-JINA - A. Aprahamian, University of Notre Dame. University of Notre Dame Michigan State University University of Chicago Argonne National Laboratory
|
|
- Percival Burns
- 5 years ago
- Views:
Transcription
1 -JINA - Joint Institute for Nuclear Astrophysics NSF-Physics Frontier Center A. Aprahamian, University of Notre Dame University of Notre Dame Michigan State University University of Chicago Argonne National Laboratory Status of JINA Physics Achievements Outreach Achievements
2 Status of Funding COOPERATIVE AGREEMENT NO. PHY Between NATIONAL SCIENCE FOUNDATION Arlington, VA and University of Notre Dame Notre Dame, IN TITLE: Joint Institute for Nuclear Astrophysics JINA PI Name: Michael Wiescher, Timothy C. Beers, Hendrik Schatz, James W. Truran EFFECTIVE DATE: August 1, 2003 EXPIRATION DATE: July 31, 2008 AUTHORITY: This Agreement is awarded pursuant to the authority of the National Science Foundation Act of 1950
3 Administrative Personnel Administrator: Outreach Coordinator: Webmaster: Kathy Burgess, Notre Dame Chasidy Box, Michigan State Suzanne Coshow, Notre Dame Ping Zheng, Notre Dame
4 Scientific Personnel 2 post-docs appointed! Sanjib Gupta - Michigan State August 2003 Global description for electron capture rates, Network simulations of nuclear processes in neutron star crust Leandro Gasques - Notre Dame October Nuclear Potential models for heavy ion reactions, Global description for pycno nuclear reaction rates
5 JINA visitors in 2003 R.E. Azuma, University Toronto, Canada August 2003 r-matrix modeling J. Fisker, Universität Basel, Switzerland September 2003 X-ray burst modeling and rp-process nucleosynthesis U. Geppert, Inst. Astrophysics Potsdam, Germany March 2003 Neutron star crust behavior, pycno nuclear processes K.L. Kratz, Universität Mainz, Germany October 2003 r-process modeling, r-process data compilation E. Somorjai, ATOMKI, Debrecen, Hungary September 2003 p-process measurements
6 JINA Students 2003 Christian Gils; Universität Konstanz, Germany Ion source ND August-September 2003 Sasha Falahat, Universität Mainz, Germany r-process ND September-December 2003 Iris Dillmann, Universität Mainz, Germany r-process ND and NSCL/MSU October-November 2003
7 Subcontract Agreements being negotiated with: SciDAC Center, UC Santa Cruz SciDAC Center, University of Arizona Institute for Theoretical Physics, UC Santa Cruz for awarding JINA fellow positions on the postdoctoral and grad student level
8 JINA - Virtual Journal for Nuclear Astrophysics Weekly web-based compilation of all nuclear astrophysics related publications from 30 scientific journals (since mid-july 2003) Editors: Sam Austin Tim Beers Hendrik Schatz
9 Data-Compilation Goal Development of web-base nuclear astrophysics data journal Editorial board review of published reaction rates & decay rates translating nuclear data into reaction rates applying a standardized format (reaclib) regular web-based up-date of reaction rate library web-based compilation of other available libraries C. Iliadis F. Käppeler H. Schatz M. Smith M. Wiescher
10 Science & Education Resources Literature Servers Nuclear Data Nuclear Astrophysics Data Information about Nuclear Astrophysics RIA Other Radioactive Beam Facilities Underground Labs University Nuclear Astrophysics Labs Astrophysics With Neutron Beam Facilities Theory Institutions Observatories History of Nuclear Astrophysicsl Educational Applets X-Ray Burst Simulations Nucleosynthesis Movies
11 JINA conferences & workshops The Nuclear Physics Of Core Collapse Supernovae May 26 - June 8, 2003; Institute of Physics, Aspen, Colorado (organizers: JINA - SciDAC U.Arizona) Underground Accelerator for Nuclear Astrophysics Oct , 2003; Marriott University Park Hotel, Tucson, AZ (Organizers: JINA INT LBNL) First Argonne/MSU/INT RIA Workshop January 8-10, 2004 ; INT, Seattle, Washington (organizers: INT-ANL-MSU-JINA)
12 The Nuclear Physics Of Core Collapse Supernovae May 26 - June 8, 2003; Institute of Physics, Aspen, Colorado 30 participants from 9 countries New Experience; Black Board Teaching
13 Topical highlights of the workshop Core Collapse Physics Organizer: Adam Burrows Reaction Rates in Nuclear Astrophysics Organizer: Michael Wiescher The r-process Organizer: Hendrik Schatz The Equation of State Organizers: Sanjav Reddy JINA Opportunities Organizer: Michael Wiescher Type I Supernovae Models Organizer: Stan Woosley Explosive Nucleosynthesis Scenarios Organizer: Jim Truran Gamma Ray Bursts Organizer: Andrew MacFadyen Type I X-Ray Bursts Organizer: Stan Woosley
14 JINA research focus, MRC MRC1: the origin of elements stellar evolution & type-ii SN nucleosynthesis low energy nuclear reactions r-process nucleosynthesis p-process nucleosynthesis MRC2: fate of matter on accreting neutron stars rp-process electron capture processes pycno-nuclear reactions
15 Equipment Development NERO neutron detector at NSCL/MSU NSCL & Institute für Kernchemie, Mainz ECR source for Notre Dame KN system ND & TU Wien, U. Giessen, ANL development JINA recoil mass separator at Notre Dame ND & NSCL/MSU, ANL development
16 NSCL Developed at NSCL with Kernchemie, Mainz Tested and calibrated at Notre Dame using a series of (α,n) reactions Used at NSCL for study of 78 Ni decay for r-process Proposed at Notre Dame for 25,26 Mg(α,n) studies as stellar neutron sources
17 Recoil FN tandem accelerator Design plan for compact recoil separator system: G.P. Berg, KVI Groningen Recoil Separator KN accelerator based on: DRAGON, TRIUMF ERNA, U. Bochum ARIES, Louvain la Neuve
18 JINA - Science Activities in Se mass measurements at ATLAS/ANL rp-process in type I XRBs; ND-ANL collaboration 78 Ni β-decay & lifetime measurement at NSCL/MSU r-process in type II SN ; MSU-ND-Mainz collaboration 112 Cd(α,γ) measurement at NSL/ND p-process in type II SN; ND-ATOMKI collaboration Type I XRB multi-zone nucleosynthesis simulation UC-Santa Cruz-MSU-ND collaboration e-capture and pycnonuclear reaction rates NSCL/MSU ND collaboration
19 Mass measurement of 68 Se as rp-process waiting point Experiment performed at focal plane of FMA through β-endpoint measurement of 68 Se decay. γ-decay of accumulated 68Se
20 Decay & endpoint measurement of 68 Se Decay curve for 68 Se Q-value of 68 Se(p,γ) 69 Br
21 Half life of 78 Ni on the r-process path β-decay half-lives Branchings for β-delayed n-emission Neutron detector NERO 3 He + n -> t + p neutron Fast Fragment Beam (fragment. 140 MeV/u 86 Kr) Si Stack Particle type (TOF, de, p) Implantation time and location β-emission time and location neutron-β coincidences
22 Preliminary results on 78 Ni E (arb units) Ni implant events 73 Co 76 Ni 73 Co Neutron gated TOF (arb units)
23 Multi-Zone X-Ray Bursts Light-curve Convection Nucleosynthesis luminosity Depth profile for Luminosity Convection υ-production Submitted; Woosley et al. Astrophys.J. 2003
24 Energy & Nucleosynthesis in Multi-Mass-Zone XRBs Prior 1 st burst After 1 st burst
25 pycnonuclear reaction rates in neutron star crust Potential models for heavy ion fusion cross sections Test with nuclei near stability Extrapolation towards drip-line Future experimental program anticipated
26 JINA Outreach at High Schools and Colleges Distribution of Flyers Discussion with teachers Introduction of teacher led student programs
27 Recruitment of Teachers Outreach to McNair Minority Program At Notre Dame
28 Membership and Committees Executive Committee: S. Austin (MSU); L. Bildsten (UC Santa Barbara) E. Rehm (ANL); H. Schatz (MSU) J.W. Truran (U. Chicago) Participating Research Institutions: University of Notre Dame Michigan State University University of Chicago Argonne National Laboratory SSC SciDaC Center, UCSC, U.Arizona ITP-UC Santa Barbara Participating Colleges: Hope College, MI Indiana University South Bend, IN Southern Indiana University, IN Clark Atlanta University, GA Xavier University, LS St. Edwards University, TX St. Mary s University, TX Intl. Advisory Committee: S. Austin (MSU) K. Langanke (Århus) V.J. Pandharipande (U.Illinois) P. Parker (Yale) C. Sneden (U. Texas) S.E. Woosley (UC Santa Cruz) Outreach Advisory Committee: P. DeYoung (Hope) K. Johnston (Elkhart Highschool) D. Pope Davis (CANDAX-McNair, ND) S. Shore (IUSB) M. Thoennessen (MSU)
29 Conclusions JINA is (nearly) fully established Activities in research & outreach Collaborations have been formed Conferences have been organized All you want to know about JINA:
JINA collaborations & conferences
JINA collaborations & conferences Goal of JINA is to initiate a broad spectrum of collaboration to maximize expertise and input to address specific research goals addressed by MRC1 and MRC2! Goal of JINA
More informationFrom the Midwest to the World the Joint Institute for Nuclear Astrophysics Hendrik Schatz Michigan State University
From the Midwest to the World the Joint Institute for Nuclear Astrophysics Hendrik Schatz Michigan State University 15 Years of Nuclear Astrophysics with JINA It started all at Notre Dame National and
More informationThe origin of heavy elements in the solar system
The origin of heavy elements in the solar system (Pagel, Fig 6.8) each process contribution is a mix of many events! 1 Heavy elements in Metal Poor Halo Stars recall: [X/Y]=log(X/Y)-log(X/Y) solar CS22892-052
More informationMRC-1: Low Energy Nuclear Reactions and Stellar Evolution
MRC-1: Low Energy Nuclear Reactions and Stellar Evolution Michael Wiescher Focus-1: Stellar Hydrogen burning in massive stars Re-evaluation of CNO cycles Focus-2: Stellar He-burning neutron sources for
More informationExperimental Nuclear Astrophysics: Lecture 3. Chris Wrede National Nuclear Physics Summer School June 20 th, 2018
: Lecture 3 Chris Wrede National Nuclear Physics Summer School June 20 th, 2018 Outline Lecture 1: Introduction & charged-particle reactions Lecture 2: Neutron-induced reactions Lecture 3: What I do (indirect
More informationJINA. Address open questions by working on the nuclear physics and the astrophysics
JINA goals Astrophysics Nuclear Physics JINA Address open questions by working on the nuclear physics and the astrophysics JINA workshop goals Interesting problems Ready to be addressed Unknowns ready
More informationRich Opportunities for Astrophysics
Rich Opportunities for Astrophysics A flood of new observations and more to come with INTEGRAL, JWST, Constellation-X, Growing computational capability Problems ripe for solution: How supernovae explode,
More informationHydrogen and Helium Burning in Type I X-ray Bursts: Experimental Results and Future Prospects. Catherine M. Deibel Louisiana State University
Hydrogen and Helium Burning in Type I X-ray Bursts: Experimental Results and Future Prospects Catherine M. Deibel Louisiana State University 8/29/14 CGS15 August 25 29, 2014 1 Click Type to I X-Ray edit
More informationNew experiments on neutron rich r-process Ge Br isotopes at the NSCL
New experiments on neutron rich r-process Ge Br isotopes at the NSCL M. Quinn* 1,2, A. Aprahamian 1,2, S. Almaraz 1,2, B.B. Skorodumov 1,2, A. Woehr 1,2 1) Institute for Structure and Nuclear Astrophysics
More informationPerspectives on Nuclear Astrophysics
Perspectives on Nuclear Astrophysics and the role of DUSEL Nuclear Astrophysics is a broad field that needs facilities from 1keV-100GeV A low energy accelerator DIANA a DUSEL is a unique instrument for
More informationb delayed g decay measurements to probe thermonuclear astrophysical explosions
b delayed g decay measurements to probe thermonuclear astrophysical explosions Chris Wrede Michigan State University and NSCL for the NSCL E10034, E12028 & E14066 collaborations NIC XIII, Debrecen, Hungary
More information70 years of Nuclear Physics at ND ( : seventy years of Nuclear Physics at Notre Dame)
70 years of Nuclear Physics at ND (1937 2007: seventy years of Nuclear Physics at Notre Dame) Nuclear Physics was born at the University of Notre Dame in 1937 with the first successful experiments accelerating
More informationNational Superconducting Cyclotron Laboratory
National Superconducting Cyclotron Laboratory Forefront national user facility for rare isotope research and education in nuclear science, astro-nuclear physics, accelerator physics, and societal applications
More informationCarbon Burning in the Universe and the Laboratory
Carbon Burning in the Universe and the Laboratory X. Tang University of Notre Dame Carbon burning processes in the Universe Carbon burning in the laboratory Limits on the molecular resonance strengths
More informationA New Measurement of the E1 Component of
A New Measurement of the E1 Component of the 12 C(α,γ) 16 O Reaction X. Tang Physics Division Argonne National Laboratory Outline Why is the 12 C(α, γ) 16 O reaction important? The 12 C(α,γ) 16 O reaction
More informationX-RAY BURSTS AND PROTON CAPTURES CLOSE TO THE DRIPLINE. The hydrogen-rich accreted envelopes of neutron stars in binary systems are
1 X-RAY BURSTS AND ROTON CATURES CLOSE TO THE DRILINE T. Rauscher 1, F. Rembges 1, H. Schatz 2, M. Wiescher 3, F.-K. Thielemann 1 The hydrogen-rich accreted envelopes of neutron stars in binary systems
More informationView From the West Coast
View From the West Coast Lars Bildsten Kavli Institute for Theoretical Physics Department of Physics University of California, Santa Barbara QuickTime and a TIFF (Uncompressed) decompressor are needed
More informationScientific goal in Nuclear Astrophysics is to explore:
Nuclear Physics in Stars Michael Wiescher University of Notre Dame Joint Institute for Nuclear Astrophysics Scientific goal in Nuclear Astrophysics is to explore: Nuclear Signature in the Cosmos The Nuclear
More informationExperimental Nuclear Astrophysics: Lecture 1. Chris Wrede National Nuclear Physics Summer School June 19 th, 2018
: Lecture 1 Chris Wrede National Nuclear Physics Summer School June 19 th, 2018 Outline Lecture 1: Introduction & charged-particle reactions Lecture 2: Neutron-capture reactions Lecture 3: What I do (indirect
More informationEVOLUTION OF SHELL STRUCTURE
EVOLUTION OF SHELL STRUCTURE W A RICHTER ITHEMBA LABS UNIVERSITY OF THE WESTERN CAPE Focus points: 1. Single-particle structure of nuclei 2. Elastic scattering 3. The Interface between Nuclear structure
More informationBeauty in PhysicsTheory and Experiment
Beauty in PhysicsTheory and Experiment Hacienda Cocoyoc, Morelos, May 14-18, 2012 My personal Journey Beauty in PhysicsTheory and Experiment Beauty in PhysicsTheory and Experiment Hacienda Cocoyoc, Morelos,
More informationCapabilities at the National Superconducting Cyclotron Laboratory. Sean Liddick NDNCA workshop, May 26-29, 2015
Capabilities at the National Superconducting Cyclotron Laboratory Sean Liddick NDNCA workshop, May 26-29, 2015 NSCL and FRIB Laboratory NSCL is funded by the U.S. National Science Foundation to operate
More informationarxiv:nucl-th/ v1 14 Nov 2005
Nuclear isomers: structures and applications Yang Sun, Michael Wiescher, Ani Aprahamian and Jacob Fisker Department of Physics and Joint Institute for Nuclear Astrophysics, University of Notre Dame, Notre
More informationMRC 3 spokesperson: H. Schatz
MRC 3 spokesperson: H. Schatz KS 1731-260 with Chandra X-ray binaries Equation of State Nova Cygni 1992 with HST Novae X-ray bursts cooling Lines during bursts M,R 15 s (1735-444) EXO0748-676 Cottam, Paerels,
More informationarxiv: v1 [nucl-ex] 1 Jul 2007
TOF-Bρ Mass Measurements of Very Exotic Nuclides for Astrophysical Calculations at the NSCL arxiv:0707.0119v1 [nucl-ex] 1 Jul 2007 M Matoš 1,2, A Estrade 1,2,3, M Amthor 1,2,3, A Aprahamian 2,4, D Bazin
More informationDirect (α,p) Reaction Measurements with HELIOS and the study of 20 Ne(α,p) 23 Na
Direct (α,p) Reaction Measurements with HELIOS and the study of 20 Ne(α,p) 23 Na Jianping Lai, Daniel Santiago-Gonzalez Catherine M. Deibel Louisiana State University 9/13/16 INPC 2016 1 (α,p) Reactions
More informationAn Introduction to. Ion-Optics. Series of Five Lectures JINA, University of Notre Dame Sept. 30 Dec. 9, Georg P. Berg
An Introduction to Ion-Optics Series of Five Lectures JINA, University of Notre Dame Sept. 30 Dec. 9, 2005 Georg P. Berg 1 The Lecture Series 1 st Lecture: 9/30/05, 2:00 pm: Definitions, Formalism, Examples
More informationRecent neutron capture measurements at FZK
René Reifarth Recent neutron capture measurements at FZK Outline: Overview of s-process nucleosynthesis Nuclear data needs for the s-process where do we stand? Recent (n,γ) cross section measurements at
More informationSe rp-process waiting point and the 69
68 Se rp-process waiting point and the Kr -delayed proton emission experiment Marcelo Del Santo Joint Institute for Nuclear Astrophysics National Superconducting Cyclotron Laboratory Frontiers 2010 Workshop
More informationConstraining Astrophysical Reaction Rates with Transfer Reactions at Low and Intermediate Energies
Constraining Astrophysical Reaction Rates with Transfer Reactions at Low and Intermediate Energies Christoph Langer (JINA/NSCL) INT Workshop: Reactions and Structure of Exotic Nuclei March 2015 1 Understanding
More informationCharge Exchange and Weak Strength for Astrophysics
Charge Exchange and Weak Strength for Astrophysics Sam Austin STANfest-July 16 2004 Charge Exchange and Weak Strength for Astrophysics Interesting phenomena Electron capture strength (GT) (Langanke talk)
More informationMotivation. 1 GSI, Darmstadt, Germany. 2 The University of Edinburgh, UK. 3 Technische Universität München, Germany
β-decay of very neutron-rich Rh, Pd, Ag nuclei including the r-process waiting point 128 Pd F. Montes 1, T. Davinson 2, T. Faestermann 3, H. Geissel 1, R. Gernhäuser 3, M. Gorska 1, K.-L. Kratz 4, Y. Litvinov
More informationOpportunities to study the SHE production mechanism with rare isotopes at the ReA3 facility
Opportunities to study the SHE production mechanism with rare isotopes at the ReA3 facility Zach Kohley National Superconducting Cyclotron Laboratory Department of Chemistry Michigan State University,
More informationNuclear Astrophysics with DRAGON at ISAC:
Nuclear Astrophysics with DRAGON at ISAC: The 21 Na(p, γ) 22 Mg reaction John M. D Auria for the DRAGON Collaboration Simon Fraser University Burnaby, British Columbia, Canada Abstract The DRAGON facility
More informationNew Reaction Rates of 64 Ge(p,γ) 65 As and 65 As(p,γ) 66 Se and the Impact on Nucleosynthesis in Type-I X-ray Bursts
New Reaction Rates of 64 Ge(p,γ) 65 As and 65 As(p,γ) 66 Se and the Impact on Nucleosynthesis in Type-I X-ray Bursts Yi Hua LAM ( 藍乙華 ) Collaborators: Jian Jun HE ( 何建軍 ), Anuj PARIKH, Hendrik SCHATZ,
More information70 years of Nuclear Physics at Notre Dame
70 years of Nuclear Physics at Notre Dame 1937-2007 Michael Wiescher A history of 5 accelerator generations ~10 student generations ~ 4 faculty generations in Nuclear structure, Nuclear reaction, Nuclear
More informationStellar Evolution: what do we know?
Stellar Evolution: what do we know? New Tools - Astronomy satellite based observatories Hubble Space Telescope Compton Gamma-Ray Observatory Chandra X-Ray Observatory INTEGRAL ground based observatories
More informationBetty Tsang, NSCL/MSU 曾敏兒. collaboration
Science of the SpRIT Time Projection Chamber From Earth to Heavens: Femto-scale nuclei to Astrophysical objects SAMURAI International Collaboration Meeting, Sept 8-9, 2014 Sendai, Japan 曾敏兒 for Betty Tsang,
More informationExplosive Events in the Universe and H-Burning
Explosive Events in the Universe and H-Burning Jordi José Dept. Física i Enginyeria Nuclear, Univ. Politècnica de Catalunya (UPC), & Institut d Estudis Espacials de Catalunya (IEEC), Barcelona Nuclear
More informationNSCL and Physics and Astronomy Department, Michigan State University Joint Institute for Nuclear Astrophysics
National Superconducting Cyclotron Laboratory An overview Ana D. Becerril NSCL and Physics and Astronomy Department, Michigan State University Joint Institute for Nuclear Astrophysics University of North
More informationDepartment of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
Spin assignments of 22 Mg states through a 24 Mg(p,t) 22 Mg measurement, K. L. Jones, B. H. Moazen, S. T. Pittman Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996,
More informationExperimental Study of Stellar Reactions at CNS
Experimental Study of Stellar Reactions at CNS Shigeru KUBONO ( 久保野茂 ) Center for Nuclear Study (CNS) University of Tokyo 1. Nucleosynthesis under Explosive Conditions + CNS-RIKEN AVF-Upgrade Project 2.
More informationExperiments on reaction rates for the astrophysical p-process
Experiments on reaction rates for the astrophysical p-process Zs. Fülöp ATOMKI Debrecen, Hungary Science case Experimental needs Used technique Trends in available data Plans for the future Heavy element
More informationFigure 2.11 from page 152 of Exploring the Heart of Ma2er
Nuclear Astrophysics The aim of nuclear astrophysics is to understand those nuclear reacbons that shape much of the nature of the visible universe. Nuclear fusion is the engine of stars; it produces the
More informationPoS(NIC XIII)028. Measurement of the p-process branching point reaction 76 Se(α,γ) 80 Kr in inverse kinematics with DRAGON
Measurement of the p-process branching point reaction 76 Se(α,γ) 80 Kr in inverse kinematics with DRAGON 1, Charlie Akers 1,2, Alison Laird 2, Artemis Spyrou 3,4, Gregory Christian 1, Devin Connolly 5,
More informationTwo-Proton Decay Experiments at MSU
Two-Proton Decay Experiments at MSU M. Thoennessen, M. J. Chromik * and P. G. Thirolf * National Superconducting Cyclotron Laboratory and Department of Physics & Astronomy, Michigan State University East
More informationFrom Notre Dame to National Labs: Cross sections at no charge!
From Notre Dame to National Labs: Cross sections at no charge! NSL 80 th Anniversary Celebration A. Couture 8 April 2018 Operated by Los Alamos National Security, LLC for the U.S. Department of Energy's
More informationNuclear Physics Questions, Achievements, Goals
Nuclear Physics Questions, Achievements, Goals Science Questions & Goals of Nuclear Physics Current status and instrumentation Implications of Nuclear Physics for other Fields The Nuclear Chart Proton:
More informationNuclear Astrophysics
Nuclear Astrophysics IV: Novae, x-ray bursts and thermonuclear supernovae Karlheinz Langanke GSI & TU Darmstadt Aarhus, October 6-10, 2008 Karlheinz Langanke ( GSI & TU Darmstadt) Nuclear Astrophysics
More informationReaction rates in the Laboratory
Reaction rates in the Laboratory Example I: 14 N(p,γ) 15 O slowest reaction in the CNO cycle Controls duration of hydrogen burning Determines main sequence turnoff glob. cluster ages stable target can
More informationASTRONOMY 220C ADVANCED STAGES OF STELLAR EVOLUTION AND NUCLEOSYNTHESIS. Spring, 2013
ASTRONOMY 220C ADVANCED STAGES OF STELLAR EVOLUTION AND NUCLEOSYNTHESIS Spring, 2013 http://www.ucolick.org/~woosley This is a one quarter course dealing chiefly with: a) Nuclear astrophysics (and nuclear
More informationarxiv:astro-ph/ v1 23 Feb 2001
The endpoint of the rp process on accreting neutron stars H. Schatz 1, A. Aprahamian 2, V. Barnard 2, L. Bildsten 3, A. Cumming 3, M. Ouellette 1, T. Rauscher 4, F.-K. Thielemann 4, M. Wiescher 2 1 Dept.
More informationSix Days at the Edge of Space: 10 Years of HASP Balloon Flight Operations
Six Days at the Edge of Space: 10 Years of HASP Balloon Flight Operations T. Gregory Guzik, Louisiana Space Grant Consortium Department of Physics & Astronomy Louisiana State University v030316 1 Primary
More informationResearch in Physics. Why? Who pays for it? How do you decide what to do? Professor Ani Aprahamian. University of Notre Dame
Research in Physics Why? Who pays for it? How do you decide what to do? Professor Ani Aprahamian University of Notre Dame The US economy depends on Science scientific and technical innovations they produce
More informationNuclear Astrophysics
Nuclear Astrophysics Jeff Blackmon (LSU) 1. Introduction, Formalism, Big Bang and H burning 2. He burning, Heavy elements & s process 3. Stellar Explosions Dominant source of energy generation in stars
More informationRecoil Separators for Nuclear Astrophysics studies Manoel Couder
Recoil Separators for Nuclear Astrophysics studies Manoel Couder Institute for Structure and Nuclear Astrophysics University of Notre Dame Joint Institute for Nuclear Astrophysics Outline Nuclear astrophysics
More informationRare Isotopes: The DNA of Stellar Explosions
Rare Isotopes: The DNA of Stellar Explosions Chris Wrede Michigan State University National Superconducting Cyclotron Laboratory PHY492/802 substitute lecture April 21 st, 2017 Outline Introduction: How
More informationNuclear Physics Questions, Directions, Applications
Nuclear Physics Questions, Directions, Applications Science Questions & Goals of Nuclear Physics Implications of Nuclear Physics for other Fields Applications of Nuclear Physics in other Fields The Nuclear
More informationUniversity of California High-Performance AstroComputing Center JOEL PRIMACK UCSC
University of California High-Performance AstroComputing Center JOEL PRIMACK UCSC http://hipacc.ucsc.edu/ As computing and observational power continue to increase rapidly, the most difficult problems
More informationDIANA A NEXT GENERATION DEEP UNDERGROUND ACCELERATOR FACILITY
DIANA D. Leitner for the DIANA collaboration Michigan State University PAC 2011 New York, April 2011 A NEXT GENERATION DEEP UNDERGROUND ACCELERATOR FACILITY Outline of the Talk Why underground? Brief science
More informationMeasuring the Specific Heat and the Neutrino Emissivity of Dense Matter
Measuring the Specific Heat and the Neutrino Emissivity of Dense Matter Edward Brown Michigan State University Joint Institute for Nuclear Astrophysics A. Piro, Carnegie Obs. Cumming, Brown, Fattoyev,
More informationInternational Nuclear Physics Conference Adelaide, Australia September 13, 2016
International Nuclear Physics Conference Adelaide, Australia September 13, 2016 This work was performed under the auspices of the U.S. Department of Energy by under contract DE-AC52-07NA27344. Lawrence
More informationBernard Frederick Schutz
1 of 5 29/01/2007 18:13 Homepage of Bernard Schutz 14 / 24 Bernard Frederick Schutz Director, Max Planck Institute for Gravitational Physics Born 11 August 1946, Paterson, NJ, USA Nationality: USA (by
More informationThe Origin of the Elements between Iron and the Actinides Probes for Red Giants and Supernovae
The Origin of the Elements between Iron and the Actinides Probes for Red Giants and Supernovae I Outline of scenarios for neutron capture nucleosynthesis (Red Giants, Supernovae) and implications for laboratory
More informationBeta decay for neutron capture
Beta decay for neutron capture Sean Liddick ICNT, June 7th, 2016 r-process calculations neutron star merger hot wind cold wind Abundance pattern is different for the different astrophysical scenarios.
More informationThe r-process and the νp-process
The r-process and the νp-process Carla Fröhlich Enrico Fermi Fellow The Enrico Fermi Institute University of Chicago GCE April 30 / 2010 Solar System Abundances?? 2 s-process peak r-process peak s-process
More informationRare isotopes in the cosmos
Rare isotopes in the cosmos Hendrik Schatz Such stellar processes as heavy-element formation and x-ray bursts are governed by unstable nuclear isotopes that challenge theorists and experimentalists alike.
More informationHigh Resolution Spectroscopy in Nuclear Astrophysics. Joachim Görres University of Notre Dame & JINA
High Resolution Spectroscopy in Nuclear Astrophysics Joachim Görres University of Notre Dame & JINA Nuclear Astrophysics Studies at RCNP Osaka Notre Dame Groningen Started in 2002 (Georg @ RCNP) with a
More informationNuclear research and education at the Australian National University
Presentation 13 Session 4 Nuclear research and education at the Australian National University Professor Andrew Stuchbery Head, Department of Nuclear Physics, Australian National University Biography Professor
More informationarxiv: v1 [astro-ph.he] 28 Dec 2010
Published in Phys. Rev. C 82, 058801(R)(2010) Re-analysis of the (J = 5) state at 592keV in 180 Ta and its role in the ν-process nucleosynthesis of 180 Ta in supernovae T. Hayakawa Quantum Beam Science
More informationNuclear physics input for the r-process
Nuclear physics input for the r-process Gabriel Martínez Pinedo INT Workshop The r-process: status and challenges July 28 - August 1, 2014 Nuclear Astrophysics Virtual Institute Outline 1 Introduction
More informationHydrogen & Helium Burning in Stars
Hydrogen & Helium Burning in Stars What remains to be done and how to do it! Hydrogen Burning: 4 He, 14 N Helium Burning: 12 C, 16 O, 22 Ne, n, s-nuclei Alba Formicola (on behalf of LUNA collaboration)
More informationFirst direct measurement of 12 C( 12 C,n) 23 Mg at stellar energies
EPJ Web of Conferences 109, 04009 (2016) DOI: 10.1051/ epjconf/ 201610904009 C Owned by the authors, published by EDP Sciences, 2016 First direct measurement of 12 C( 12 C,n) 23 Mg at stellar energies
More informationFUNDAMENTALS OF PHYSICS Vol. III - Nuclear Synthesis In Nature- K. Langanke, M. Wiescher
NUCLEAR SYNTHESIS IN NATURE K. Langanke Institute for Physics and Astronomy, University of Aarhus, DK-8000 Aarhus C, Denmark M. Wiescher Department of Physics, University of Notre Dame, USA Keywords: Big
More informationExperimental Initiatives in Nuclear Astrophysics
Experimental Initiatives in Nuclear Astrophysics Carl Brune Astrophysics: H and He burning, S process Facilities: neutron and gamma beams, underground accelerators, ICF plasmas Joint DNP Town Meetings
More informationTheory for nuclear processes in stars and nucleosynthesis
Theory for nuclear processes in stars and nucleosynthesis Gabriel Martínez Pinedo Nuclear Astrophysics in Germany November 15-16, 2016 Nuclear Astrophysics Virtual Institute Outline 1 Ab-initio description
More informationFacility for Rare Isotope Beams Update for Nuclear Physics News
Facility for Rare Isotope Beams Update for Nuclear Physics News FRIB Overview The Facility for Rare Isotope Beams (FRIB) is a major new scientific user facility under construction in the United States
More informationBackground (α,n) reactions at low energies: 10,11 B(α,n) 13,14 N
Background (α,n) reactions at low energies: 10,11 B(α,n) 13,14 N (Richard) James deboer Nuclear Physics in Astrophysics VIII Catania, Italy June 20, 2017 Improved rates for neutron production reactions
More informationPresentation at the 10th RIBLL Collaboration Symposium, Beijing, 2017/1/7
Presentation at the 10th RIBLL Collaboration Symposium, Beijing, 2017/1/7 Outline 1. Background 1.1 Decay for proton-rich nuclei 1.2 Astrophysical implications 2. Experiments 2.1 Introduction 2.2 Experimental
More informationMeasurement of the 62,63. Ni(n,γ) cross section at n_tof/cern
Measurement of the 62,63 Ni(n,γ) cross section at n_tof/cern University of Vienna 01. September 2011 ERAWAST II, Zürich Nucleosynthesis of heavy elements BB fusion neutrons Abundance (Si=10 6 ) Fe Mass
More informationExperimental Approach to Explosive Hydrogen Burning with Low-Energy RI Beams
Hirschegg 06-1 Experimental Approach to Explosive Hydrogen Burning with Low-Energy RI Beams S. Kubono Center for Nuclear Study (CNS) University of Tokyo 1. Low Energy RI Beam Production 2. Proton Resonance
More informationLetter of Intent: Nuclear Fusion Reactions from laser-accelerated fissile ion beams
Letter of Intent: Nuclear Fusion Reactions from laser-accelerated fissile ion beams Peter G. Thirolf, LMU Munich D. Habs, H. Ruhl, J. Schreiber, LMU Munich, MPQ Garching T. Dickel, H. Geissel, W. Plass,
More informationCURRICULUM VITAE Roman V. Krems
CURRICULUM VITAE Roman V. Krems POSTAL ADDRESS: Department of Chemistry, University of British Columbia 2036 Main Mall, Vancouver, B.C. Canada V6T 1Z1 Telephone: +1 (604) 827 3151 Telefax: +1 (604) 822
More informationFuture research of 12 C(a,g) 16 O. Claudio Ugalde
Future research of 12 C(a,g) 16 O Claudio Ugalde 12 C(a,g) 16 O Reaction Key reaction for stellar structure, evolution, and nucleosynthesis in stars. Affects the synthesis of most of the elements of the
More informationMeasurements for 44 Ti at TRIUMF-ISAC 40
Measurements for Ti at TRIUMF-ISAC 40 Ca(, ) Ti and future RIB experiments (ETH Zurich) for the DRAGON collaboration Vancouver, B.C., Canada Role of Ti in Astrophysics laboratory half-life of 58.9 +/-
More informationU.S. Experimental Activities Report. WPEC Meeting, May Donald L. Smith, Chair. on behalf of the
U.S. Experimental Activities Report WPEC Meeting, 13-15 May 2002 by Donald L. Smith, Chair on behalf of the CSEWG Measurements and Basic Physics Committee Introduction This presentation summarizes the
More informationPrediction of Astrophysical Reaction Rates: Methods, Data Needs, and Consequences for Nucleosynthesis Studies
Prediction of Astrophysical Reaction Rates: Methods, Data Needs, and Consequences for Nucleosynthesis Studies arxiv:astro-ph/0007453v1 28 Jul 2000 Thomas Rauscher 1, Robert D. Hoffman 2, Stanford E. Woosley
More informationNuclear Astrophysics II
Nuclear Astrophysics II Lecture 5 Fri. June 1, 2012 Prof. Shawn Bishop, Office 2013, Ex. 12437 shawn.bishop@ph.tum.de http://www.nucastro.ph.tum.de/ 1 Where to from here? We are now at a crossroads for
More informationAn introduction to Atomki
An introduction to Atomki challenges for small scale facilities Atomki: Instititute for Nuclear Research, Hungarian Academy of Sciences Science on Stage festival 2017 10th jubilee in Debrecen/Hungary!
More informationMichigan State University, East Lansing MI48824, USA INTRODUCTION
Two-Proton Decay of the First Excited State of 17 Ne M.J. Chromik 1;2,P.G. Thirolf 1;2, M. Thoennessen 1, M. Fauerbach 1, T. Glasmacher 1, R. Ibbotson 1, R.A. Kryger 1, H. Scheit 1, and P.J. Woods 3 1
More informationNuclear astrophysics at ISOLDE
Nuclear astrophysics at ISOLDE Oliver Sølund Kirsebom Aarhus University 19 August 2015 NICE workshop, SDU 1. Experiments with radioactive beams 2. Electron-capture supernovae 3. Stellar helium burning
More informationNuclear Spectroscopy of Very Neutron-rich rich Ag and Cd Isotopes
132 Nuclear Spectroscopy of Very Neutron-rich rich Ag and Cd Isotopes Iris Dillmann*,# for the Mainz- Maryland- Oslo- CERN/ ISOLDE- Collaboration * Institut für Kernchemie, Universität Mainz (Germany)
More informationNeutrinos and Nucleosynthesis from Black Hole Accretion Disks. Gail McLaughlin North Carolina State University
Neutrinos and Nucleosynthesis from Black Hole Accretion Disks Gail McLaughlin North Carolina State University 1 Neutrino Astrophysics What do neutrinos do in astrophysical environments? What do neutrinos
More informationDecay properties of neutron-rich nuclei on the r-process path
Nuclear science frontier explored by ultra-high power lasers, Feb. 03 Osaka Decay properties of neutron-rich nuclei on the r-process path Shunji NISHIMURA ( RIKEN Nishina Center / NAOJ) Nuclear Parameters
More informationVita Davison E. Soper
Vita Davison E. Soper Title: Professor, Department of Physics Address: Institute of Theoretical Science University of Oregon Eugene, Oregon 97403-5203 Phone Number: (541) 346-5162 Education: B.A., Amherst
More informationH/He burning reactions on unstable nuclei for Nuclear Astrophysics
H/He burning reactions on unstable nuclei for Nuclear Astrophysics PJ Woods University of Edinburgh H T O F E E U D N I I N V E B R U S I R T Y H G Explosive H/He burning in Binary Stars Isaac Newton,
More informationMeasurements of the Astrophysically Important 40 Ca(α,γ) 44 Ti Reaction Rate. Daniel Robertson JINA Frontiers Meeting Oct.
Measurements of the Astrophysically Important 40 Ca(α,γ) 44 Ti Reaction Rate Daniel Robertson JINA Frontiers Meeting 21-23 Oct. 2010 Why study 44 Ti at all? Recent observations of live 44 Ti highlight
More informationProduction and Separation of Radioactive Beams. Mg and 20 Na with MARS
Production and Separation of Radioactive Beams 20 Mg and 20 Na with MARS Gopal Subedi, Colby College REU 2009, Cyclotron Institute, TAMU Advisor: Dr. Robert E. Tribble August 23, 2009 1 Overview Motivation
More informationFirst RIA Summer School on Exotic Beam Physics, August 12-17, Michael Thoennessen, NSCL/MSU. Lecture 1: Limits of Stability 1 A = 21
Limits of Stability At the moment we are limited in our view of the atomic nucleus Proton Drip Line? Known Nuclei Heavy Elements? Fission Limit? Some Basic Nuclear Property Neutron Drip Line? RIA Will
More informationStudying Neutron-Induced Reactions for Basic Science and Societal Applications
Studying Neutron-Induced Reactions for Basic Science and Societal Applications Correlations in Hadronic and Partonic Interactions 2018 A. Couture Yerevan, Armenia 28 September 2018 Operated by Los Alamos
More information