Statements (53)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:watch
|
| gptkbp:bfsLayer |
3
|
| gptkbp:bfsParent |
gptkb:Neutron_Star_Crust
|
| gptkbp:affects |
thermal conductivity
neutron star stability |
| gptkbp:can_create |
very low temperatures
|
| gptkbp:can_lead_to |
neutron superfluidity
|
| gptkbp:composed_of |
gptkb:neutrons
|
| gptkbp:exhibits |
phase transitions
vortex formation quantum behavior quantum turbulence |
| gptkbp:first_described_by |
gptkb:Lev_Landau
|
| gptkbp:flows_into |
without friction
|
| gptkbp:focuses_on |
gptkb:physicist
experimental nuclear physics |
| gptkbp:has_property |
zero viscosity
|
| gptkbp:has_role |
stellar evolution
|
| https://www.w3.org/2000/01/rdf-schema#label |
Superfluid Neutrons
|
| gptkbp:influence |
gravitational wave emissions
|
| gptkbp:interacts_with |
magnetic fields
|
| gptkbp:is_characterized_by |
long-range order
non-classical rotational inertia superfluid density |
| gptkbp:is_connected_to |
nuclear matter properties
|
| gptkbp:is_described_as |
gptkb:military_officer
|
| gptkbp:is_essential_for |
understanding cosmic phenomena
understanding neutron star cooling understanding neutron star dynamics |
| gptkbp:is_influenced_by |
external pressures
density and temperature |
| gptkbp:is_involved_in |
energy transport
pulsar glitches |
| gptkbp:is_observed_in |
laboratory experiments
|
| gptkbp:is_related_to |
pairing interactions
Bardeen-Cooper-Schrieffer theory nuclear interactions |
| gptkbp:is_studied_in |
nuclear physics
quantum simulations fundamental physics |
| gptkbp:key |
neutron star interiors
neutron star structure |
| gptkbp:number_of_stages |
gptkb:physicist
|
| gptkbp:occurs_in |
gptkb:physicist
|
| gptkbp:recognizes |
observations of neutron stars
|
| gptkbp:related_concept |
condensed matter physics
extreme astrophysical environments |
| gptkbp:related_model |
effective field theories
|
| gptkbp:resulted_in |
neutron pairing
|
| gptkbp:subject |
high-energy astrophysics
astrophysical research astrophysical modeling |
| gptkbp:was_a_factor_in |
neutron star mergers
|