High-Energy Calibration of a BGO detector of the GLAST Burst Monitor Andreas von Kienlin*, Gerald J. Fishman¶, Michael S. Briggs§, Gary L. Godfrey† and Helmut Steinle* *

Source URL: www.batse.msfc.nasa.gov

• Radioactivity
• Astrophysics
• Fermi Gamma-ray Space Telescope
• Spaceflight
• Gamma ray
• Electronvolt
• Electron
• Physics
• Space telescopes
• Nuclear physics

Marina Barbui, Ph.D. Texas A&M University Measuring cross-sections of astrophysical interest in a laser experiment Measuring cross-sections of astrophysical interest at very low

Source URL: physics.tamu.edu

• Materials science
• Quantum electrodynamics
• Energy conversion
• Nuclear fusion
• Plasma
• Coulomb explosion
• Electron
• Laser
• Nuclear reaction
• Physics
• Astrophysics
• Nuclear physics

Physics high-ranking Journals (category 2) Advances in Physics Annual Review of Astronomy and Astrophysics Annual Review of Nuclear and Particle Science Applied Physics Letters Astronomy & Astrophysics

Source URL: phys.au.dk

• Physical Review Letters
• Physical chemistry
• Nature Chemistry
• Physics Letters
• Chemical physics
• ChemBioChem
• American Chemical Society
• Journal of Physics B
• Methods in Organic Synthesis
• Publishing
• Chemistry
• Academic publishing

BOOK REVIEWS The Evolution of Matter: From the Big Bang to the Present Day2 Earth scientists have long embraced the deep dimension of time and the powerful unifying

Source URL: www.elementsmagazine.org

• Nuclear physics
• Structure of the Earth
• Astrophysics
• Nucleosynthesis
• Formation and evolution of the Solar System
• Chemical element
• Isotope
• Subduction
• Crust
• Geology
• Plate tectonics
• Physics

© 2015 UK ATOMIC ENERGY AUTHORITY The following article appeared in Nuclear Fusion, Vol.55, No.1, January 2015, ppMitigation of MHD induced fast-ion redistribution in MAST and implications for MAST-Upgrade desig

Source URL: www.ccfe.ac.uk

• Chemistry
• Astrophysics
• Fusion power
• Plasma
• Neutral beam injection
• Tokamak
• Nuclear fusion
• Ion source
• Madison Symmetric Torus
• Physics
• Fusion reactors
• Plasma physics

THEORETICAL PROBLEM No. 3 WHY ARE STARS SO LARGE? The stars are spheres of hot gas. Most of them shine because they are fusing hydrogen into helium in their central parts. In this problem we use concepts of both classica

Source URL: www.jyu.fi

• Nuclear chemistry
• Nuclear physics
• Chemical elements
• Stellar astronomy
• Astrophysics
• Nuclear fusion
• Helium
• Star
• Electron
• Physics
• Chemistry
• Matter

Early Galactic Chemical Evolution and r-Process Nucleosynthesis in Black-Hole forming Supernovae [1] W. Aoki (NAOJ), T. Suda (NAOJ), T. Kajino (NAOJ/UT), R. N. Boyd (University of California, Lawrence Livermore National

Source URL: th.nao.ac.jp

• Nuclear physics
• Supernovae
• Light sources
• Nucleosynthesis
• Supernova
• Abundance of the chemical elements
• Star
• R-process
• Chemical element
• Physics
• Astronomy
• Astrophysics

PHD QUALIFY EXAMINATION — STELLAR ASTROPHYSICS March, points) A low mass sequence star has mass M , radius R and effective surface temperature Teff . (a) (15 points) Find the average time a photon reside

Source URL: www.astro.ncu.edu.tw

• Stellar evolution
• Space
• Stellar astronomy
• Light sources
• Hertzsprung-Russell classifications
• Star
• White dwarf
• Nuclear fusion
• Main sequence
• Astronomy
• Physics
• Star types

Antonios Kontos, Ph.D. MIT Kavli Institute of Astrophysics and Space Research New nuclear physics tools for the study of Classical Novae and X-ray Bursts Classical Novae and X-ray bursts are explosive

Source URL: physics.tamu.edu

computational infrastructure for nuclear astrophysics Michael(Smith,(Physics(Division,(Oak(Ridge(Na:onal(Lab(

Source URL: www.nucastrodata.org

• Nuclear astrophysics
• Nova
• Uncertainty
• Knowledge
• Astrophysics
• Statistics
• Science