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INTERNATIONAL PHD PROJECTS IN APPLIED NUCLEAR PHYSICS AND INNOVATIVE TECHNOLOGIES This project is supported by the Foundation for Polish Science – MPD program, co-financed by the European Union within the European Regional Development Fund
Three-Nucleon dynamics With
BINA detector
By:
Ghanshyam Khatri
Supervisors:
Prof. Stanisław Kistryn, (Jagiellonian University, Poland)
Prof. Nasser Kalantar-Nayestanaki, (KVI & University of Groningen, The Netherlands)
22 May, 2012 PhD Seminar @ Jagiellonian University
Self Intro
• from a small city SURAT, not far from Mumbai !
• Before coming to UJ : 2007, B.Sc. - Physics @ Navyug Sci. College (VNSGU) 2007, May-July, Summer Project @ BARC-Mumbai 2007-08, Sci. Asst. Job @ Inst. for Plasma Research, India 2008-10, Joint-European Master in Nuclear Fusion @ Ghent University, Belgium Nancy University, France Royal Institute of Technology, Sweden 2010-present
4
Introduction
How many known forces in Nature ?
1. Gravity (Newton’s apple) 2. Electromagnetic (Sun light) 3. Weak Nuclear (Fukushima & Chernobyl) 4. Strong Nuclear (Reactor & Bombs)
6
Introduction
How many known forces in Nature ?
1. Gravity (Newton’s apple) 2. Electromagnetic (Sun light) 3. Weak Nuclear (Fukushima & Chernobyl) 4. Strong Nuclear (Reactor & Bombs)
7
Introduction
How many known forces in Nature ?
1. Gravity (Newton’s apple) 2. Electromagnetic (Sun light) 3. Weak Nuclear (Fukushima & Chernobyl) 4. Strong Nuclear (Reactor & Bombs)
1935 (Yukawa-theory): ‘Meson exchange between two nucleon’
8
Ph
oto
Cre
dit
: Sc
ien
ce P
ho
to L
ibra
ry
Introduction
How many known forces in Nature ?
1. Gravity (Newton’s apple) 2. Electromagnetic (Sun light) 3. Weak Nuclear (Fukushima & Chernobyl) 4. Strong Nuclear (Reactor & Bombs)
1935 (Yukawa-theory): ‘Meson exchange between two nucleon’
1947 (Powell & his team ): ‘Experimentally found Meson’
9
Ph
oto
Cre
dit
: W
ikip
ed
ia
Ph
oto
Cre
dit
: Sc
ien
ce P
ho
to L
ibra
ry
Introduction
How many known forces in Nature ?
1. Gravity (Newton’s apple) 2. Electromagnetic (Sun light) 3. Weak Nuclear (Fukushima & Chernobyl) 4. Strong Nuclear (Reactor & Bombs)
1935 (Yukawa-theory): ‘Meson exchange between two nucleon’
1947 (Powell & his team ): ‘Experimentally found Meson’
10
Ph
oto
Cre
dit
: W
ikip
ed
ia
Ph
oto
Cre
dit
: Sc
ien
ce P
ho
to L
ibra
ry
Introduction
How many known forces in Nature ?
1. Gravity (Newton’s apple) 2. Electromagnetic (Sun light) 3. Weak Nuclear (Fukushima & Chernobyl) 4. Strong Nuclear (Reactor & Bombs)
1935 (Yukawa-theory): ‘Meson exchange between two nucleon’
1947 (Powell & his team ): ‘Experimentally found Meson’
Smoking Meson ??? 11
Ph
oto
Cre
dit
: W
ikip
ed
ia
Ph
oto
Cre
dit
: Sc
ien
ce P
ho
to L
ibra
ry
12
Modern phenomenological/meson exchange NN potentials:
Nijmegen I Nijmegen II CD-Bonn Argonne V18 …
…today after almost 6 decades !
Introduction
13
Modern phenomenological/meson exchange NN potentials:
Nijmegen I Nijmegen II CD-Bonn Argonne V18 …
…are able to explain the Interaction between two nucleons accurately e.g. np- & nn-scattering , deuteron (2H) properties
np-scattering
Experiment Theory ̶ ̶ ̶
. . .
High precision data from Los Alamos W. P. Abfalterer et al., PRL 81, 57 (1998)
…today after almost 6 decades !
Introduction
14
Modern phenomenological/meson exchange NN potentials:
Nijmegen I Nijmegen II CD-Bonn Argonne V18 …
…are able to explain the Interaction between two nucleons accurately e.g. np- & nn-scattering , deuteron (2H) properties
np-scattering
Experiment Theory ̶ ̶ ̶
. . .
High precision data from Los Alamos W. P. Abfalterer et al., PRL 81, 57 (1998)
…today after almost 6 decades !
Introduction
Most of the present NN-scattering data can be reproduced solely with 2NF models with χ2 /datum ~ 1, but…
15
np-scattering
Experiment Theory ̶ ̶ ̶
. . .
High precision data from Los Alamos W. P. Abfalterer et al., PRL 81, 57 (1998)
Introduction
…but FAILS to describe larger system (A>2) !
16
even for the simplest A=3 e.g. 3H and 3He ….unable to reproduce the data
np-scattering
nd-scattering
Experiment Theory ̶ ̶ ̶
. . .
High precision data from Los Alamos W. P. Abfalterer et al., PRL 81, 57 (1998)
Introduction
…but FAILS to describe larger system (A>2) !
Model Triton B.E. [MeV]
Nijm I 7.72
Nijm II 7.62
AV18 7.62
Reid-93 7.63
Exp. 8.48
H. Witala et al. PRL 81, 1183 (1998) St. Kistryn et al. PRC 68, 054004 (2003)
+
V12+V23 +V31=Vtheory
=
3N System
….a new notion: Three-Nucleon Force (3NF)
3NF = V123
~
Introduction
17
+
V12+V23 +V31=Vtheory
=
3N System
….a new notion: Three-Nucleon Force (3NF)
3NF = V123
~
….adding 3NF in original 2NF helps !
Model 3H [MeV] 4He [MeV]
2NF 7.62 24.2
2NF +3NF 8.47 28.3
Experiment 8.48 28.4
H. Witala et al. PRL 81, 1183 (1998) St. Kistryn et al. PRC 68, 054004 (2003)
CD-Bonn+TM99 AV18+Urbana XI
additional 3NF
Introduction
18
25
3N dynamics Three-body forces in a NUCLEAR system !
N
N
N
3
1
3
1
2
2 ji
ij
i i
vm
H
Vvm
Hji
ij
i i
3
1
3
1
2
2
28
3N dynamics Theoretical models
provides exact treatment for the 3N system also allows to include 3NF
Faddeev framework (based on pairwise N-N interactions)
29
3N dynamics Theoretical models
provides exact treatment for the 3N system also allows to include 3NF
Main 2NF Models -Nijmegen I & II -CD Bonn (Charge Dependant) -Argonne V18 - …
Faddeev framework (based on pairwise N-N interactions)
Calculations from: Prof. Witała and Prof. Glöckle
30
3N dynamics Theoretical models
provides exact treatment for the 3N system also allows to include 3NF
Main 2NF Models -Nijmegen I & II -CD Bonn (Charge Dependant) -Argonne V18 - …
Additional 3NF Models -Tucson Melbourne (TM99) -Urbana IX - Illinois (IL2) - …
Faddeev framework (based on pairwise N-N interactions)
+
Calculations from: Prof. Witała and Prof. Glöckle
31
3N dynamics Theoretical models
provides exact treatment for the 3N system also allows to include 3NF
Main 2NF Models -Nijmegen I & II -CD Bonn (Charge Dependant) -Argonne V18 - …
Additional 3NF Models -Tucson Melbourne (TM99) -Urbana IX - Illinois (IL2) - …
Faddeev framework (based on pairwise N-N interactions)
+
Other Approaches: Coupled Channels with Δ-isobar excitation (Prof. Deltuva, Portugal) Chiral Perturbation Theory (ChPT) only upto NNLO (Prof. Epelbaum, Germany)
Calculations from: Prof. Witała and Prof. Glöckle
K. Ermisch et al.,
PRC 68, 054004 (2003),
PRC 71, 064004 (2005)
dpdp
pd
ela
stic
sca
tter
ing
cro
ss s
ecti
on
s
32
3N dynamics Models vs. Data
pd
ela
stic
sca
tter
ing
cro
ss s
ecti
on
s
K. Ermisch et al.,
PRC 68, 054004 (2003),
PRC 71, 064004 (2005)
dpdp
33
3N dynamics Models vs. Data
K. Ermisch et al.,
PRC 68, 054004 (2003),
PRC 71, 064004 (2005)
dpdp
pd
ela
stic
sca
tter
ing
cro
ss s
ecti
on
s
34
3N dynamics Models vs. Data
K. Ermisch et al.,
PRC 68, 054004 (2003),
PRC 71, 064004 (2005)
dpdp
pd
ela
stic
sca
tter
ing
cro
ss s
ecti
on
s
35
3N dynamics Models vs. Data
K. Ermisch et al.,
PRC 68, 054004 (2003),
PRC 71, 064004 (2005)
dpdp
pd
ela
stic
sca
tter
ing
cro
ss s
ecti
on
s
36
3N dynamics Models vs. Data
K. Ermisch et al.,
PRC 68, 054004 (2003),
PRC 71, 064004 (2005)
dpdp
pd
ela
stic
sca
tter
ing
cro
ss s
ecti
on
s
37
3N dynamics Models vs. Data
39
3N dynamics
Are we done ? …No !
3NFs helped to improve theories, but still some discrepancy remains Do we understand the exact form of 3NFs !!? Include other ingredients ? Can we consider the validity through complete phase-space of 3N dynamics ? Urgent need for systematic and High-Precision data-base Next steps: dp-breakup, 4N-system detailed root-map to the 3N-system
40
3N dynamics
Are we done ? …No !
3NFs helped to improve theories, but still some discrepancy remains Do we understand the exact form of 3NFs !!? Include other ingredients ? Can we consider the validity through complete phase-space of 3N dynamics ? Urgent need for systematic and High-Precision data-base Next steps: dp-breakup, 4N-system detailed root-map to the 3N-system
Are there effects other than 3NFs ? …Yes
41
3N dynamics
Are we done ? …No !
3NFs helped to improve theories, but still some discrepancy remains Do we understand the exact form of 3NFs !!? Include other ingredients ? Can we consider the validity through complete phase-space of 3N dynamics ? Urgent need for systematic and High-Precision data-base Next steps: dp-breakup, 4N-system detailed root-map to the 3N-system
Are there effects other than 3NFs ? …Yes
Coulomb and Relativistic (but importance is limited in certain region of phase-space) Recently coulomb effect was included successfully in the calculations with coupled channel calculations ! [Prof. Deltuva, Portugal] Relativistic effects, recent work !! 4NF ? (ChPT predicts 2NF>>3NF>>4NF)
45
BINA Detector
• Big Instrument for Nuclear-polarization Analysis (a 4π detector)
BINA @AGOR 2004-2012
46
BINA Detector
• Big Instrument for Nuclear-polarization Analysis (a 4π detector)
BINA @AGOR 2004-2012
MWPC
ΔE E
47
BINA Detector
150 phoswich Scintillators =Target chamber (~10-5 mbar)
Forward scintillators (E-wall)
[9x12x220 cm3]
Thin scintillators for particle identification
(ΔE -wall) [1.8x10.8x0.1 cm3]
Wire chamber (MWPC) Three planes X, Y & U [118x118x148 wires]
Beam
Wall covers θ=10-35 ͦ
+ Ball covers
θ=up to 165 ͦ ≡
4π Phase-Space
MWPC: CF4(80%) + Isobutene(20%) gas-mixture 20µm diameter tungsten wire
Ball: Triangular fast scint. and slow phoswitch parts connected to PMT’s through lightguide
49
BINA Detector Liquid Target
Very tricky to handle it
thin transparent CH2 foil
Liquid Hydrogen (and Deuterium)
50
BINA Detector Liquid Target
Very tricky to handle it Hydrogen and Deuterium (gas-liquid phase transition @ few Kelvin) Balancing gas pressure within mechanical-stress limit of the target foil Filling in steps: insert a little gas which can be handle by the target foil and then cool it down to liquid (sudden pressure drop), repeat it …
thin transparent CH2 foil
Liquid Hydrogen (and Deuterium)
51
BINA Detector Liquid Target
Very tricky to handle it Hydrogen and Deuterium (gas-liquid phase transition @ few Kelvin) Balancing gas pressure within mechanical-stress limit of the target foil Filling in steps: insert a little gas which can be handle by the target foil and then cool it down to liquid (sudden pressure drop), repeat it … KVI Record: I’m the only - handled the target system without breaking !
thin transparent CH2 foil
Liquid Hydrogen (and Deuterium)
53
Present & Future
Data Analysis of dp and dd @ Ed=160 MeV from the last Experiment with BINA Results Planed for Poster presentation @ ENPC-2012, Bucharest 2012: Giving new life to BINA @ BCC (Bronowice Cyclotron Center), Krakow
Present
Future
54
Present & Future
Data Analysis of dp and dd @ Ed=160 MeV from the last Experiment with BINA Results Planed for Poster presentation @ ENPC-2012, Bucharest 2012: Giving new life to BINA @ BCC (Bronowice Cyclotron Center), Krakow
BINA@BCC; new experiments with proton beam up-to 250 MeV, BINA@BCC; construction of polarized targets ?? WASA@COSY ; Experiment in Jan-2013 (may be polarized beam ?) Extend the study to larger nucleon system (A>3), 4NF ? Look for exclusive channels and other observables Fine-tuning of models with inclusion of additional components in the dynamics e.g. coulomb and relativistic effects, N3LO for ChPT, different meson-exchanges…
Present
Future
55
Summary
3NF definitely improves models: we are in right direction !
Looking for effects beyond 2NF+3NF : coulomb, Relativistic, 4NF
BINA gets “residence permit ” in Poland !
Make systematic and high-precision database to validate the models
3NF Experiments at : KVI, RIKEN, RCNP, IUCF, Julich and
and now BINA@BCC in Krakow