Statements (64)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:physicist
|
| gptkbp:bfsLayer |
2
|
| gptkbp:bfsParent |
gptkb:physicist
|
| gptkbp:average_temperature |
10^8 K
|
| gptkbp:can_be |
gptkb:Nuclear_Pasta
gptkb:Superfluid_Neutrons |
| gptkbp:composed_of |
Electrons
Neutrons Protons |
| gptkbp:diameter |
1 km to 2 km
|
| gptkbp:examines |
gptkb:physicist
Stellar Evolution Astrophysical Research Stellar Remnants |
| gptkbp:exhibits |
Crystallization
|
| gptkbp:financial_performance |
Degenerate Pressure
|
| https://www.w3.org/2000/01/rdf-schema#label |
Neutron Star Crust
|
| gptkbp:is_affected_by |
Thermal Conductivity
Magnetic Fields Thermal Equilibrium Nuclear Forces |
| gptkbp:is_associated_with |
gptkb:Gravitational_Waves
Pulsars X-ray Binaries |
| gptkbp:is_characterized_by |
High Density
High Energy Density High Pressure Extreme Conditions Low Temperature Quantum Effects Non-ideal Behavior |
| gptkbp:is_considered |
Theoretical Models
Astrophysical Simulations Astrophysical Models Astrophysical Observations |
| gptkbp:is_explored_in |
Numerical Relativity
Observational Astronomy |
| gptkbp:is_influenced_by |
gptkb:Neutron_Star_Mergers
gptkb:Electromagnetic_Radiation Supernova Explosions |
| gptkbp:is_linked_to |
gptkb:Gamma-Ray_Bursts
Astrophysical Events Neutron Star Cooling Neutron Star Formation |
| gptkbp:is_part_of |
gptkb:physicist
gptkb:Compact_Objects High-Energy Astrophysics Astrophysical Objects Neutron Star Interior Neutron Star Structure |
| gptkbp:is_related_to |
gptkb:political_movement
Nuclear Physics Cosmic Rays |
| gptkbp:is_studied_in |
gptkb:Neutron_Star_Mergers
gptkb:observatory Astrophysical Phenomena Neutron Star Properties Equation of State Neutron Star Mass Limits |
| gptkbp:is_subject_to |
Extreme Gravity
|
| gptkbp:located_in |
gptkb:Outer_Layer_of_Neutron_Star
|
| gptkbp:occurs_in |
Phase Transitions
|
| gptkbp:population |
10^17 kg/m^3
|
| gptkbp:supports |
Nuclear Reactions
|