-Proton Correlations in unstable nuclei
Driving force behind the shell evolution?
AME extrapolations
G. Audi et al., Nucl. Phys. A 729, 337 (2003)
Properties of heavy N = Z nuclei (waiting point)
(rp) nucleosynthesis
Reduced T = 0 np interaction
np correlations:
T. Otsuka et al., PRL 95, 232502(2005).
Two-nucleon Knockout Reactions in Inverse Kinematics
High incident energy🡪 Spectator
Momentum Distribution
Cross Section
Gain Direct Spectroscopic Information
Total J of the removed pair of nucleons
Spatial overlap of the removed two nucleons
E.C. Simpson et al., PRL 102,132502(2009)
🡪 Is it a good tool for systematic study of np correlations with RI beams?
Beam energy (>100 MeV/u)
1
2
Projectile
Spatially correlated
Target
Heavy-ion target
9Be or 12C
Proton target
Two types of Hammer
proton/ Heavy-ion target
1
2
Target
AZ
Stripping-Stripping
Target
A-2
A-2
Target
Free nucleon1
Free nucleon2
Diffraction-Diffraction
Stripping-Diffraction
Target
A-2
Free nucleon
Direct 2N-removal
Be/C target: 2p-removal from neutron-rich nuclei
~10%
~30%
~60%
K. Wimmer et al., PRL 109 (2012)
Pair knockout
56(12)% “di-proton” correlated events
28Mg(-2p) on Be target @ 93 MeV/u
Suppress two-step evaporation contribution
28Mg🡪27Na* (Sn=6.7 MeV) 🡪 26Ne+p
(Sp=13.3 MeV)
-1p
1p-Evaporation
26Ne+2p coincidence
8
12C(p,3He) , 12C(p, t) @ 52 MeV
M. Yasue et al., JPSJ. 42, 367 (1977)
“Unusual” neutron-proton Correlations in 12C (N = Z = 6)
Behavior of T = 0 interaction:
function of pair relative momentum
R. Subedi et al., Science 320, 1476(2008)
12C( e, epN )@4.627GeV
Back-to-back
Correlated p or n
Knocked-out p
High-momentum transfer
🡪 Short-range correlations
p
n
p
~
18
p
~
2.3
σ-np
σ-nn
P. J. Lindstrom et al., PRC 28,1602(1938)
1
2
Target
9Be
Projectile 12C
b
12C(12C,10Z)X @ 2.1 &1.05 GeV/u
~
5~6
σ-np
σ-pp
For 12C
pair counting ratio:
p
n
p
~
2.7
p
Short range
Longer range
Relative momentum q (fm-1)
Ab initio variational Monte Carlo
np pair
pp pair
R. Schiavilla et al., PRL 98, 132501(2007)
M. Alvioli et al., PRL 100, 162503(2008)
Relative momentum q (fm-1)
Different mechanisms
🡪 Sensitive to different range of 2N forces
🡪To obtain of a complete picture of np correlations
Inclusive 2N-removal data from 12C
T=1
p
n
T=0&1
n
n
p-shell SM
NCSM
10Be | σWBP | 6.52 |
Experiment | 5.81±0.29 |
p
p
T=1
T = 1
T = 1
p
n
p
p
n
n
Rs :0.89(4)
Rs :0.82(4)
Rs :1.8(0.2)
p-shell SM
(WBP)
T=0&1
T = 0 & 1
E. C. Simpson et al., PRC 83, 014605(2011)
For pp & nn (T = 1) removal, calculations are broadly consistent with data.
For np (T = 0 & 1) removal, calculations underestimate data by a factor of 2.
What do we find with inclusive data?
First Calculation:np-removal from 12C @ 2.1 GeV/u with 12C target
Indicate insufficient T = 0 np-spatial correlations in p-shell SM
Need to disentangle the T = 0 & T = 1
More exclusive data is necessary.
What do we need in next step?
To provide a clear answer
Due to Interactions or Model space?
Observables: np-removal from 12C
Verify the np correlations present in SM & Test the role of 3N Force
Partial cross sections in np removal🡪 Sensitive to the interaction used
E. C. Simpson et al., PRC 86, 054609 (2012)
Structure of 12C &10B can be described using NCSM (NN + 3N).
11
Experimental Setup
9Be(12C,10Be) 9Be(12C,10B) @190MeV/u
18O primary beam: 250MeV/u , ~0.08pnA
Production target: 9Be (5mm)
Secondary beam: 12C 190MeV/u 12k cps
Purity: 97%
Secondary target: 9Be (1.879g/cm2 )
Beam on Target: 10.7 h
TOF − ΔE
11B
12C
13N
BigRIPS PID
SAMURAI
Superconducting Analyser for Multi-particles from RAdioIsotope beams
W/O proton detection
σnp= σnp-direct + σnp-indirect
Indirect contribution is negligible (High particle separation energy)
Indirect: -1n knockout followed by 1p evaporation & Sequential knockout
Experimental Setup around SAMURAI
BDCs: Tracking of 12C beam
DALI2 (NaI): Gamma rays
NEBULA: Neutrons
FDCs: Tracking of 10B, 10Be residues
Hodoscope: TOF & ΔE of 10B, 10Be residues
Multi-particle Detector Systems
Large Acceptance
Bρmax/ Bρmin = 2 ~ 3
Measured in one setting.
SAMURAI Spectrometer
DALI2
9Be(12C,10Be + γ) X
9Be(12C,10B+ γ) X
FDC2
HODF
HODP
B=1.8T
10C
10B/12C
10Be
Experimental Challenges
Apply Hardware Cut to Exclude Unreacted 12C
SBT
High Trigger Counting Rate
Unreacted 12C beam will be accepted by SAMURAI.
12C beam
SAMURAI Magnet
Target
PID of Fragments & Inclusive cross sections
10B
10Be
PID without HODP5
PID of HODP5
Unreacted 12C was cut off.
With target
empty target
After subtraction
Clear identification of 10B
Energy (MeV/u) | 10B σ-np (mb) | 10Be σ-pp (mb) | 10B/10Be σ-np/σ-pp |
190 | 42(2) | 9.1(3) | 4.6(3) |
250 | 48(2) | 6(10) | 8(13) |
1050 | 28(2) | 5.3(3) | 5.2(5) |
2100 | 35(3) | 5.8(3) | 6.0(7) |
P. J. Lindstrom et al., PRC 28,1602(1938)
J. M. Kidd et al., PRC 37,2613(1998)
np removal from 12C
Counts/ 20keV
J, T, E, T1/2 & decay branching ratios are known.
9Be(12C,10B + γ) X
Add-back Reconstruction was applied to improve the peak-to-noise ratio & photo-peak efficiency.
Fit function: Response functions(GEANT4) + Exponential background (Error of efficiency from GEANT4: 4%)
First exclusive np-removal data
?
E(MeV)
Discrepancy mainly arises from the GS.
J=3
J=3
J=3
J=3
🡪Strong splin-aligned (p3/2)
np pair configurations in 12C?
🡪Unclear reaction process?
12C 11B* 10B
-p
-n
12C 11C* 10B
-n
-p
Sp=16 MeV
Sn=19 MeV
Evaporation
n-evaporation
p-evaporation
Counts
n
p
Diff-Diff
n
½ Strp-Diff
n
X
12C🡪10B+n
Difficult to subtract two-step process from the measured Erel spectrum
12C 11B* 10B
p in s-shell
-n
Erel (MeV)
10B
Contaminations in Erel(10B+n)
10B
10B
Be/C target: np removal
Two-step process: neutron evaporation
Target
After the reaction
Proton target: Quasi-free scattering reaction
12C(p,2p)11B @ 400 MeV/u
Before the reaction
Quasi-free scattering
with specific kinemtics
V. Panni et al., PLB 753, 204 (2016).
Y.L. Lu@BNU
V. Panin@GSI
Proton target: Indirect contribution measured from 12C(p,2p)
12C 11B* 10B (different final states)
-1p in s-state
-n
12C(p,2p)
(17%)
(n+10B) Decay ratio of the s-hole state in 11B: 17(2)%
V. Panni et al., PLB 753, 204 (2016).
Excitation Energy of 11B
Two step process to 10B:
~80% goes to the ground state
Proton target: Indirect contribution measured from 12C(p,2p)
Gamma spectrum of 12C(p,2p)(10B+n)
Evaporation to 10B: 8(1) mb out of 42(2) mb
0s-hole state in 12C: C2S = 1.62
Calculated by C.X. Yuan
Be target: Indirect contribution in two-nucleon removal
10Be: 1.6 (6) mb out of 9.2(5) mb
Measured decay branching ratios to individual final states of 10B from 12C(p,2p)11B*
(assuming same contribution from n & p evaporation)
20% contribution
10B | σWBP | σexp. |
Inc.(mb) | 21.20 | 34(3) |
10Be | σWBP | σexp. |
Inc.(mb) | 7.48 | 7.5(4) |
SM calculations with WBP interactions describe well T = 1 but underestimate T = 0
p
T = 1
p
T = 0&1
p
n
First exclusive np-removal data to 10B
Energy (MeV/u) | 10B σ-np (mb) | 10Be σ-pp (mb) | 10B/10Be σ-np/σ-pp |
190 | 34(3) | 7.5(4) | 4.5(4) |
np removal
While that to T = 0 states are broadly underestimate by the theory by a factor of 2
🡪 Insufficient treatment of T = 0 np
correlations in WBP calculations
Residues | Jπ | T | σexp.(mb) |
10B | 3+ | 0 | 13.8(19) |
| 1+ | 0 | 9.8(12) |
| 0+ | 1 | 2.3(3) |
| 1+ | 0 | 3.4(6) |
| 2+ | 0 | 1.7(4) |
| 2+a | 1 | 2.8(3) |
Inclusive |
|
| 34(3) |
SM calculations with WBP interactions describe well T = 1 but underestimate T = 0
Clear enhancement of T = 0 than T = 1 np correlations was observed.
T = 1 5.6(4) mb
T = 0 29(2) mb
R(σT = 0/σT = 1)
= 5.6(5)
ab initio no-core shell model (NCSM)
10B | σWBP | σNCSM(NN+3N) | σNCSM3(NN) | σexp. |
Inc. (mb) | 21.84 | 30.81 | 30.40 | 34(3) |
9Be(12C,10B ) X
Compared with p-shell SM, NCSM predicted larger inclusive cross sections, and in line with measurement
NCSM with NN+3N describe much better the measured cross sections to the T = 0 states than p-shell SM.
Inclusion of 3N is necessary to describe the measured trend of the partial cross sections.
However, NCSM calculations with realistic nuclear forces overestimate the T = 1 parts.
Heavy-ion target
9Be or 12C
Proton target
Two types of Hammer
Probe: Knockout Reactions in Inverse Kinematics
25
Analysis of the 12C(p, pd)10B reaction
Deuteron kinetic energy:
Where
Determine whether it is a deuteron.
Extracting (p, pd) reaction pathways using kinematic conditions
(p,pd)
26
R. Subedi et al., Science 320, 1476(2008)
Pair knockout
Sequential
52Ca🡪51K* (Sn=4.9 MeV, Sp=16.6 MeV) 🡪50K+n
-1p
Evaporation-1n
Multiple possible process
Could we see np pair?
(p, 2pn) from neutron-rich nuclei @ 250 MeV/u
27
52Ca🡪50K Multiple comp.
(p, 2pn) from neutron-rich nuclei @ 250 MeV/u
Geant4 Simulations
52Ca🡪51K* 🡪50K+n
-1p
Sequential
Sequential
(p,pd)
C.L. Hao
52Ca(p,2p)51K*🡪50K+n
Evaporation
1n-evap.
sequen. + Pair
MINOS+SAMURAI @ RIBF
MINOS@RIBF
STRASSE @ RIBF
LH2+Si tracker
Decent angular resolution
Missing-mass & gamma Spe.
Multi-platform LH2 target
Development of the LH2 target for HIAF
H.N. Liu et al., EPJA 59, 121 (2023)
MF4
Stable Nuclei
Unstable
Primary beam from Booster
External target Area
SRC study along isotopic chain with (p, 2pn), (p, pd)
Under construction @BNU
Cold head
Target cell
Condensor
Changeable target arm
HIRIBL
29
Summary
Partial cross sections (Disentangle T = 0 & T = 1 np pair)
1. R(σT = 0/σT = 1) = 5.6(5), suggesting a stronger T = 0 np correlations.
2. Compared with the theory:
SM calculations with WBP interactions describe well T = 1 NN removal.
but underestimate the T = 0 np removal by a factor close to 2.
🡺 Insufficient treatment of T = 0 np correlations in the p-shell
NCSM calculations with NN+3N provide a much better description of the
measured partial cross sections to the T = 0 states than the p-shell model.
9Be(12C,10Be + γ) X
9Be(12C,10B+ γ) X
Probe: Two-nucleon knockout reactions from 12C at 190 MeV/u
Obtain the first exclusive np-removal data with the γ+residue measurement
Evaporation contribution in np-removal is significant and such components could not be directly identified when using HI target.
QFS with proton target is a promising tool, the (p,2pn) data analysis is ongoing…
Backup slides
Counts/ 30keV
9Be(12C,10Be + γ) X
Add-back Reconstruction was also performed.
Fit function:
Response functions(GEANT4)+Exponential background
pp removal from 12C
J, T, E, T1/2 & decay branching ratios are known. (Only states with positive parity are considered)
32
Analysis of gamma spectrum
Consider fitting the ¹⁰B gamma spectrum:
Response function of the excited state of ¹⁰B
Background
Low-energy background caused by protons produced in the reaction
Low-energy background caused by beam bombardment of the target (primarily bremsstrahlung) .
Simulated using R3BROOT
Consider using a double-exponential background
Gamma spectrum of 11B following 12C(p,2p) 11B*
Constraining the Shape and Counts of a Double-Exponential Background Using the Gamma Spectrum of 11B
Uncertainty of the fitting:
Statistical Error in Experimental Spectrometer Counting
Errors Resulting from Different Constraint Methods for Dual-Exponential Background
Uncertainty arising from the inclusion of the proton background
33
(p, 3p) reactions in neutron-rich
nuclei @ 250 MeV/u
Sequential
Pair K.O. + Breakup =5~15%
A. Frotscher et al., PRL 125, 012501(2020).
Only Angular distribution
🡺Dominance of sequential
R. Subedi et al., Science 320, 1476(2008)
81Ga🡪80Zn* (Sn=6.3 MeV)
(Sp=16.5 MeV)
-1p
First exclusive np-removal data
Residues | Jπ | T | σexp.(mb) |
10Be | 0+ | 1 | 3.9(3) |
| 2+ | 1 | 4.0(2) |
| 2+ | 1 | 0.9(1) |
| 0+ | 1 | 0.3(1) |
Inclusive |
|
| 9.1(3) |
10B | 3+ | 0 | 20.3(12) |
| 1+ | 0 | 10.3(6) |
| 0+ | 1 | 2.7(2) |
| 1+ | 0 | 3.8(3) |
| 2+ | 0 | 1.9(3) |
| 2+a | 1 | 2.9(3) |
Inclusive |
|
| 42(2) |
p
T = 0&1
p
n
T = 1
Partial cross sections
Large cross section to T = 0 3+ state in np removal (20/42 mb)
🡪Indicate a strong
splin-aligned np paired
configurations in 12C
np-removal:
T = 1 6.2(4) mb
T = 0 36(1) mb
R(σT = 0/σT = 1) = 5.9(4)
🡪Shown stronger T = 0 np correlations
v
R(σ-np/σ-pp) = 4.6(3)
pp-removal:
T = 1 9.1(3) mb
J=3
J=3
J=3
J=3
p
Comparison with Theory
J=3
J=3
J=3
R(σnp/σpp) = 4.6(3)
Structure:
TNA from p-shell SM
Reaction: Eikonal theory
Two-nucleon amplitudes (TNA)
Theoretical cross sections:
Data: 190 MeV/u@9Be
Theory: 250 MeV/u @12C
Partial cross sections to T = 1 states could be reasonably reproduced by the theory.
While that to T = 0 states are broadly underestimate by the theory by a factor of 2.
pp removal
np removal
Partial cross sections to T = 1 states could be reasonably reproduced by the theory.
While that to T = 0 states are broadly underestimate by the theory by a factor of 2.
described in p-shell shell model.
🡪 Insufficient treatment of T = 0 np
correlations in SM or Eikonal theory
ab initio no-core shell model (NCSM)
10B | σWBP | σNCSM(NN+3N) | σNCSM3(NN) | σexp. |
Inc. (mb) | 21.20 | 29.91 | 29.51 | 42(2) |
9Be(12C,10B ) X
Compared with p-shell SM, NCSM predicted larger inclusive cross sections, but still insufficient to describe the data.
Discrepancy between theory and data mainly arises from the GS.
#1 Structure:
The large partial cross section to the ground state indicates an enhanced collectivity in 12C.
0p3/2
0p1/2
1s1/2
0d5/2
0d3/2
0f7/2
Role of 3N Forces
9Be(12C,10B ) X
However, NCSM with NN+3N still cann’t reproduce the data quantitatively.
3N forces
3N is also necessary to predict the right trend of the measured partial cross sections.
3N is necessary to describe the energy level of 10B.
Eikonal Theory for 2N Removal
β1
β2
Target
9Be
12C
Projectile
b
surface collision
Eikonal model:
Only consider the interactions between (β1,Target), (β2,Target) & (Residue,Target)
Interaction between (β1, β2) are missing.
12C( e, epN )@4.627GeV
Incl. | (mb) |
σ-p | 82(2) |
σ-n | 62(2) |
σ-np_SRC | ~30 |
σWBP | 21.20 |
σ-np | 42(2) |
1N removal in Eikonal theory
2N removal in reality
#2 Eikonal model:
Removal of short-range correlated pair is missing.
R. Subedi et al., Science 320, 1476(2008)
39
Summary
Partial cross sections (Disentangle T = 0 & T = 1 np pair)
The measured inclusive 1N&2N removal cross sections from 12C in our work show reasonable consistency with previous results.
Inclusive cross sections
1. R(σT = 0/σT = 1) = 5.9(4), suggesting a stronger T = 0 np correlations.
2. Compared with the theory:
T = 1 NN removal: σexp~ σth T = 0 np removal: σexp~ 2σth
Such discrepancy shows that either the T = 0 np correlations in the SM is
insufficient or the reaction mechanism of SRC pairs removal is missing
in the Eikonal model.
3. NCSM calculations: Discrepancy between data and theory mainly arises
from the T = 0 3+ GS. 3N is necessary to predict the right trend of the measured partial cross sections.
9Be(12C,10Be + γ) X
9Be(12C,10C+ γ) X
9Be(12C,10B+ γ) X
Probe: Two-nucleon knockout reactions from 12C at 190 MeV/u
Obtain the first exclusive np-removal data with the γ+residue measurement
40
Collaborators
RIKEN J. Lee, H. Liu, P. Doornenbal, N. Inabe, T. Isobe, T. Kubo, S. Kubono, T. Motobayashi, M. Nishimura, H. Otsu, H. Sakurai, H. Sato, Y. Shimizu, H. Wang, S. Takeuchi, K. Yoneda
CNS/ Unvi. Of Tokyo
M. Matsushita, D. Steppenbeck
NSCL/ MSU B. A. Brown
TRIUMF P. Navratil
Tohoku Univ.
T. Kobayashi
Tokyo Tech.
Y. Kondo, N. Kobayashi, R. Minakata, T. Nakamura, S. Ogoshi, Y.Togana
RCNP, Osaka U.
N. Aoi
LPC de CAEN
J. Gibelin, S. Leblond�
Univ. of Kyoto
Y. Matsuda R. Minakata
Seoul National Univ.
J. Hwang
Theory Collaboration:
Univ. of Surrey
J. A. Tostevin, E.C.Simpson
LBNL
A. O. Macchiaveli, P. Fallon
PKU H. Liu, Yanlin Ye
Thank you very much for your attention!
4 types of Nucleonic pairs
Neutron-Proton Pair Correlations
Isoscalar (T=0, S=1) np pair
(deuteron-like)
🡪 new phase of nuclear matter
Well defined from the
isospin symmetry
pp
nn
np
np
T = 1, J = 0
T = 0, J > 0
Isoscalar
Isovector
Only 60~70% p involves the “Independent particle motion”
Long-standing ambitions:
Obtaining direct information of T = 0 np pair correlations
(e, eꞌp) reactions
Mean Field
Important ingredient:Pair Correlations
n & p in the same valence shell
(deutron-like)
A lot of uncertainties
N = Z system: A dominance of np pair
Correlations
L. Lapikas et al., NPA 553, 297c(1993).
43
Drip-line nucleus
Nuclear Structures Driven by Nuclear Forces
How do nuclear forces evolve with Isospin asymmetry?
Independent Particle Model
Shell structure & Magic numbers
(Mayer & Jensen
1963 Nobel Prize)
How do nuclear structures change with Isospin asymmetry?
Mean field: Woods-Saxson
+ Spin-Orbital Interaction
Mean Field
Correlations
Stable Nuclei
Sp Sn~8 MeV
20MeV
Sn < 1 MeV
Two-nucleon Knockout Reactions in Inverse Kinematics
1
2
Target
9Be/12C
12C
Projectile
b
surface collision
Core survival and nucleon “removal”🡪
Only affect the nucleon near surface
High incident energy🡪
Spectator (eikonal reaction model)
Momentum Distribution
Cross Section
Gain Direct Spectroscopic Information
Total J of the removed pair of nucleons
Spatial overlap of the removed two nucleons
E.C. Simpson et al., PRL 102,132502(2009)
2+
4+
0+
4+
Fig. 1 Calculated P// of 26Ne after pure π[d5/2]2 two proton removal from 28Mg at 82 MeV/u
🡪 A promising tool for systematic study of np correlations in N=Z nuclei
Electron-induced 2N removal reactions : study stable nuclei.
Cross section of 2N transfer reaction is small.
Beam energy (>100 MeV/u)
Background shape of γ spectrum
12C(9Be, X)9Be
The adopted exponential background shape in the analysis is reliable.
9Be(-2pn): Ybg
10B(-np) : Ybg
10Be(-2p) : 1/2Ybg
🡪Ybg mainly depends on the removed neutron.
Only the ground state of 9Be is bound.