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Separation energy
Arxiv:1904.10318V1 [Nucl-Th] 20 Apr 2019 Ucinltheory
Range of Usefulness of Bethe's Semiempirical Nuclear Mass Formula
Modern Physics to Which He Did This Observation, Usually to Within About 0.1%
R-Process Nucleosynthesis: on the Astrophysical Conditions
Final Excitation Energy of Fission Fragments
Semi-Empirical Mass Formula 3.3 4.6 7.2 Ch 4
Nuclear Reaction Rates
Handbook for Calculations of Nuclear Reaction Data, RIPL-2 Reference Input Parameter Library-2
Nuclear Physics and Astrophysics SPA5302, 2019 Chris Clarkson, School of Physics & Astronomy
[email protected]
Magic Numbers Nucleon Separation Energies
Nuclear Binding Energy 1 Nuclear Binding Energy
Nuclear and Nuclear Excitation Energies
ENERGY DEPENDENT PROMPT NEUTRON MULTIPLICITY PARAMETERIZATION for ACTINIDE PHOTOFISSION A.I. Lengyel , O.O. Parlag , I.V. Pylyp
CONFIRMATION of the ISOMERIC STATE in 26P PHYSICAL REVIEW C 96, 014306 (2017) and the Decay Station
A Study of Nuclear Binding Energy of Magic Number Nuclei and Energy Splitting Considering Independent Particle Shell Model
Single-Particle Properties and Nuclear Data
Nuclear Stability, the Shell Model Nuclear Stability
Neutron Separation Energies of Ca, Sn and Pb Isotopes Using Different
Top View
Lecture Notes, Chapter 5. Nuclear Structure
Mass Chains of Light Hypernuclei and Separation Energies of Mirror Hypernuclei from BWMH Mass Formula
R-Process Nucleosynthesis of the Heavy Elements
Fissility of Actinide Nuclei by 60-130 Mev Photons
Arxiv:1104.0066V2 [Nucl-Th] 12 Jul 2011
Arxiv:1904.09962V1 [Nucl-Ex] 22 Apr 2019
Nuclear Photofissility in the Quasi-Deuteron Energy Region
SUB-BARRIER PHOTOFISSION MEASUREMENTS in 238U and 232Th
Neutron Star Mergers and Nucleosynthesis of Heavy Elements
And Two-Neutron Separation Energies for Neutron-Rich Copper Isotopes *
Formation of Medium Heavy Mass Nuclei Through R-Process R. R. Swain1, S
One and Two Proton Separation Energies from Nuclear Mass Systematics Using Neural Networks
Nuclear Properties for Astrophysical and Radioactive-Ion-Beam Applications∗
Assignment # 3
Β − H + N → H 2 (Stable) + N → H 3 (Unstable) → He3 (Stable) + N → He 4 (Stable)
Finding Nuclear Drip Lines and Studying Two Proton Emission
Lecture 1: Light and Unbound Nuclei
Nuclear Drip Line 1 Nuclear Drip Line
Lecture 2 (Pdf)
And Two-Nucleon Halo Nuclei in Effective Field Theory (160 Pp.) Director of Dissertation: Daniel R
Arxiv:1705.08329V2 [Nucl-Th] 30 Jul 2017 Components: One for Even-Even Nuclei, One for Odd- Very Important)
238U Photofission in the Energy Region of the Giant Dipole
Arxiv:1604.08143V1 [Nucl-Th] 27 Apr 2016 Clei
Nuclear Structure of 186Re David A
Proton and Neutron Drip Lines
Lecture 16 Slides
Measurements of Isomeric Yield Ratios of Proton-Induced Fission of U and Th
Prompt Neutron Polarization Asymmetries in Photofission Of