The table below shows the most common keywords used by the author. The letters in brackets after some keywords denote if the keyword corresponds to Solar Physics (S) or Heliospheric Physics (H).
| Keyword
| Occurrences
|
|---|
| =A<
| 48
|
| Nuclear Experiment
| 32
|
| 6<
| 25
|
| 27.20.+n
| 25
|
| =19
| 25
|
| Transfer Reactions
| 25
|
| 27.30.+t
| 14
|
| =38
| 14
|
| 20<
| 14
|
| Nucleosynthesis In Novae Supernovae And Other Explosive Environments
| 12
|
| 25.70.Hi
| 12
|
| Decay By Proton Emission
| 11
|
| Electron And Muon Capture
| 11
|
| 23.50.+z
| 11
|
| 23.40.-s
| 11
|
| Hydrostatic Stellar Nucleosynthesis
| 11
|
| Beta Decay
| 11
|
| Double Beta Decay
| 11
|
| Spectroscopic Factors And Asymptotic Normalization Coefficients
| 9
|
| Nuclear Theory
| 9
|
| 21.10.Jx
| 9
|
| 26.20.+f
| 8
|
| Elastic Scattering
| 8
|
| 25.60.Bx
| 8
|
| 25.60.-t
| 7
|
| 25.60.Gc
| 7
|
| 25.40.Lw
| 7
|
| Radiative Capture
| 7
|
| Lifetimes
| 7
|
| Reactions Induced By Unstable Nuclei
| 7
|
| 21.10.Tg
| 7
|
| Breakup And Momentum Distributions
| 7
|
| 21.10.Dr
| 6
|
| 26.65.+t
| 6
|
| 25.40.Hs
| 6
|
| Nuclear Reaction Models And Methods
| 6
|
| Solar Neutrinos
| 6
|
| Elastic And Quasielastic Scattering
| 6
|
| 25.60.Je
| 6
|
| 26.30.-k
| 6
|
| 25.70.Bc
| 6
|
| Binding Energies And Masses
| 6
|
| 26.30.+k
| 6
|
| Nucleosynthesis
| 6
|
| 24.10.-i
| 6
|
| 23.40.Bw
| 5
|
| 24.10.Ht
| 5
|
| 26.30.Ca
| 5
|
| Optical And Diffraction Models
| 5
|
| Weak-interaction And Lepton Aspects
| 5
|
| Explosive Burning In Accreting Binary Systems
| 5
|
| 26.50.+x
| 4
|
| 39<
| 4
|
| Beta-decay
| 4
|
| Gamma Transitions And Level Energies
| 4
|
| 23.20.Lv
| 4
|
| Micro Pattern Gas Amplifier Detector
| 4
|
| 24.30.Gd
| 4
|
| Other Resonances
| 4
|
| 27.40.+z
| 4
|
| Nuclear Physics Aspects Of Novae Supernovae And Other Explosive Environments
| 4
|
| Radioactive Ion Beams
| 4
|
| =58
| 4
|
| 21.10.Re
| 3
|
| 24.50.+g
| 3
|
| Collective Levels
| 3
|
| Supernovae
| 3
|
| Cluster Models
| 3
|
| Interaction And Reaction Cross Sections
| 3
|
| Nuclear Reactions
| 3
|
| 23.40.Hc
| 3
|
| Direct Reactions
| 3
|
| Relation With Nuclear Matrix Elements And Nuclear Structure
| 3
|
| Resonances
| 3
|
| Science And Society
| 3
|
| 25.70.Ef
| 3
|
| Publisher's Note
| 3
|
| 27.60.+j
| 3
|
| X-ray Bursts
| 3
|
| 25.60.Dz
| 3
|
| 90<
| 3
|
| 99.10.Fg
| 3
|
| =149
| 3
|
| 21.60.Gx
| 3
|
| 01.75.+m
| 3
|
| 26.20.-f
| 3
|
| X-ray Sources
| 2
|
| X- And Gamma-ray Spectroscopy
| 2
|
| Strongly Damped Collisions
| 2
|
| Spin Parity And Isobaric Spin
| 2
|
| Spectrometers
| 2
|
| Sources Of Radioactive Nuclei
| 2
|
| 01.10.Fv
| 2
|
| Resonance
| 2
|
| Properties Of Nuclei
| 2
|
| Physics - Instrumentation And Detectors
| 2
|
| Nucleosynthesis In Late Stellar Evolution
| 2
|
| Nuclear Tests Of Fundamental Interactions And Symmetries
| 2
|
| Nuclear Structure
| 2
|
| Nuclear Energy Levels
| 2
|
| Nuclear Astrophysics
| 2
|
| MPGAD
| 2
|
| Micromegas
| 2
|
| Mass And Neutron Distributions
| 2
|
| Ionisation Chambers
| 2
|
| Implantation
| 2
|
| Gas-filled Counters: Ionization Chambers Proportional And Avalanche Counters
| 2
|
| Excited States
| 2
|
| Elastic And Inelastic Scattering
| 2
|
| Cyclotrons
| 2
|
| Coupled-channel And Distorted-wave Models
| 2
|
| Coulomb Energies
| 2
|
| Conferences Lectures And Institutes
| 2
|
| Compound Nucleus
| 2
|
| Collective Models
| 2
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 2
|
| Angular Distribution And Correlation Measurements
| 2
|
| Alpha Decay
| 2
|
| Abundances
| 2
|
| 98.70.Qy
| 2
|
| 29.40.Cs
| 2
|
| 29.30.Kv
| 2
|
| 29.25.Rm
| 2
|
| 26.20.Np
| 2
|
| 25.70.Lm
| 2
|
| 25.70.Gh
| 2
|
| 25.45.De
| 2
|
| 24.80.+y
| 2
|
| 24.10.Eq
| 2
|
| 23.60.+e
| 2
|
| 23.20.En
| 2
|
| 21.60.Ev
| 2
|
| 21.60.Cs
| 2
|
| 21.10.Sf
| 2
|
| 21.10.Hw
| 2
|
| 21.10.Gv
| 2
|
| 21.10.-k
| 2
|
| Shell Model
| 2
|
| Direct Measurements
| 1
|
| Normalising
| 1
|
| Dark Matter
| 1
|
| Dark Energy
| 1
|
| 01.40.-d
| 1
|
| Course Design And Evaluation
| 1
|
| Thick Target Method
| 1
|
| Three-body Coulomb Problem
| 1
|
| Cosmic Ray Nucleosynthesis
| 1
|
| Tracking And Position-sensitive Detectors
| 1
|
| Two-proton Decay
| 1
|
| Ultra-low Background
| 1
|
| Nuclear Astrophysics - Direct Nuclear Reactions - DWBA Analysis
| 1
|
| Nuclear Data Compilation
| 1
|
| Charged-particle Spectrometers: Electric And Magnetic
| 1
|
| Nuclear Matter
| 1
|
| Black Holes
| 1
|
| Nuclear Physics For Astrophysics
| 1
|
| Nuclei With Mass Number 20 To 38
| 1
|
| Other Topics In Nuclear Reactions: Specific Reactions
| 1
|
| Asymptotic Stability
| 1
|
| βp βγ
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astrophysical S-factor
| 1
|
| Astronomical Telescopes
| 1
|
| Astronomical Catalogs Atlases Sky Surveys Databases Retrieval Systems Archives Etc.
| 1
|
| 21.65.-f
| 1
|
| And Other Explosive Environments
| 1
|
| White Paper
| 1
|
| Activation Methods
| 1
|
| 21.60.Fw
| 1
|
| Particle Identification
| 1
|
| =89
| 1
|
| Peripheral Collisions
| 1
|
| Physics
| 1
|
| Physics - Accelerator Physics
| 1
|
| =189
| 1
|
| Position Sensitive Particle Detectors
| 1
|
| 2H-induced Reactions
| 1
|
| Potential Energy Surfaces For Excited Electronic States
| 1
|
| 98.70.Rz
| 1
|
| 150<
| 1
|
| 97.60.Lf
| 1
|
| 97.60.Bw
| 1
|
| 97.20.Li
| 1
|
| 97.10.Cv
| 1
|
| 96.50.-e
| 1
|
| 95.80.+p
| 1
|
| 95.75.Pq
| 1
|
| 95.55.Fw
| 1
|
| 95.55.Cs
| 1
|
| 95.36.+x
| 1
|
| 95.35.+d
| 1
|
| Projectile And Target Fragmentation
| 1
|
| Projectile Fragments
| 1
|
| 59<
| 1
|
| Proton Decay
| 1
|
| 32.80.Rm
| 1
|
| 31.50.Df
| 1
|
| 29.87.+g
| 1
|
| 29.40.Wk
| 1
|
| 29.40.Gx
| 1
|
| 01.78.+p
| 1
|
| X-ray Astronomy
| 1
|
| 29.30.Aj
| 1
|
| β–p Decay Of 20Mg
| 1
|
| 29.20.dg
| 1
|
| 27.70.+q
| 1
|
| Proton Detection
| 1
|
| 27.50.+e
| 1
|
| Proton Radiative Capture
| 1
|
| Radiative Transfer [S]
| 1
|
| Radioactive Sources
| 1
|
| 26.65.+t Solar Neutrinos
| 1
|
| Rare Isotope Production
| 1
|
| Reaction Kinetics
| 1
|
| 26.40.+r
| 1
|
| Research In Physics Education
| 1
|
| Resonance Reactions
| 1
|
| 26.30.+k Nucleosynthesis In Novae
| 1
|
| Review
| 1
|
| X-rays
| 1
|
| S-factors.
| 1
|
| 26.20.+f Hydrostatic Stellar Nucleosynthesis
| 1
|
| Scattering
| 1
|
| 25.90.+k
| 1
|
| 25.70.Pq
| 1
|
| 25.70.Mn
| 1
|
| 21.10.Pc
| 1
|
| Science And Government
| 1
|
| β-p Decay Of 20Mg
| 1
|
| Scientific Societies
| 1
|
| Scientific Visualisation
| 1
|
| 25.70.-z
| 1
|
| Single-particle Levels And Strength Functions
| 1
|
| 25.60.Gc Breakup And Momentum Distributions
| 1
|
| Social Sciences
| 1
|
| Societies
| 1
|
| Solid-state Detectors
| 1
|
| 25.60.-t Reactions Induced By Unstable Nuclei
| 1
|
| Space-based Ultraviolet Optical And Infrared Telescopes
| 1
|
| 25.55.Hp
| 1
|
| 01.40.Fk
| 1
|
| 25.45.-z
| 1
|
| Stars: Abundances
| 1
|
| Stars: AGB And Post-AGB
| 1
|
| 25.40.Cm
| 1
|
| 01.40.Di
| 1
|
| 24.60.Dr
| 1
|
| Statistical Compound-nucleus Reactions
| 1
|
| Stellar Evolution
| 1
|
| Ionization Chamber
| 1
|
| 24.30.-v
| 1
|
| Interplanetary Physics [H]
| 1
|
| Low And Intermediate Energy Heavy-ion Reactions
| 1
|
| Stellar Structure Interiors Evolution Nucleosynthesis Ages
| 1
|
| Hyperspherical Harmonic Method
| 1
|
| Magnetic Spectrometer
| 1
|
| Hot CNO Breakout
| 1
|
| Hindrance
| 1
|
| High Energy Physics - Phenomenology
| 1
|
| Ground-based Ultraviolet Optical And Infrared Telescopes
| 1
|
| Giant And Subgiant Stars
| 1
|
| βp βα
| 1
|
| Gamma-rays
| 1
|
| Gamma-ray Sources
| 1
|
| Gamma-ray Bursts
| 1
|
| Mathematical Procedures And Computer Techniques
| 1
|
| Fusion Cross Section
| 1
|
| Fermi Energy
| 1
|
| Extrapolation Models
| 1
|
| Explosive Nuclear Astrophysics
| 1
|
| Models Based On Group Theory
| 1
|
| Experiments
| 1
|
| 24.10.-i Nuclear Reaction Models And Methods
| 1
|
| Molecule-electron Collisions
| 1
|
| Multifragment Emission And Correlations
| 1
|
| Elastic Proton Scattering
| 1
|
| Multiphoton Ionization And Excitation To Highly Excited States
| 1
|
| Telescopes
| 1
|
| Educational Institutions
| 1
|
| Education
| 1
|
| Neutron-proton Interactions
| 1
|
| Neutron-rich Nuclides
| 1
|
| Deep Inelastic Transfer
| 1
|