Download presentation

Presentation is loading. Please wait.

Published byLucas MacGregor Modified over 4 years ago

1
Nuclear structure and reactions @IN2P3 Selected Higlights Shell evolution and nuclear interactions Reactions with weakly bound nuclei Nuclear Astrophysics Heavy and SHE Nuclear symetries Fundamental interactions Nuclear collisions / phase transition

2
Shell evolutions and NN interactions Disappearence of the N=28 shell closure N~16 shell gap and the location of continuum Neutron proton interactions in 92 Pd Two proton radioactivity Physics/status @ ALTO

3
5 Physical Review Letters, 1 Physical Review C 1 TOP 1%, 1 TOP 10% most quoted papers Ca S Si 42 S i -Progressive collapse of N=28 shell closure: E(2 + ) 42 Si 44 S N=28 N=20 Collapse of the N=28 shell closure Ca, Z=20 48 Ca 34 Si S, Z=16 Si, Z=14 36 S 40 Ca 46 Ar 48 Ar 44 Ar 43 S -Use of complementary experimental techniques (transfer, in-beam, isomer decay, coulex, deep inelastic) -Various structures observed (triaxial, prolate, coexistence) -Interpret this in term of nuclear forces (spin orbit, tensor) E e- (keV) 1365 keV e + e - e - conv 0 + 2 0 + 1 44 S (GANIL, IPNO, LPC Caen, IPHC Strasb)

4
UK labs + IPN Orsay, GANIL, LPC Caen from IN2P3 Evolution of shell gaps using (d,p) and (d,t) with 20 O and 26 Ne beams at SPIRAL TIARA-MUST2-EXOGAM-VAMOS COLLABORATION Position sensitive Si Barrel Hyball annular detectors 4 MUST2 SPIRAL1 beams Exogam -5 0 5 5 Th. Neutron SPE (MeV) 10 15 20 Neutron Number 14 16 d 5/2 s 1/2 d 3/2 d5d5 d3d3 O s1s1 fp states ? 8 (d,p) (d,t) 20 O Energy [MeV] 3/2 + (3/2 + ) Preliminary B. Fernandez SnSn Location of the unbound d 3/2 orbit

5
EXOGAM: 11 Clovers with partial shield. ~ 10% for E =1.3 MeV The Neutron Wall: 50 liquid scintillator detectors. 1n ~ 23% DIAMANT: 80 CsI(Tl) dets. p or ~ 66% 92 Pd spectroscopy using EXOGAM-Nwall-DIAMANT

6
92 Pd: A new spin aligned np coupling scheme B. Cederkall et al. Nature (2010) 92 Pd 92 Pd, exp. 96 Pd exp 0+0+ 0+0+ (2 + ) (4 + ) (6 + ) 2+2+ 4+4+ 6+6+ 8+8+ 0 874 1786 2536 0 1415 2099 2530 J=9 Pd 46 92 J=9 J=0 Pd 5046 96 Spin-aligned pairing Normal pairing G. De France, GANIL co-spokesperson

7
Angular and energy distributions agree with Grigorenko model 3 body decay Experiment Theory Experiment Theory angle Collaboration IN2P3: CENBG, GANIL Two proton radioactivity: 45 Fe, 54 Zn 45 Fe (2p) CENBG TPC Future plans @ GSI

8
ALTO @ Orsay Production of 5. 10 11 f/s by photofission of 238 UC x 3 dedicated lines : BEDO (beta-decay), SPECOLOR (colinear spectroscopy) and POLAREX (polarized states) Laser ion source already in operation for Ga and Cu BEDO Specolor Achievements published so far: Beta-decay spectroscopy of N~50 nuclei (D. Verney IPNO) increase of intensity coming soon

9
Reactions with weakly bound nuclei Fusion with 6,8 He Nuclear break up with 6 He

10
Neutron correlations, quantum tunneling in weakly bound nuclei 6 He n n 8 He n n 6 He+ 65 Cu reaction ->, neutrons Enhancement of pair transfer Favour a di-neutron configuration Neutron transfer dominatesFusion of 8 He comparable to 6 He ! Di-neutron config. also in Nuclear break-up of 6 He (Assié, Scarpaci IPNO, D. Lacroix GANIL) PRL 103, 232701 (2009) Lemasson, Alahari et al. Chatterjee, Navin et al. PRL 101, 032701 (2008)

11
Nuclear astrophysics Study of 13 C(,n) for AGB stars Study of 18 F destruction in novae Study of 60 Fe destruction in supernovae Incompressibility of nuclear matter with N/Z ratio

12
60 Fe cosmic ray emittor possibly detected by INTEGRAL Destroyed mainly by 60 Fe(n, ) 61 Fe reaction Studied by 60 Fe(d,p) 61 Fe at GANIL E* NpNp 61 Fe S. Giron, F. Hammache, N. de Séréville preliminary Drotleff 93 Brune 93 Orsay 3/2 + Gamow peak 1/2 + M.G. Pellegriti, F. Hammache et al. PRC 70 (2008) 042801 13 C(,n) 16 O source of neutrons for s process in AGB stars Studied at Orsay TANDEM using 13 C( 7 Li,t) 17 O Nuclear Astrophysics Collaboration IPNO/CSNSM/GANIL ½+ 18 F(p, ) 19 Ne JC Dalouzy, de Oliveira et al. PRL 102 (2009) 162503 new 18 F main source of radiation in novae Destroyed mainly by 18 F(p, ) 19 Ne reaction Studied by 19 Ne(p,p) 18 F(p) at LLN

13
Isospin dependence of the nuclear matter incompressibility Study of giant monopole mode in 56 Ni and 68 Ni 56 Ni (5.10 4 pps) @50A.MeV Interaction with d gas in MAYA C. Monrozeau, E. Khan (IPN Orsay) Phys. Rev. Lett. 100, 042501 (2008) Linked to nuclear matter incompressibility K Determine its value while increasing isospin value… L=2 L=0 E*= 13-15MeV E*= 21-23MeV d d [mb/sr] CM (deg)

14
Heavy and superheavy elements Study of Nb, Fm nuclei The cluster structure of 212 Po Probing Z=120 stability from fission times

15
256 Rf 253 No 246 Fm Spectroscopy of SHE J. Piot (CSNSM) et al 246 Fm 253 No, 256 Rf: K isomers @ Dubna, ANL 246 Fm, 254 No: Fission barrier and dynamics @ JYFL, ANL CSNSM Orsay, IPHC Strasb from IN2P3

16
Manifestation of clustering in 212 Po A. Astier et al. PRL 104 (2010)042701 Enhanced E1 transitions interpreted as oscillatory motion of the -core distance in 208 Pb 35° 148° Doppler shifted lines T E1 < 1ps stopping time Collab: CSNSM, IPNO VIVITRON + EUROGAM

17
00.20.40.60.8 (deg) Normalized Yield Fusion-Fission 0 0.2 0.4 0.6 0.8 1 1.2 0 0.2 0.4 0.6 0.8 1 1.2 0 0.2 0.4 0.6 0.8 1 1.2 U sequential fission+ …….. Quasi-elastic (target) min 0.2 t reac > 10 -18 s Blocking technique: evidence for long times at Z=120 t reac < t min (thermal vibrations) min 0.1 t min 10 -18 s INDRA, Collab: IPNO, GANIL, IPNL

18
Lifetime of SHE nucleus (Z=120) from X rays detection D. Jacquet (IPNO), M. Morjean (GANIL) et al. PRELIMINARY X rays from Z=120 seems to be observed Would be compatible with long fission times > 10 -18 s Highest Z values come from fission of compound Z=120 nucleus

19
Symmetries in nuclei Phase transition in A~100 nuclei Tetrahedral shapes

20
Mass measurements of 96,97 Kr @ ISOLDE Critical-Point Boundary for the Nuclear Quantum Phase transition near A=100 S. Naimi, G. Audi (CSNSM) et al. PRL 105 (2010) 032502 No deformation evidenced around A=100 in Kr chain !

21
Search for Tetrahedral shapes Huge gaps for tetrahedral configurations Possible signatures : hindered inter-band E2 transitions and Q 0 ~0 Experimental program JYVL, Orsay, LNL,ANL, ILL Collaboration TetraNuc IN2P3 : IPHC Strasbourg, IPN Lyon, CSNSM Orsay, IPN Orsay Hindered E2 in one band-head of 156 Gd Independent Q 0 measurement planned…

22
Fundamental interactions Superallowed Fermi interactions: 0 + 0 + β decay between isobaric analogs CVC hypothesis: Universal weak-vector coupling Need T 1/2, BR, Q Gamow Teller transitions in mirror systems 29 P, 31 S : T 1/2 - Jyväskylä – 2009 39 Ca : T 1/2 – ISOLDE - EPJ A44, 363 (2010) Perspectives : T 1/2, BR - 15 O, 21 Na, 39 Ca @ SPIRAL, 23 Mg, 31 S, 41 Sc @DESIR, Jyväskylä or ISOLDE 38 Ca : T 1/2, BR – LISE/GANIL - 2009 30 S : T 1/2 – Jyväskylä, Accepted in EPJ A 38 Ca : T 1/2 – ISOLDE - EPJ A44, 363 (2010) 42 Ti : T 1/2, BR, Q – Jyväskylä, PRC 80, 035502 (2009) 26 Si : T 1/2 – Jyväskylä, EPJ A38, 247 (2008) 62 Ga : T 1/2, BR, Q – Jyväskylä, GSI – 3 publications Perspectives : T 1/2, BR – 14 O, 18 Ne, 34 Ar @ SPIRAL 26 Si, 30 S, 38 Ca, 42 Ti @ LISE and Jyväskylä 62 Ga, 66 As, 70 Br, 74 Rb, 78 Y, 82 Nb, 86 Tc, 90 Rh, 94 As, 98 In @DESIR Collabs IN2P3: CENBG, GANIL

23
Nuclear collisions / phase transitions -Isospin dependence of symmetry energy - Production of superheavy nuclei Modeling of multinucleon transfer Shell effects in SHE by means of fission times Modelling fusion and fission Experimental study of fission of transuranium Fundamental + applied (VAMOS Gedepeon, Euratom) Phase transition in nuclear matter Bimodality of fragment distrib E. Bonnet et al. PRL 105 (2010) 142701 Collabs: GANIL, IPNO, IPNL INDRA detector G. Lehaut et al. PRL 104 (2010) 232701

24
Some Conclusions IN2P3 physicists: - Involved in different valuable items of nuclear structure and reactions -Have significant impact in the collaborations -Use various detectors and accelerators (GANIL amounts to about 50%) -Deeply involved in future projects (AGATA, S3, FAZIA, PARIS) AGATA B(E2) transitions in 74 Zn using plunger method Proposal: IRFU

25
This was not a fully inclusive presentation !

26
Below Fermi energy: stopping (isotropy) decreases Study of nuclear stopping in central collisions INDRA and ALADIN collaborations (G. Lehaut et al.), Phys. Rev. Lett. 104, 232701 (2010) Stopping systematics for central collisions of symmetric systems INDRA@GANIL,GSI Isotropy/Stopping Above Fermi energy: stopping depends on system size MEAN FIELD IN-MEDIUM NUCLEON-NUCLEON COLLISIONS

28
18 F main source of radiation in novae Destroyed mainly by 18 F(p, ) 19 Ne reaction Use 19 Ne(p,p) 18 F(p) at LLN Broad resonance in 19 Ne Proton energy distribution A broad resonance influencing the 18F destruction in novae ½+ 18 F(p, ) 19 Ne Dalouzy et al. PRL 102 (2009) 162503

29
T 1/2 = 0,09 s T 1/2 = 0,9 s 84 Ga 84 Ge 83 Ge 624,3 242,4 100 306,5 84 As 83 As 1046 247,7 N=48 0.10.20.30.40 N=50 0.10.20.30.40 N=52 0.10.20.30.40 N=54 0.10.20.30.40 D1S Gogny HFB calculation GCM Bohr dynamics 2+ (4+)

30
VAMOS 20 O(d,t) 19 O MUST2 (a) (c) 20 O(d,p) 21 O (b) E t (MeV) 1 2 3 4 5 2 4 6 8 E d (MeV) E*=1.2 MeV g.s. 40 60 80 100 120 140 160 10 20 30 40 2 3 4 5 E (MeV) 1 Angle (deg) 2.42.6 2.22.3 2.5 A/Q 20 O(d,pn) 20 O Angle (deg) Energy [MeV] 3/2 + (3/2 + ) Preliminary B. Fernandez

31
Collab: IPHC, IPNO, IPNL,

Similar presentations

OK

Trend for Precision Soil Testing % Zone or Grid Samples Tested compared to Total Samples.

Trend for Precision Soil Testing % Zone or Grid Samples Tested compared to Total Samples.

© 2018 SlidePlayer.com Inc.

All rights reserved.

To make this website work, we log user data and share it with processors. To use this website, you must agree to our Privacy Policy, including cookie policy.

Ads by Google