Publication data of Ostgaard, Erlend:
Link to Inspire
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Citations
Citations
w/o self-citaion
self-citaion
1970
1980
1990
2000
2010
2020
0
200
400
600
800
Created with Highcharts 9.0.1
Publications
publications per year
Publications
Publications per year
Cumulative publications
1970
1980
1990
2000
2010
2020
0
12
24
36
48
60
0
1.5
3
4.5
6
7.5
Created with Highcharts 9.0.1
h-index
h-index
h-index
h-index w/o self-citaion
1970
1980
1990
2000
2010
2020
0
2
4
6
8
10
12
Created with Highcharts 9.0.1
Citations
Breakdown of Most Cited Papers
rest
Calculations of total mass, radius, and moment of inertia for neutron stars
Towards solution of the gamma-ray burst mystery. 2. 'Failed type I supernova / hypernova' in high redshift starburst galaxies
Towards solution of the gamma-ray burst mystery. 2. 'Failed type I supernova…
ENERGY AND MAGNETIC SUSCEPTIBILITY OF NEUTRON MATTER. 2. VARIATIONAL CALCULATIONS BY PANDHARIPANDE'S LOCV METHOD
ENERGY AND MAGNETIC SUSCEPTIBILITY OF NEUTRON MATTER. 2. VARIATION…
Neutron star matter. Phase transition to a neutron solid?
SOLID CORES IN NEUTRON STARS?
Electrical conductivity of neutron star cores in the presence of strong magnetic fields: Effects of interactions and superfluidity of nucleons
Electrical conductivity of neutron star cores in the presence of strong magne…
Lowest-order constrained-variation calculations of binding energies for symmetric and asymmetric nuclear matter
Lowest-order constrained-variation calculations of binding energies for symm…
Neutron matter calculations by the Fermi-hypernetted-chain method
Liquid He-3. 3. The Binding Energy and Other Properties at Zero Temperature
Neutron star properties from modern meson exchange potential models
Null geodesics and embedding diagrams of the interior Schwarzschild-de Sitter space-times with uniform density
Null geodesics and embedding diagrams of the interior Schwarzschild-de Sitt…
Calculations of mass and moment of inertia for neutron stars
Kerr-Newman-de Sitter black holes with a restricted repulsive barrier of equatorial photon motion
Kerr-Newman-de Sitter black holes with a restricted repulsive barrier of equat…
Solution of the Bethe-Goldstone equation
Neutron matter
SUPERFLUIDITY OF NEUTRON MATTER. 1. SINGLET PAIRING
Superfluidity of neutron matter (II). triplet pairing
Asymmetric nuclear matter and neutron star properties
Asymmetric nuclear matter and neutron star properties
1970
1980
1990
2000
2010
2020
0
200
400
600
800
Created with Highcharts 9.0.1
Fraction [%]
Breakdown of Most Cited Papers (Fraction)
Calculations of total mass, radius, and moment of inertia for neutron stars
Towards solution of the gamma-ray burst mystery. 2. 'Failed type I supernova / hypernova' in high redshift starburst galaxies
Towards solution of the gamma-ray burst mystery. 2. 'Failed type I supernova…
ENERGY AND MAGNETIC SUSCEPTIBILITY OF NEUTRON MATTER. 2. VARIATIONAL CALCULATIONS BY PANDHARIPANDE'S LOCV METHOD
ENERGY AND MAGNETIC SUSCEPTIBILITY OF NEUTRON MATTER. 2. VARIATION…
Neutron star matter. Phase transition to a neutron solid?
SOLID CORES IN NEUTRON STARS?
Electrical conductivity of neutron star cores in the presence of strong magnetic fields: Effects of interactions and superfluidity of nucleons
Electrical conductivity of neutron star cores in the presence of strong magne…
Lowest-order constrained-variation calculations of binding energies for symmetric and asymmetric nuclear matter
Lowest-order constrained-variation calculations of binding energies for symm…
Neutron matter calculations by the Fermi-hypernetted-chain method
Liquid He-3. 3. The Binding Energy and Other Properties at Zero Temperature
Neutron star properties from modern meson exchange potential models
Null geodesics and embedding diagrams of the interior Schwarzschild-de Sitter space-times with uniform density
Null geodesics and embedding diagrams of the interior Schwarzschild-de Sitt…
Calculations of mass and moment of inertia for neutron stars
Kerr-Newman-de Sitter black holes with a restricted repulsive barrier of equatorial photon motion
Kerr-Newman-de Sitter black holes with a restricted repulsive barrier of equat…
Solution of the Bethe-Goldstone equation
Neutron matter
SUPERFLUIDITY OF NEUTRON MATTER. 1. SINGLET PAIRING
Superfluidity of neutron matter (II). triplet pairing
Asymmetric nuclear matter and neutron star properties
Asymmetric nuclear matter and neutron star properties
1970
1980
1990
2000
2010
2020
0
25
50
75
100
Created with Highcharts 9.0.1
Citations/1 Year
Citations/Period
Citations / 1 Year
Moving average
1970
1980
1990
2000
2010
2020
0
10
20
30
40
50
1 Month
3 Months
6 Months
12 Months