A Monte Carlo approach to the study of medium-light...
Transcript of A Monte Carlo approach to the study of medium-light...
A Monte Carlo approach to the studyof medium-light hypernuclei properties
Diego Lonardoni
University of Trento - Physics DepartmentINFN - Gruppo Collegato di Trento
December 16, 2011
1. The method• DMC• DMC for nuclei: AFDMC
2. Hypernuclei• hyperon-nucleon interaction• AFDMC for hypernuclei
3. Preliminary results
4. Conclusions and perspectives
Outline
Diffusion Monte Carlo
� =it
� � ⇤
⇤�⇥(R, �) = H⇥(R, �)
⇥(R, �) = e�(H�E0)�⇥(R, 0)
=⇥�
n=0
cne�(En�E0)�⇤n(R)
�(R, 0) =��
n=0
cn⇥n(R)
lim��⇥
⇥(R, �) = c0⇤0(R)
DMC = projection method
Diffusion Monte Carlo
⇥(R, � + d�) = �R|⇥(� + d�)⇥
=
⌅�R| e�(H�E0)d�
⇤⇤R⇥⇥⌥ ⌃⇧ �
G(R,R�,d�)
�R⇥|⇥(�)
⇥dR⇥
walkers
potential term
d� d�
kinetic term
d�
Nucleon-nucleon interaction
2 body
3 body
Nucleon-nucleon interaction
Vij =n�
p=1
vp(r)Opij
2 body
3 body
Op=1,8ij = {1,�i · �j , Sij ,Lij · Sij}� {1, ⇥i · ⇥j}
Op=9,14ij =
⇤L2ij , L
2ij (�i · �j) , (Lij · Sij)
2⌅� {1, ⇥i · ⇥j}
Op=15,18ij =
�Tij , (�i · �j)Tij , Sij Tij , �
zi + �zj
⇥
Vijk = CSW2⇡ O2⇡,SW
ijk + CPW2⇡ O2⇡,PW
ijk + C�R3⇡ O3⇡,�R
ijk + CRORijk
Auxiliary Field Diffusion Monte CarloProblem:
P � e�12�d⇥O
2
e�12�d⇥O
2
=1�2�
�dx e�
x2
2 +⇥��d⇥xO
Idea: Hubbard-Stratonovich transformation
� �= A�⇤
i
ci · ⇥i
⇥
auxiliary fieldMC calculation
� A!
Z!(A� Z)!4A components
Auxiliary Field Diffusion Monte CarloAV6: Op=1,6
ij = {1,�i · �j , Sij}� {1, ⇥i · ⇥j}⇤ ⇥� ⌅VSD+VSI
VSD =1
2
A�
n=1
3�
�=1
�(⌅)n O(⌅)2
n� A(⌅)i,j : A�A
+1
2
3A�
n=1
�(⇤)n O(⇤)2
n A(⇤)i�,j⇥ : 3A� 3A
+1
2
3A�
n=1
3�
�=1
�(⇤⌅)n O(⇤⌅)2
n� A(⇤⌅)i�,j⇥ : 3A� 3A
rotation of spin-isospin states
15A auxiliary fieldsgood for Hubbard-Stratonovich
Hypernuclei
single �hypernucleus
double �hypernucleus
� = u+ d+ s
HypernucleiPANDA @ FAIR- anti-proton beam- double �-hypernuclei- �-ray spectroscopy
STAR @ RHIC- HI collider- anti �-hypernuclei- exotica?
JLAB- electron-production- single �-hypernuclei- �-wavefunction
SPHERE @ JINR- heavy ion beams- single �-hypernuclei- weak decay
BNL- heavy ions beams- anti-hypernuclei- single �-hypernuclei- double �-hypernuclei
ALICE @ LHC- URHIC collider- anti �-hypernuclei- exotica?
KEK � J-PARC- intense K� beams- single and double �-hypernuclei- �-ray spectroscopy for single �
KAOS @ MAMI C- electron-production- single �-hypernuclei- �-wavefunction FINUDA @ DAFNE
- e+e� collider- stopped-K� reaction- single �-hypernuclei- �-ray spectroscopy
HypHI @ GSI- heavy ion beams- single �-hypernuclei
at extreme isospins- magnetic moments
BNL JLABKEKJ-PARC
2010 2020
ALICEPANDASTAR
SPHEREFINUDAHypHI
2000
KAOS
Hypernuclei
H. Ðapo, B.-J. Schaefer, and J. Wambach. Appearance of hyperons in neutron stars. Phys. Rev. C, 81(3):035803, Mar 2010
Hypernuclei
H. Ðapo, B.-J. Schaefer, and J. Wambach. Appearance of hyperons in neutron stars. Phys. Rev. C, 81(3):035803, Mar 2010
Hyperon-nucleon interaction
2 body
3 body
[1]
Hyperon-nucleon interaction
V⇤i
(r) = v0(r) + v0(r)"(Px
� 1) +1
4v�
T 2⇡
(m⇡
r)�⇤ · �i
v0(r) = vc(r)� v2�(r)
vc(r) = Wc
�1 + e
r�r̄a
⇥�1
v2�(r) = v̄ T 2� (m�r)
2 body
3 body HS ok!only 2-body operators
HS ok!
V⇤ij = CSW2⇡ O2⇡,SW
⇤ij + CPW2⇡ O2⇡,PW
⇤ij + CDOD⇤ij
[1]
The idea
hypernucleus
nucleus �nuc = DetN JNN
�hyp = DetN JNN Det� JN�
B� =⇥�nuc|HN |�nuc⇤⇥�nuc|�nuc⇤
� ⇥�hyp|HN +H�|�hyp⇤⇥�hyp|�hyp⇤
propagator via HS auxiliary fields15A+ 3A ·A�
information about the hyperon-nucleon interaction
Hyp: nuclear effects cancel
The idea: behind the scene
Startingpoint:
good wave function
robust method for nuclei +
different AFDMC approaches
different single particle orbitals
work in progress
present and future collaborations
-33.0
-32.9
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-32.5
-32.4
-32.3
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-32.1
-32.0
-31.9
-31.8
-31.7
-31.6
0e+00 1e-05 2e-05 3e-05 4e-05 5e-05 6e-05 7e-05 8e-05 9e-05 1e-04
ener
gy [M
eV]
do [1/MeV]
4He binding energy
V4’ potential
Code PsiT-weight Skyrme.orbCode PsiT-weight HF-B1.orbCode Elocal-weight HF-B1.orbCode PsiT-weight HF-V4p.orb
The idea: behind the scene
GFMCPhys.Rev.Lett.89182501-1:4(2002)
The idea: behind the scene
-34.0
-33.0
-32.0
-31.0
-30.0
-29.0
-28.0
-27.0
-26.0
-25.0
-24.0
-23.0
-22.0
-21.0
-20.0
-19.0
-18.0
0e+00 1e-05 2e-05 3e-05 4e-05 5e-05 6e-05 7e-05 8e-05 9e-05 1e-04
en
erg
y [
Me
V]
d! [1/MeV]
4He binding energy
V6’ potential
Code PsiT-weight HF-B1.orb
Code Elocal-weight HF-B1.orb
Code Elocal-weight Skyrme.orb
Code Elocal-weight HF-V6p.orb
GFMCPhys.Rev.Lett.89182501-1:4(2002)
Hypernuclei preliminary results
0.50
1.00
1.50
2.00
2.50
3.00
3.50
4.00
4.50
5.00
5.50
6.00
6.50
7.00
0e+00 1e-05 2e-05 3e-05 4e-05 5e-05 6e-05 7e-05 8e-05 9e-05 1e-04
ener
gy [M
eV]
do [1/MeV]
5RHe R-separation energy
V4’+VRN HF-B1.orb
V6’+VRN HF-B1.orb
V4’+VRN+VRNN HF-B1.orb
V6’+VRN+VRNN HF-B1.orb
3 body⇤NN
exp
[2] Journal of Physics G: Nuclear and Particle Physics, 32(3):363-373, 2006
[2]
Hypernuclei preliminary results
0.00
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.10
0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0
dens
ity [1
/fm3 ]
r [fm]
5RHe density
N-density V4’+VRN HF-B1.orbR-density V4’+VRN HF-B1.orb
Hypernuclei preliminary results
0.00
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.10
0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0
dens
ity [1
/fm3 ]
r [fm]
5RHe density
N-density V4’+VRN+VRNN HF-B1.orbR-density V4’+VRN+VRNN HF-B1.orb
3 body⇤NN
Hypernuclei preliminary results
0.00
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.10
0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0
dens
ity [1
/fm3 ]
r [fm]
5RHe density
N-density V6’+VRN HF-B1.orbR-density V6’+VRN HF-B1.orb
Hypernuclei preliminary results
0.00
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.10
0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0
dens
ity [1
/fm3 ]
r [fm]
5RHe density
N-density V6’+VRN+VRNN HF-B1.orbR-density V6’+VRN+VRNN HF-B1.orb
3 body⇤NN
Hyp: ok!
Conclusions and perspectives
AFDMC algorithm can be easily extended to the study of hypernuclear systems
development of an accurate hyperon-nucleon potential
development of an accurate hyperon-hyperon potential
study of heavier -hypernuclei: , � 17�O7
�He
study of -hypernuclei: 6��He��
Conclusions and perspectives
To do(high priority)
deeper investigation in the AFDMC algorithm
better trial wave function
single particle orbitals
correlation functions
Thank you
[1] Hypernuclear potentials:
A. A. Usmani, Steven C. Pieper, and Q. N. Usmani. Variational calculations of the –separation energy of the hypernucleus. Phys. Rev. C, 51(5):2347–2355, May 1995.
A. A. Usmani and S. Murtaza. Variational Monte Carlo calculations of hypernucleus. Phys. Rev. C, 68(2):024001, Aug 2003.
A. A. Usmani. N space–exchange correlation effects in the hypernucleus. Phys. Rev. C, 73(1):011302, Jan 2006.
5⇤He
5⇤He
⇤
⇤17⇤O