Solutions.

Slides:



Advertisements
Similar presentations
Neutron-induced Reactions
Advertisements

Methods to directly measure non-resonant stellar reaction rates
NUCLEAR REACTION MODELS FOR SYSTEMATIC ANALYSIS OF FAST NEUTRON INDUCED (n,p) REACTION CROSS SECTIONS M.Odsuren, J.Badamsambuu, G.Khuukhenkhuu Nuclear.
Experimental studies of low energy proton irradiation of thin vacuum deposited Aluminum layers T. Renger, M. Sznajder, U.R.M.E. Geppert Chart.
Nuclear Astrophysics II Lecture 5 Fri. June 1, 2012 Prof. Shawn Bishop, Office 2013, Ex
The 12C+12C fusion reaction: a new opportunity at ATLAS Xiaodong Tang 1 & Chenglie Jiang 2 1) Univ. of Notre Dame 2) ANL.
Classical novae, type I x-ray bursts, and ATLAS Alan Chen Department of Physics and Astronomy McMaster University.
Experimental Determination of Neutron Cross Sections of Yttrium by Activation Method by Barbara Geier Supervisors: Assoc. Prof Dr. Wolfgang Sprengel RNDr.
Nuclear Reactions Kinematics. m d c 2 + m Li c 2 E* m Be c m  c 2 + m  c 2.
Neutral Particles. Neutrons Neutrons are like neutral protons. –Mass is 1% larger –Interacts strongly Neutral charge complicates detection Neutron lifetime.
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.
Reminder n Please return Assignment 1 to the School Office by 13:00 Weds. 11 th February (tomorrow!) –The assignment questions will be reviewed in next.
CNO cycle All initial abundances within a cycle serve as catalysts and accumulate at largest  Extended cycles introduce outside material into CN cycle.
25 9. Direct reactions - for example direct capture: Direct transition from initial state |a+A> to final state B +  geometrical.
Neutrinos from the primary proton- proton fusion process in the Sun pp neutrinos constitute nearly the entirety of solar neutrino flux Secondary neutrinos.
Cross section measurements for analysis of D and T in thicker films Liqun Shi Institute of Modern Physics, Fudan University, Shanghai, , People’s.
Validation of the Bremsstrahlung models Susanna Guatelli, Barbara Mascialino, Luciano Pandola, Maria Grazia Pia, Pedro Rodrigues, Andreia Trindade IEEE.
Shall We Play a Game of Thermonuclear War?. 2Thermonuclear Energy Thermonuclear Energy Sources Electrostatic Potential Electrostatic Potential E c ~ e.
Data processing in the Activation technique experiment. Making stacked or sandwiched in the repeated order of Al-Cu-Mo. Irradiation of the samples Using.
Ruđer Bošković Institute, Zagreb, Croatia CRP: Development of a Reference Database for Ion Beam Analysis Measurements of differential cross sections for.
New methods to measure the cross sections of 12 C+ 12 C fusion reaction Xiao Fang Department of Physics University of Notre Dame.
Lambda hypernuclear spectroscopy at JLab Hall-C Graduate School of Science, Tohoku University Toshiyuki Gogami for the HES-HKS collaboration 1.Introduction.
University of Victoria Astr 501 Matt Penrice
Audrey Wright TUNL REU 2013 University of Texas at Austin Adviser: Dr. Calvin Howell Other Group Members: Dr. Alexander Crowell, Dr. Mitzi Boswell Evaluating.
If the Coordinates system is. R r b (impact parameter.
Nuclear astrophysics data needs for charged-particle reactions C. Iliadis (University of North Carolina)
 -capture measurements with the Recoil-Separator ERNA Frank Strieder Institut für Physik mit Ionenstrahlen Ruhr-Universität Bochum HRIBF Workshop – Nuclear.
Nuclear structure and fundamental interactions Solid state physics Material irradiation Micrometeorite research and study Astrophysics Nuclear astrophysics.
Studies of Helium proportional counters response on fast neutrons, at NCSR “Demokritos” M. Zamani, M. Manolopoulou, S. Stoulos, M. Fragopoulou School of.
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,
ALNA- Accelerator Laboratory for Nuclear Astrophysics Underground Heide Costantini University of Notre Dame, IN, USA INFN, Genova, Italy.
3/2003 Rev 1 I.2.9 – slide 1 of 35 Session I.2.9 Part I Review of Fundamentals Module 2Basic Physics and Mathematics Used in Radiation Protection Session.
 ( E ) = S(E) e –2   E -1 2      m  m   m   m   Reaction Rate(star)    (E)  (E) dE Gamow Peak  Maxwell Boltzmann.
 ( E ) = S(E) e –2   E -1 2       m  m   m   m   Reaction Rate(star)    (E)  (E) dE Gamow Peak  Maxwell Boltzmann.
Particle Production of Carbon Target with 20Tto2T5m Configuration at 6.75 GeV (Updated) X. Ding, UCLA Target Studies April 3, /3/14.
(F.Cusanno, M.Iodice et al,Phys. Rev. Lett (2009). 670 keV FWHM  M. Iodice,F.Cusanno et al. Phys.Rev.Lett. 99, (2007) 12 C ( e,e’K )
Neutrino-Nucleus Reactions at Medium and Low Energies [contents] 1. Neutrino and weak interaction 2. Cross section for ν-A and e-A reactions 3. EMC effect.
POLARIZATION MEASUREMENTS AND ABSOLUTE POLARIZATION VALUES EVOLUTION DURING PROTON BEAM ACCELERATION IN THE RHIC ACCELERATOR COMPLEX A.Zelenski, T.Roser,
Jan. 18, 2008 Hall C Meeting L. Yuan/Hampton U.. Outline HKS experimental goals HKS experimental setup Issues on spectrometer system calibration Calibration.
Experimental Nuclear Astrophysics: Key aspects & Open problems Marialuisa Aliotta School of Physics University of Edinburgh Nuclear Physics Autumn Retreat.
Search for low spin states at high excitation energies in 20 Ne with the p,t reaction iThemba LABS & Stellenbosch University Energy Postgraduate Conference.
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1.
NEEP 541 – Neutron Damage Fall 2002 Jake Blanchard.
Meson Production at Low Proton Beam Energy (Update) X. Ding, UCLA Target Studies May 9, /9/113.
An alternative description of electron screening Matej Lipoglavšek Jožef Stefan Institute, Ljubljana, Slovenia Instit ut "Jož ef Stefa n" Russbach, March.
Shuya Ota: Japan Atomic Energy Agency, Rutgers University H. Makii, T. Ishii, K. Nishio, S. Mitsuoka, I. Nishinaka : Japan Atomic Energy Agency M. Matos,
 -capture measurements with a Recoil-Separator Frank Strieder Institut für Physik mit Ionenstrahlen Ruhr-Universität Bochum Int. Workshop on Gross Properties.
Cross Section Measurement of 9 Be( ,n) 8 Be and Implications for α+α+n-> 9 Be in the r-Process C.W. Arnold, T.B. Clegg, C. Iliadis, H.J. Karwowski, G.C.
V. Nuclear Reactions Topics to be covered include:
David Mountford University of Edinburgh
University of Colorado
Nuclear Reaction Studies for Explosive Nuclear Astrophysics
the s process: messages from stellar He burning
Direct measurements for nuclear
12C(p,)13N Nuclear Reaction Rates  12C 13N Nuclear reactions
Report to Delta Review: Hadronic Validation
Nucleosynthesis 12 C(
Guidance for hands-on exercise Neutron target
Matteo Negrini Università degli Studi di Ferrara - INFN
1. Introduction Secondary Heavy charged particle (fragment) production
Study of the resonance states in 27P by using
Study of the resonance states in 27P by using
Fragmentation cross sections of Fe26+, Si14+ and C6+ ions of 0
 s(E) = S(E) e–2ph E-1 s Nuclear Burning in Stars s(Estar) s
Elastic alpha scattering experiments
Nuclear structure of 8B studied by proton resonance scatterings on 7Be
Experiment (Jlab Exp : CLAS eg3)
The Nanosecond bunching system at KIGAM Tandem Accelerator
Shall We Play a Game of Thermonuclear War?
Proposal for an Experiment: Photoproduction of Neutral Kaons on Deuterium Spokespersons: D. M. Manley (Kent State University) W. J. Briscoe (The George.
Presentation transcript:

Solutions

Cross section vs. experimental yield [for special case of “thin” target] Example: 1H + 1H 2H + e+ +  (first step of pp chain; solar Gamow peak: 6 keV) cross section: theo=8·10-48 cm2=8·10-24 barn at Elab=1 MeV [Ecm=0.5 MeV] proton beam: total charge (Q), current (I), elementary charge N0/t=(Q/t)/q=I/q=1 Ampere/1.6·10-19 C=6·1018 incident protons/s proton target: dense hydrogen gas [Nt=1020 protons/cm2] ® Nr=(8·10-48 cm2)(1020 protons/cm2)(6·1018 protons/s)=5·10-9/s [1 reaction in 6 years!] We need very high beam currents of very low energies!

From: Newton, J. R. , Longland, R. , and Iliadis, C From: Newton, J.R., Longland, R., and Iliadis, C. Matching of experimental and statistical-model thermonuclear reaction rates at high temperatures. Phys. Rev. C 78, 025805, 8 pages (2008). Se also: Newton, J.R., Iliadis, C., Champagne, A.E., Coc, A., Parpottas, Y., and Ugalde, C. Gamow peak in