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Symposium on Astro -Particle and Nuclear Physics. In Honour of 70th Birthday of Prof. Q.N. Usmani. 9/13/2014. 1. Professor M. Z. Rahman Khan. Energies of multi-strange α -cluster hypernuclei using variational Monte Carlo Method. MOHAMMAD SHOEB - PowerPoint PPT Presentation
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104/21/23 1
Symposium on Astro-Particle and Nuclear Physics
In Honour of 70th Birthday of
Prof. Q.N. Usmani
04/21/23
04/21/23 2
Professor M. Z. Rahman Khan
04/21/23 3
404/21/23 4
Energies of multi-strange α-cluster hypernuclei using variational Monte
Carlo Method
MOHAMMAD SHOEB
Department of Physics, Aligarh Muslim University, Aligarh-202 002,
India
04/21/23
504/21/23 5
Outline
1.Introduction2. Hamiltonian in α-cluster model3. Potential models4.Variational wavefunctions5. Results and discussion6. Summary
04/21/23
604/21/236
1. Introduction:Aim of nuclear physics
Complete knowledge of the interaction among octet of baryons in a unified way
04/21/23
7
Motivation of studying Strange and multi-strange hypernuclei
• to extract interaction between hyperon-N and hyperon-hyperon
Existence of hypernuclei represent a new state of matter may exhibit new symmetries,
selection rules, etc.
04/21/23
8
Presence of hyperon(s) may modify the properties of the core
moment inertia of deformed nucleus rotational and vibrational states structure of
nucleusHypernucleus provides us a opportunity to
investigate properties of hyperon(s) in nuclear medium
Hyperon(s) inside nuclei may be used as probe to study the nuclear structure
04/21/23
904/21/23 9
It is believed that hyperons matter forming the inner core of neutron stars would have significant effect on their properties.
Schaffner-Bielich [NP 804(2008)309 and ref. their in ] has discussed that hypernuclear potential depths, two-body hyperon- nucleon and hyperon three-body forces as well as hyperon-hyperon interaction would
04/21/23
10
Therefore, determination of hyperon- nucleon and hyperon-hyperon interaction becomes very important for investigating
the properties of neutron stars.
have a impact on the maximum mass, mass-radius relation, and cooling properties of
neutron stars.
04/21/23
11
Hypernuclear physics is likely to play key role in the study: Properties of neutron stars
Equation state of nuclear matter Figure in the next slide shows interdisciplinary
nature of hypernuclei linking particle, nuclear, many-body, astrophysics etc.
[ref. Erni et al arXiv: hep-ex/0903.3905]04/21/23
1204/21/23
1304/21/23 13
Segr tablee
04/21/23
14
Extension of the nuclear chart in a new dimension, strangeness S
04/21/23
15
-Hypernuclear events
, ( ground and excited states), or
(Hida event ) and
He6 Be10
Be11
Be12 B13
04/21/23
16
Hypernuclear experiments planned or operative at various (nine) laboratories all over the World
04/21/23
17
Experimental facilities for hypernuclear physics program
List of a few leading laboratories where
Hypernuclear physics program to produce and identify hypernuclei with strangeness S= -1 to -3 is being pursued
• TJNAF(Thomas Jefferson National Accelerator Facility) at
Newport news in USA
Electro-production
• FINUDA(FIsica NUclearea DA NE): A special accelerator,
DA NE (Double Annular ring For Nice Experiment), designed at INFN (Instituto Nazionale di Fisica Nucleare)
Kepe
04/21/23
1804/21/23 18
e e510
MeV510
MeV
(M=1020 MeV, 20
2310 s)
Head on collision
decays
),( 00 KK
),( KKCopious production
A beam of of extremely high intensity and precise low energy is expected to insert “strangeness” inside nucleus to
produce hypernuclei.
K
ZZK AAStop
04/21/23
19
• J-PARC(Japan Proton Accelerator Research Complex) at
KEK: Already a rich data related to both the spectroscopy and
decay of hypernuclei at KEK have been measured.
Program for production and unambiguous identification of
hypernuclei and excited states using reaction
( )
Excited states of double-Λ hypernuclei
04/21/23 19
KK ,
04/21/23
20
• ANDA ( ANnihilation at DArmstadt ): A
beam hits primary target to produce
;
Stopping and absorption of in the
secondary target produce hypernucei.
Program to produce S= -3, -hypernuclei
04/21/23 20
P P p
pp 0np
04/21/23
21
MeV 28 p ppIn primary target In secondary target, e.g. Li, Be, B,
Schematic picture describing production of double Λ hypernuclei at PANDA
04/21/23
22
Multi-strange hypernuclei
Schaffner et al [Ann. Phys.(NY)235(1994) 35 ] observed that a would become particle stable against the strong decay
if a sufficient number of bound ’s Pauli blocked this decay mode. Thus
is the lightest system suggested to study. At present production of multi-strange hypernuclei seems to be impossible.
04/21/23 22
N
)4(7 SHe
04/21/23
23
However, it will interesting to theoretically study the stability of multi-strange systems. Such a study is likely to have implication on future experimental efforts in producing,
identifying and measuring the properties of multi-strange hypernuclei.
Therefore, we have included in our study multi-strange hypernuclei apart from strange
ones.
04/21/23
2404/21/23 24
2. Hamiltonian in α-cluster modelHypernuclei studied in the α-cluster model using VMC
s-shell:
p-shell:
Systems within rectangular boxes are the ones whose stability predictions are to be made.
,6He He7
,9Be
,11Be ,13C
,9Be ,10Be),2/5,2/3(*9 Be ),2(*10
Be
,10Be ,13C C14),2(13
C
04/21/23
25
Hamiltonian for the five-body system in Ξαα model with α treated as rigid:
Be11
4
5
α
α
Ξ
3
2
1Λ
Λ
5
412
2
1
)()(
)3()(
i
i
rViK
KiKH
04/21/23
2604/21/23 26
2
1
2
1
5
4
5
44533 )()()()(
i i j iiiji rVrVrVrV
),(2
154
iii rrV
…..(1)
hK K. E. operator , 21hhV potential energy for the
21hh
V; phenomenological
dispersive three-body potential with Yukawa
form factors.
the particle pair
04/21/23
2704/21/23 27
Hamiltonian for
5
312
2
1
)()()(ii
rViKiKH
C14 in ΛΛααα model
2
1
5
3
5
3
2
1
5
3
5
),()()(i j
jkijkji j ji
ijij rrVrVrV
),( 45,3534 rrrV3
4
5
1
2
….(2) α
αα
Λ
Λ:V phenomenological repulsive
three-body potential with
Gaussian form factors
04/21/23
2804/21/23 28
3. Potential Models
3.1 Two-body potentialsThree-range Gaussian BB(=ΛΛ, Ξ) potentials in spin state (=s,t)
….(3)
(7.26 MeV)
04/21/23
2904/21/23 29
Potentials
For =
04/21/23
3004/21/23 30
Potentials
04/21/23
3104/21/23 31
…(4)
(4)
04/21/23
3204/21/23 32
potentials for l th partial waves that fit scattering phase shifts. potential of Chien and Brown has been used for only as the energy is not very sensitive to the choice of the potential.
V
Ali-Bodmer
potentials
Be9
04/21/23
3304/21/23 33
Two-range Gaussian potentials
•Isle fits of and its weak decay
modes
B He5
•MSA is obtained from Brueckner-Hartee-Fock
Theory and slightly modified to fit
of
[Euro. Phys. J. 16(2003)21]
B He5
04/21/23
3404/21/23 34
…..(5)
04/21/23
3504/21/23 35
0V B
V
(4). In the previous slide its graph
is shown by black color line.
WS24 with = 24.0, as suggested by Dover and Gal [Ann.Phys. 146 (1983 )309], has been obtained from a analysis
of old and ambiguous data B
energy = -2.09 MeV for WS24 and Isle potential
= -0.06 MeV for WS14
0V
04/21/23
3604/21/23 36
3.2 Phenomenological Three-body potential among
and clusters
Microscopic calculations of Bodmer and Usmani
for shows that contribution of dispersive
three-body NN force for the triad
where one nucleon from each is participating
Be9
21NN
1N
2N
04/21/23
3704/21/23 37
is quite significant, neglecting it among cluster
overbinds and . In cluster model calculation we [Pramana68 (2007)943] have proposed to simulate phenomenologically the dispersive energy in the triad through a simple form
(6)
)()(210 rfrfWV
Be9 Be10
. arar /)exp(
04/21/23
3804/21/23 38
and .
Phenomenological three-body potential
gives good fit to the binding energy and rms radius of
in the cluster model for AB [ NP 83(1966)66 & phys
Lett B 389(1996)631] potential.
C12
15.0 fma
( 7)
04/21/23
3904/21/23 39
4.Variational wavefunctions Construction of good trial wavefunction• Physics necessary to describe the ground and excited state• Reasonably efficient to compute Wavefunctions are product of two-body correlation functions and the appropriate spin functions
4.1 Wavefunctions
(i) and model
g.s. ,degenerate doublet and ,
. Replacing by gives w.f. for .
)(rfhh
Be9
)2/1,2/1(),( zJJ 021l
)2/3,2/3(),( zJJ )2/5,2/5(
221l
:)2/5,2/3(*9 Be
Be9
04/21/23
4004/21/23 40
(ii) and : model
g.s. , excited state ,
(iii) and : model
g.s. , degenerate doublet ,
Be10 )2(*10
Be
)0,0(),( zJJ 021l )2,2(),( zJJ
221l
C13 )2/5,2/3(13
C
),2/1( m 021l
)2/5,2/3( 221l
04/21/23
4104/21/23 41
Replacing by gives w.f. of . (iv) Wavefunctions for , and
(a) wavefunction for in model:
=
C13
,6He He7 ,10Be
Be11
Be11
JJ z
)(43lmY
m
m
2/1
2
1
2100 )()(
04/21/23
4204/21/23 42
(b) Wavefunction for : suppress a and a indices
in the wavefunction of in (a) above
(c) Wavefunction for : suppress a index
in the wavefunction of in (a) above
(d) Similarly wavefunction for can be obtained.
He6
Be11
He7
Be11
,10Be
04/21/23
4304/21/23 43
4.2 Calculation of correlation function
A procedure developed by Urbana group. Solution of the following Schroedinger type equation
etc.
pair .
Potential between particles .
)(rf hh
hh
hh
04/21/23
4404/21/23 4404/21/23
4504/21/23 45
04/21/23
4604/21/23 46
5.Procedure for energy calculation
( 8 )
For local operator H the energy can be written in a formsuitable for Monte Carlo calculation. Defining local energy
04/21/23
4704/21/23 47
and a multivariate probability distribution
( 9)
The variational energy is written as
(10 )
04/21/23
4804/21/23 48
(11)
General procedure for calculation of energy in VMCmethod:
(12)
04/21/23
4904/21/23 4904/21/23
5004/21/23 50
The energy is evaluated using
(i) model of : and
(ii) model of : and
(iii) model of : and (iv) model of : and
Similarly for other hypernuclei
He6 N
He7 N
N
,9Be
Be10 N
04/21/23
5104/21/23 51
To explore the structure of and
The quadrupole moment ( ) in the cluster model
is calculated using
where runs over coordinate of two s, treated as point particles
and distances are being measured from the cm of two alphas.
Be9 Be10
2efm
i
04/21/23
5204/21/23 52
5. Result and Discussion
VMC energy: s-Shell Hypernuclei and
NSC97e
,
:ESC00, ND, NSC97b
He6 He7
He6
He7
V
04/21/23
5304/21/23 53
: Isle and WS
= 2.09 MeV , =3.45 (Isle) and 3.36 (WS) fm
( ) fm for WS24
Isle WS
(12.6, 2.93) (4.8, 2.2)
00
B
00 , ra
0R
0potentials
04/21/23
5404/21/23 54
Filikhin et al
Faddeev
Faddeev-Yakubovsky
predicted for unbound for Isle soft
replusive potential bound for WS24 potential
Prediction: binding energy
capable of discriminating between radial shape of central
potentials, very unlikely, as this violates shape independence of
low energy data
He7
0
He6
He7
He7
04/21/23
5504/21/23 55
potential dependent configuration for
stronger potential a configuration speculated
i.e. screened by . configuration for weaker potential
Detailed VMC calculation
:ESC00, ND, NAGSIM, NSC97e, NSC97b
:NSC97e
: Isle , WS24, WS14
He7
0)( 0 )( 0
V
0V
0V
04/21/23
5604/21/23 56
F and FY [Filikhin et al JPG35(2008)] bold face within round bracket
04/21/23
5704/21/23 57
Our VMC calculation demonstrates and have
negative energies and is bound for WS24 and Isle
potential ( while is unbound for Isle potential in F-Y
method) .
Gross property such as energy, not good discriminator of the
shapes of the two-body potential.
is unbound for WS14 potential.
Due to strong conversion process ,we will comment
on stability of in the last.
He6 He7
He7
He7
He7
NHe6
04/21/23
5804/21/23 58
04/21/23
5904/21/23 59
0
Pyramid on triangular isosceles base
Isosceles plane
Two planes
ESC00, NAGSIM, NSC97b
,R ,R R RandArms
in general increase with decrease in
strength of potential
but no change in the configuration
04/21/23
6004/21/23 60
)()( 76 HeSHeS
)(
being screened by two lambdas
our calculation support not )(
as opposed to speculation of Filikhin et al
configuration whether interaction is weak or strong
.[JPG36(2009)045104]
04/21/23
6104/21/2361
p-Shell hypernuclei:
(i) , , , and
Experimental =6.71 MeV
=17.6 0.4 MeV ( 14.5 0.4 MeV assuming
, a ray of about 3.0 MeV must have escaped the identification of decay product from the emulsion ).Excited states:
=3.66 MeV
Demchi-Yanagi event
= MeV
Be9 Be10
C13 C14
)( 9BeB
)( 10BeB *910 BepBe
))2/5,2/3(( 9 BeB
))2(( 10 BeB 35.0
21.033.12
C130
04/21/23
62
Revised = 11.90 0.13 MeV
=11.69 MeV
))2(( 10 BeB
)(13CB
04/21/23
6304/21/23 63
and of three-body potential are
adjusted to fit ground state energy
0W
Ali-Bodmer [Chien-Brown]
a0W
potential
04/21/23
6404/21/23 64
No free potential parameters
04/21/23
6504/21/23 65
No free potential parameters
Isle+AB
MSA+AB
04/21/23
6604/21/23 66
No free potential parameters
Demchi-Yanagi event B =12.33 MeV
04/21/23
6704/21/23 67
-Ve quadrupole moment for : Oblate shape
: Experimental Q =5.3
N replaced by
Prolate Oblate
Not much difference between the calculated energy using AB and
CB alpha-alpha, Isle and MSA lambad-alpha interactions.
Therefore, we consider only AB alpha-alpha and Isle lambda-alpha
interactions.
)2/5,2/3(9 Be
)2/3(9 Be 2fme
)2/3(9 Be )2/5,2/3(9 Be
04/21/23
6804/21/23 68
= 11.69 MeV First we analysed sub system Ground state energy = -7.26 MeV Excited state energy = -2.84 MeV Energies of ( and ) calculated variationally in cluster
model. i) interaction(AB) very repulsive, gives energy -0.7 MeV.
ii) + parameters and
adjusted to fit the ground state. sitting at the vertices of
equilateral triangle.
)(13CB Experimental
)0(12 C
)2(12 CC12 0 2
MeVW 0.163 fm7.7V
V V
4.17 fm
C12
2.4fm
c.m.04/21/23
6904/21/23 69
Filikhin et al JPG35 (2008)
FY calculation with out
04/21/23
7004/21/23 70
and in < for (Shrinkage of core )
> in , wanders at the periphery of core
R C13 C12
)3(R
)3( R )3(R C13
04/21/23
7104/21/23 71
Variational energy VMC energy
(present work) = - 4.99 MeV
in alpha cluster model using
Jacobian-coordinate
MeV
Gaussian-basis function method
( Hiyama et al [Prog.Theo.Phys.97(1997)881] ).
)2(12 C
0-7.17
-4.29
2
C12
Exp. -2.84MeV
Exp. -7.26MeVJ
04/21/23
7204/21/23 72
Ground and degenerate doublet
Interaction (AB)+ (Isle) + +
(no free
parameter)
Exp. -7.26+(-11.69) MeV
C13 )2/5,2/3(
2/1
)2/5,2/3(
-18.81
-14.98 Prediction
V V
C13 JMeV
04/21/23
7304/21/23 73
: VMC prediction for G.S. energy in model
fits energy(-7.26 MeV) + Isle + (AB) VMC Energy =-31.29 MeV; Predicted binding of = -7.16- (-31.29)= 24.12MeV
C14
He6
B
VV V
C14
04/21/23
7404/21/23 74
in model :VMC Prediction
(Isle & WS) + +
C13 0
0 V V
Filikhin et al JPG35(2008)
04/21/23
7504/21/23 75
(ii) Prediction for the energies of and
Calculated energy of the above systems in and models using combinations of (Isle, WS24, Ws14), (NSC97e) and (NSC97( b,e), NAGSIM) potentials along with dispersive three-body force.
,9Be Be10 Be11
,0
0 0
0 0
04/21/23
7604/21/23 76
04/21/23
7704/21/23 77
04/21/23
7804/21/23 78
VMC energy for < Faddeev method
Due to interplay between Calculation limited to s-wave
two-body correlations ,
contribution from partial
waves higher than s-wave
is simulated.
energy for Isle and WS24 differ by 3%
for twice of
Separation energy in nearly independent of
strength.
Be9
Be10
B Be10 He6
Be11S
04/21/23
79
Do the negative energies of and implies stabilty ?
No
Due to strong conversion
depending on the depth of WS
potential, these systems can decay as:
;
Be10
He6
N0
HeHe 56
BeBe 910
04/21/23
8004/21/23 80
Calculated
level scheme
for two depths
of
potential.
It seems very
unlikely that
will ever
observed in
future experi-
mental effort.
0
Be10
04/21/23
81
Note: All the calculations where appears were performed for hyperon. To obtain binding of hypernucleus a coulomb correction 1.5 to 2.0 MeV per alpha particle is to be added to the binding of hypernucleus containing .
04/21/23 81
0
0
04/21/23
82
6.Summary• VMC for binding energy of three-, four-, and
five-body alpha cluster s- and p-shell hypernuclei
• First cluster model VMC calculation for predicting the energy of multistrange hypernuclei
• VMC energy for is insensitive to the shape of potential as opposed to Faddeev-Yakubovsky method
04/21/23 82
He7
04/21/23
83
• is unbound and stability depends on
potential depth• Predicted the energies for and for ground
state • , and are predicted to be stable for
WS14 • Demachi-Yanagi event is interpretted as excited
and exited state energy of degenerate doublet of explained.
)2(13 C
C14
Be90
C130
)2(10 Be
Be110
)2/5,2/3( Be9
Be100
He60
04/21/23
84
Thank you
04/21/23