Study on 1n halo nuclei from light to medium mass region
Shi-Sheng Zhang (张时声)
Beijing University of Aeronautics and Astronautics (Beihang University)
The 8th International Workshop on Nuclear Dynamics in Heavy-ion Reactions,
Taiyuan, Shanxi, August 21st-24nd, 2026.
Background & Motivations:Nuclear physics under extreme conditions
First p-wave halo nucleus
Heaviest
halo nucleus
stable
N halo
P halo
1n halo
2n halo
4n halo
Sn < 2 MeV
ρn dilute, radius increase, s/p wave
N
Y
N
large σR
N
Y
N
Y
narrow dσ/dp//
soft dipole resonance
Y
Y
N
HALO
Observables:
structure
reaction
Part I: CDFT + Glauber model for medium mass region�1n halo description from structure to reaction observables
37Mg
31Ne
43,45Si
The 8th International Workshop on Nuclear Dynamics in Heavy-ion Reactions,
Taiyuan, Shanxi, August 21st-24nd, 2026.
Year 2009
Year 2010 - 2012
Year 2014
History of p-wave 1n halo nuclei 31Ne & 37Mg
T. Nakamura, et al., PRL 103, 262501 (2009).
T. Sumi, et al.,
PRC 85, 064613 (2012).
Anti-symmetrized Molecular Dynamics (AMD)�+ double-folding model (DFM)
+ resonating group method (RGM)
W. Horiuchi, et al.,
PRC 81, 024614 (2010).
Skyrme-Hartree-Fock (SHF)� + Glauber Model
K. Minomo, T. Sumi, et al.,
PRL 108, 052503 (2012).
T. Nakamura, et al., PRL 112, 142501 (2014). April 7th.
S.S. Zhang, et al., PLB 730, 30 (2014). March 7th
Year 2014
Year 2022
Year 2024
History of p-wave 1n halo nuclei 31Ne & 37Mg
A unified description of the halo nucleus 37Mg from microscopic structure to reaction observables
J. L. An, …, S.S. Zhang, PLB 849, 138422(2024)
S. Watanabe, et al., PRC 89(4) 044610 (2014).
N. Kobayashi, T. Nakamura, et al., PRL 112, 242501 (2014). June 18th.
S.S. Zhang, S.Y. Zhong, et al. JPG 49, 025102 (2022).
S.Y. Zhong, S.S. Zhang, et al. SCPMA 65, 262011 (2022).
AMD+DFM+RGM FAILED!
A unified description from structure to reaction applicable for medium-mass region halo nuclei is strongly desired!
Goals
Spherical structure
(RAB)
Deformed structure
(DRHBc、D-RHFB )
Deformed reaction
(Glauber)
Spherical reaction
(Glauber)
Spherical reaction
(Glauber)
Deformed reaction
(D/TRHBc、NLEFT )
Step 1
Step 2
Step 3
Observables
JPG 2022. 01 cover article
SCPMA 2022.06
submitted
Radius, density distribution
cannot be directly detected
ZSS, MSS, ZSK, ZJ, PLB 730, 30 (2014).
Neutron density distributions (DD)
3/2-
RAB (RMF+ACCC+BCS) approach:
predict spin and parity for g.s. in 31Ne: 3/2-
confirmed by
T. Nakamura, et al. PRL 112, 142501 (2014).
Glauber model
Spherical Glauber model
B. Abu-Ibrahim, et al. CPC., 151(3) (2003) 369-386.
Phase shift χ
Reaction CS σ
Longitudinal momentum distribution dσ/dp//
Longitudinal Momentum distribution
Step 1 :
spherical + spherical
Reaction cross sections
Gaussian function fit
RAB density
deviations
ZSS, ZSY, SB, and MSS, JPG 49 (2022) 025102
Halo hints
JPG cover article
Density distribution
50 mb deviation
CDFT:RAB (s.p. resonant states + pairing) + spherical Glauber model
Solving the Dirac-Hartree(-Fock)-Bogoliubov equations have been achieved!
deformed
B. Abu-Ibrahim, et al. CPC., 151(3) (2003) 369-386. J. Hong, et al, PRC, 96(6) (2017) 064603.
Phase shift χ
Reaction CS σ
Longitudinal momentum distribution dσ/dp//
spherical
Step 2:
deformed + spherical
1n Removal CS
Momentum distribution
Improved
ZSY, ZSS*, et al. SCPMA, 65 (2022) 262011
Reaction CS
CDFT:DRHBc (axial deformed + pairing + continuum) + spherical Glauber model
50 mb deviation
DRHBc theory + Glauber model:
AJL, ZKY*, LQ, ZSY, ZSS*, PLB 849 (2024) 138422.
deformation + pairing + continuum
K. Y. Zhang, et al., PLB 844 (2023) 138112.
Highly cited in 2024
PC-F1
Exp. Data are taken from
Kobayashi N, et al.
PRL 112(24): 242501(2014).
momentum distribution
Reaction CS
Observables for 1n halo 37Mg
Step 3:
deformed + deformed
Impact
CDFT:DRHBc (axial deformed + pairing + continuum) + deformed Glauber model
deformed + deformed (NL1)
deformed + spherical
spherical + spherical
deformed + deformed (NL3)
31Ne + 12C
240 MeV/A
Improved by 20 mb
In between
β2=0.25
Summary I
Gaussian fitting
RAB densities
Realize a unified description of halo nuclei with medium masses�from microscopic structure to reaction observables
the best
JPG 49 (2022) 025102 cover
SCPMA 65 (2022) 262011
Agree with data , improved by 20 mb
in between
Improved by 50 mb
↔ dilute in coordinate space
Close to the upper limit of Exp. data
improved by 30%
improved by 26%
PC, AJL,…, ZSS*, ZKY*, PLB 877: 140487 (2026).
Predict deformed halo candidates
Exp. Data:
B. Hue, et al., Phys. Conf. Ser 934: 012058 (2017).
Y. Penionzhkevich, et al., KnE Energy 3: 21 (2018).
Same energy in center of mass coordinate
Key points in the reply to the PLB’s referee
Triaxial Relativistic Hartree-Bogoliubov theory in continuum(TRHBc)
Exp. Data:
M. Wang, et al., CPC 45: 030003 (2021).
H. Heylen, et al., PRC 103: 014318 (2021).
ZKY, etal.
PRC 108: L014301 (2023);
PRC 112: 044308 (2025).
CDFT:TRHBc (triaxial deformed + pairing + continuum) + spherical Glauber model
AJL, ZSS*, ZKY*, JPG 53(7): 075105 (2026).
Part II: NLEFT + Glauber model for light mass region�1n halo description from structure to reaction observables
The 8th International Workshop on Nuclear Dynamics in Heavy-ion Reactions,
Taiyuan, Shanxi, August 21st-24nd, 2026.
NLEFT(Nuclear Lattice Effective Field Theory): 11Be halo
Shihang Shen, et al., PRL 134, 162503 (2025)
Parity Inversion: 11Be Jπ (1/2+ )
From microscopic structure to reaction observables
NLEFT configurations
Deformed Glauber
Intrinsic density
Reaction observables
correlated A-body samples
configuration alignment
orientation-resolved S(b)
No fitted density parametrization
NLEFT + deformed Glauber model is valid for elastic scattering!
For p + ¹²C,
Predictions for ¹¹Be + ¹²C,
⇒ Larger transverse interaction radius
⇒ Signal of halo ¹¹Be with spatially extended valence neutron
Elastic differential cross sections for p + ¹²C and ¹¹Be + ¹²C at 800 MeV/A as a function of the momentum transfer q
Deformation can largely reduce σR(7-12Be + 12C / 9Be) by ~50 mb
⇒ clear signal of 1n halo for 11Be
Narrow longitudinal momentum distributions at 63 MeV/A and 790 MeV/A
790 MeV/A — predictions for future measurement!
the dσ/dp// for ¹⁰Be+n residues after 1n removal reactions are narrower than those for ⁸Be+n.
63 MeV/A — calculated shape agrees with the data
Colored band: uncertainty from Sn(exp) – Sn(NLEFT)
11Be: Sn = 0.5–1.9 MeV
10Be: Sn = 0.9–1.7 MeV
For light nuclei, NLEFT+deformed Glauber model works!
unpublished
1n halo
2n halo
JPG2026
PLB2026
SCPMA2022
JPG2022
JPG2025
EPJA2024
PLB2024
PLB2023
Systematic study on neutron-rich isotopes with 15<A<50 & 6<Z<14
Thanks for your attention!
NLEFT(Nuclear Lattice Effective Field Theory)
S. Elhatisari, et al., Nature 630, 59 (2024).
Densities from Pinhole Algorithm
S. Elhatisari et al., PRL 119, 222505 (2017)