REQUIREMENTS for Zero-Degree Ion Selection in TRANSFER Wilton Catford University of Surrey, UK & SHARC collabs.

Slides:



Advertisements
Similar presentations
Marina Barbui Trento, Italy, April 7-11, 2014
Advertisements

GEANT4 Simulations of TIGRESS
Gammasphere-ORRUBA: Dual Detectors for Experimental Structure Studies ATLAS User Meeting, May Andrew Ratkiewicz Rutgers University.
Coupling ORRUBA and GRETINA Steven D. Pain Oak Ridge National Laboratory ORRUBA Coupling with GS Coupling with GRETINA Instrumentation GRETINA Workshop,
Γ spectroscopy of neutron-rich 95,96 Rb nuclei by the incomplete fusion reaction of 94 Kr on 7 Li Simone Bottoni University of Milan Mini Workshop 1°-
A new Si recoil tracking detector for the R 3 B experiment at GSI Nick Ashwood The University of Birmingham.
GAMMA-PARTICLE ARRAY FOR DIRECT REACTION STUDIES SIMULATIONS.
Direct Reactions at Eurisol In the light of the TIARA+MUST2 campaign at GANIL B. Fernández-Domínguez.
Direct Reactions at Eurisol In the light of the TIARA+MUST2 campaign at GANIL B. Fernández-Domínguez.
Status Report of Neutron Detector Simulation Development Brian Roeder Postdoc LPC Caen 20 Sept
Status of TACTIC: A detector for nuclear astrophysics Alison Laird University of York.
GAMMA-PARTICLE ARRAY FOR DIRECT REACTION STUDIES SIMULATIONS.
1107 Series of related experiments; first for transfer with TIGRESS Nuclear structure motivation for 25,27 Na beams Nuclear astrophysics motivation for.
Reaction rates in the Laboratory Example I: 14 N(p,  ) 15 O stable target  can be measured directly: slowest reaction in the CNO cycle  Controls duration.
Reaction rates in the Laboratory Example I: 14 N(p,  ) 15 O stable target  can be measured directly: slowest reaction in the CNO cycle  Controls duration.
SATURN HST/ IR 1998, TETHYS VOYAGER2 1981, URANUS HST/ IR 1986 What can we learn from transfer, and how is best to do it? Wilton Catford University of.
ANASEN - Array for Nuclear Astrophysics Studies with Exotic Nuclei Silicon-strip detector array backed with 2-cm-thick CsI Gas proportional counter for.
Spectrometer Workshop 10/3 – 11/3 Lund University.
Possibility of bringing TRI  P to HIE-ISOLDE Dual magnetic Spectrometer Olof TENGBLAD ISCC Oct. 22nd 2013 There will be a presentation during the ISOLDE.
Nov.29,2011/HU group meeting Spectroscopic Investigation of P-shell Λ hypernuclei by (e,e'K + ) - Analysis Updated Status - Chunhua Chen Hampton Universithy.
T.C. Jude D.I. Glazier, D.P. Watts The University of Edinburgh Strangeness Photoproduction: Polarisation Transfer & Cross-Section Measurements.
Polarisation transfer in hyperon photoproduction near threshold Tom Jude D I Glazier, D P Watts The University of Edinburgh.
Medium heavy Λ hyper nuclear spectroscopic experiment by the (e,e’K + ) reaction Graduate school of science, Tohoku University Toshiyuki Gogami for HES-HKS.
The Inverse Kinematics Resonance Elastic Scattering Reaction of 10,11,12 Be+p Liu Yingdu( 刘应都 ) PHD candidate Advisor : Wang Hongwei, Ma Yugang
Direct Reactions with ORRUBA and GRETINA Steven D. Pain Oak Ridge National Laboratory GRETINA Workshop, ANL, February 2013.
Study of the Halo Nucleus 6 He using the 6 Li(   ) 6 He Reaction Derek Branford - Edinburgh University for the A2-Collaboration MAMI-B Mainz.
Study of the 40 Ca(  ) 44 Ti reaction at stellar temperatures with DRAGON Christof Vockenhuber for the DRAGON collaboration Vancouver, B.C., Canada.
From CATE to LYCCA Mike Taylor Particle Identification After the Secondary Target.
Single-neutron structure of neutron-rich nuclei near 132 Sn Jolie A. Cizewski Department of Physics & Astronomy Rutgers University.
Setup for hypernuclear gamma-ray spectroscopy at J-PARC K.Shirotori Tohoku Univ. Japan for the Hyperball-J collaboration J-PARC E13 hypernuclear  -ray.
The neutron magic numbers N=16, 20 & 28 for neutron rich exotic nuclei, as probed by nucleon transfer with radioactive beams Wilton Catford University.
Sep. 2003CNS Summer School Feb 分 => Talk なら 35 枚だが、 lecture だと少なめ? 50 分 => Talk なら 35 枚だが、 lecture だと少なめ?
Yury Gurchin June 2011 MEASUREMENT OF THE CROSS-SECTION IN DP-ELASTIC SCATTERING AT THE ENERGIES OF 500 AND 880 MEV AT NUCLOTRON.
UNIVERSITY OF JYVÄSKYLÄ RDDS measurements at RITU and prospects at HIE-ISOLDE T. Grahn University of Jyväskylä HIE-ISOLDE Spectrometer Workshop, Lund
A new position sensitive strip array Wilton Catford (Surrey, UK) with LPC Caen, Birmingham, Paisley T R A ransfer eaction rray.
RNB Cortina d’Ampezzo, July 3th – 7th 2006 Elisa Rapisarda Università degli studi di Catania E.Rapisarda for the Diproton collaboration 18 *
PRESORT OF THE DATA OF THE COLOGNE TEST EXPERIMENT ● Quality and integrity of data ● Detector numbering and positions ● Calibrations and gain stability.
I. MARTEL SGFDC UNIVERSITY OF HUELVA JULY 2007 Collaboration: University of Huelva, Spain (coordinator) GSI-Darmstadt, Germany. University of.
Experimental Nuclear Physics Some Recent Activities 1.Development of a detector for low-energy neutrons a. Hardware -- A Novel Design Idea b. Measure the.
Study of unbound 19 Ne states via the proton transfer reaction 2 H( 18 F,  + 15 O)n HRIBF Workshop – Nuclear Measurements for Astrophysics C.R. Brune,
Β decay of 69 Kr and 73 Sr and the rp process Bertram Blank CEN Bordeaux-Gradignan.
NS08 MSU, June 3rd – 6th 2008 Elisa Rapisarda Università degli studi di Catania E.Rapisarda 18 2.
Nuclear Astrophysics ARUNA Workshop, Notre Dame, IN Carl R. Brune Ohio University, Athens Ohio June 12-13, 2014.
J-PARC でのハイパー核ガンマ線分光実験用 散乱粒子磁気スペクトロメータ検出器の準備 状況 東北大理, 岐阜大教 A, KEK B 白鳥昂太郎, 田村裕和, 鵜養美冬 A, 石元茂 B, 大谷友和, 小池武志, 佐藤美沙子, 千賀信幸, 細見健二, 馬越, 三輪浩司, 山本剛史, 他 Hyperball-J.
SATURN HST/ IR 1998, TETHYS VOYAGER2 1981, URANUS HST/ IR 1986 What can we learn from transfer, and how is best to do it? Wilton Catford University of.
Possibility of bringing TRI  P to HIE-ISOLDE a Dual magnetic Spectrometer reconsidered Olof TENGBLAD ISCC 16th February 2015 (Previous: ISCC 22nd Oct.
Combining TIGRESS with charged- particle detection at ISAC-II Fred Sarazin Matt Porter-Peden Luke Erikson Colorado School of Mines.
VAMOS « Hot » results and perspectives * Spectroscopy of n-rich nuclei produced by fission * New gas-filled spectrometer-separator for fusion Getting ready.
The experimental evidence of t+t configuration for 6 He School of Physics, Peking University G.L.Zhang Y.L.Ye.
Summary of LOIs to INTC (24 June 2010). Call for Letters of Intent (deadline May 21) 34 Letters submitted 284 Participants from 76 Laboratories in 22.
100MeV/u 12 C+ 12 C Scattering at RCNP Weiwei Qu 、 Gaolong Zhang 、 Satoru Terashima 、 Isao Tanihata 、 Chenlei Guo 、 Xiaoyun Le 、 Hoo Jin Ong 、 Harutaka.
Study of repulsive nature of optical potential for high energy 12 C+ 12 C elastic scattering (Effect of the tensor and three-body interactions) Gaolong.
Technical solutions for N=Z Physics David Jenkins.
Exploring the alpha cluster structure of nuclei using the thick target inverse kinematics technique for multiple alpha decays. Marina Barbui June, 23 rd,
Jun Chen Department of Physics and Astronomy, McMaster University, Canada For the McMaster-NSCL and McMaster-CNS collaborations (5.945, 3+ : **) (5.914,
PJ Woods University of Edinburgh In-ring detector systems.
26th September 2014 Guillermo Ribeiro 1 G. Ribeiro, E. Nácher, A. Perea, J. Sánchez del Río, O. Tengblad Instituto de Estructura de la Materia – CSIC,
Fusion excitation measurement for 20 O + 12 C at E/A = 1-2 MeV Indiana University M.J. Rudolph, Z.Q. Gosser, K. Brown ✼, D. Mercier, S. Hudan, R.T. de.
Exploring the alpha cluster structure of nuclei using the thick target inverse kinematics technique for multiple alpha decays. The 24 Mg case Marina Barbui.
Focal plane detector discussion Kwangbok Lee Low Energy Nuclear Science team Rare Isotope Science Project Institute for Basic Science July 11,

Young Researchers Session in IFIN-HH 2016
What can we learn from transfer, and how is best to do it?
Vamos + Exogam Spectrometer
1. Introduction Secondary Heavy charged particle (fragment) production
Variable Mode High Acceptance Spectrometer
Recent Highlights and Future Plans at VAMOS
Status and perspectives of the LNS-FRIBS facility
What can we learn from transfer, and how is best to do it?
Presentation transcript:

REQUIREMENTS for Zero-Degree Ion Selection in TRANSFER Wilton Catford University of Surrey, UK & SHARC collabs

INCIDENT BEAM (d,t) forward of 45° (d,d) just forward of 90° (d,p) from 180° to forward of 80° The energies are also weakly dependent on mass of the beam so a general purpose array can be utilised USING RADIOACTIVE BEAMS in INVERSE KINEMATICS

INCIDENT BEAM (d,t) forward of 45° (d,d) just forward of 90° (d,p) from 180° to forward of 80° transfer products on neutron-rich side can sequentially n-decay (filling a bigger cone) (with smaller momentum) USING RADIOACTIVE BEAMS in INVERSE KINEMATICS isobaric beams can be identified and/or physically separated (possibly further stripped, e.g. 15 N 3+ / 21 O 4+ ) Knock-on carbons from CD 2 targets fusion-evaporation products from reactions on C in CD 2 targets + other things, anyone….?

What would an ideal zero-degree device achieve? identification of reaction products physical separation of reaction products of interest, from the beam physical separation of reaction products of interest, from fusion-evap physical separation of isobaric beams or other beam contaminants large enough angular acceptance to pick up sequential decay products excellent angular resolution to allow kinematic reconstruction – missing-p to avoid compromising the placement of gamma-ray detectors to be consistent with good coverage by other detectors around target to have sufficient flight path to allow for the use of TOF methods to be as transportable as the rest of the set-up, to optimise exploitation What are we prepared to lose? What is the compromise? accept limited mass identification of reaction products? forego physical separation? tolerate limited angular acceptance? angular resolution? relax the requirement of portability? Wilton Catford, University of Surrey, UK – HIE-Isolde Spectrometer Workshop, Lund, March 2011

24 Ne(d,p  ) N=16 replaces broken N=20 W.N. Catford et al., Eur. Phys. J. A25, Suppl. 1, 245 (2005). Schematic of the TIARA setup. A beam of 10 5 pps of 24 Ne at 10.5A MeV was provided from SPIRAL, limited to 8  mm.mrad to give a beam spot size of mm. The target was 1.0 mg/cm 2 of (CD 2 ) n plastic. The TIARA array covered 90% of 4  with active silicon. OUR EXPERIMENT TO STUDY 25 Ne d 3/2

TIARA Recent experiments at SPIRAL merge the TIARA array with the French MUST2 telescopes at at the forward angles. The TIARA barrel has a second layer of Si added, to help with punchthrough.

Vamos+Exogam GATE ON GAMMA COINCIDENCE REMOVES GROUND STATE Geant4 Simulation Requiring Vamos FP Plastic 24 Ne (d,p) 25 Ne ~ 10 A.MeV

24 Ne (d,p) 25 Ne Requiring Vamos (Focal Plane Plastic) Without Vamos Requirement BEAM (d,t) tritons Knock-on carbon elastics (saturation) (90 degrees) ~ 10 A.MeV

24 Ne (d,p) 25 Ne 26 Ne (d,p) 27 Ne ~ 10 A.MeV

20 O(d,p) 21 O 26 Ne(d,p) 27 Ne 2500 pps S M Brown et al 10,000 pps B Fernandez et al 21 O 20 O E x (keV ) J  C 2 S(0 + ) 0 3/  /2  0.64  /  /2  0.44  0.22 Gamma ( 20 O) Gamma ( 27 Ne) Bound States Bound State Particle ID 0° Unbound States n + 20 O decay Unbound States

Ch. DIGET, YORK / GEMMA WILSON & WNC, SURREY Prototype of new type of experiment for us – where the states are so close together in this odd-odd nucleus that we will need to GATE on gamma transitions in order to separate the different final states SHARC Aug 2009 At ISAC2 we have used the isotone of 24 Ne namely 25 Na as the projectile. The new array is SHARC (Ch. Aa. Diget et al., York UK, Surrey, LPC Caen, TRIUMF, TIGRESS, CSM, LSU, …) … which is compact and fits inside TIGRESS We used up to 3 x 10 7 pps 25 Na at 5.00 MeV/u. Nucleon transfer by (d,p) at 5 MeV/u at ISAC2 WILTON CATFORD, SURREY

SHARC

Schematic TIGRESS resolution and decay scheme Trifoil Tags recoil events All beam goes through 30µm Al foil Catches fusion evaporation products from carbon Downstream box Elastically scattered p and d Upstream box ejected protons CD detector ejected protons

25 Na(d,p) 26 Na at 5.00 MeV/A: proton-neutron coupling TIGRESS resolution and decay scheme Trifoil Tags recoil events All beam goes through 30µm Al foil Catches fusion evaporation products from carbon Downstream box Elastically scattered p and d Upstream box ejected protons CD detector ejected protons

SHARC chamber (compact Si box) TIGRESS zero degrees Bank of 500 preamplifiers cabled to TIG10 digitizers BEAM WILTON CATFORD, SURREY

Preliminary Analysis: E vs θ Energy v Theta with trifoil 26 Na g.s. 26 Na ex. states (d,d) (p,p)

26 Ne(d,p) 27 Ne 26 Ne(d,p) 27 Ne  26 Ne+n ZERO DEGREE = SPECTROMETER ZERO DEGREE = SCINTILLATOR RESULTS from TIARA/MUST2 Nov2007RESULTS from SHARC Aug2009

26 Ne(d,p) 27 Ne 10 A.MeV ZERO DEGREE = SPECTROMETER ZERO DEGREE = SCINTILLATOR RESULTS from TIARA/MUST2 Nov2007RESULTS from SHARC Aug Na(d,p) 26 Na 5 A.MeV

(d,d) (p,p) (d,p) MISSING MOMENTUM using 26 Ne beam to study (d,p) with VAMOS 26 Ne ions in VAMOS 27 Ne ions in VAMOS EXCLUDE

What would an ideal zero-degree device achieve? identification of reaction products physical separation of reaction products of interest, from the beam physical separation of reaction products of interest, from fusion-evap physical separation of isobaric beams or other beam contaminants large enough angular acceptance to pick up sequential decay products excellent angular resolution to allow kinematic reconstruction – missing-p to avoid compromising the placement of gamma-ray detectors to be consistent with good coverage by other detectors around target to have sufficient flight path to allow for the use of TOF methods to be as transportable as the rest of the set-up, to optimise exploitation What are we prepared to lose? What is the compromise? accept limited mass identification of reaction products? forego physical separation? tolerate limited angular acceptance? angular resolution? relax the requirement of portability? Wilton Catford, University of Surrey, UK – HIE-Isolde Spectrometer Workshop, Lund, March 2011