Neutron Stars

GPTKB entity

Statements (54)
Predicate Object
gptkbp:instance_of gptkb:astronomy
gptkbp:are_detected_by observing their radiation
gptkbp:are_part_of gptkb:the_Milky_Way_Galaxy
the life cycle of stars
gptkbp:can extreme temperatures
superconductivity
high rotational speeds
high magnetic fields
neutron superfluidity
accretion disks
rapid rotation
varied compositions
high surface gravity
extreme gravitational effects
neutron star mergers
high energy emissions
neutron star equations of state
neutron star mergers as sources of heavy elements
different types based on rotation and magnetic field
gptkbp:can_be gptkb:magnetars
pulsars
the densest known objects in the universe
gptkbp:can_collapse_into black holes
gptkbp:can_detect radio telescopes
gptkbp:can_have_crust made of atomic nuclei and electrons
gptkbp:can_have_magnetic_field_strength up to 10^11 to 10^15 T
gptkbp:can_have_surface_temperature up to 1 million K
gptkbp:composed_of gptkb:neutrons
gptkbp:emissions_standard gptkb:X-rays
gptkbp:exhibits gptkb:gravitational_waves
time dilation effects
spin-up and spin-down behavior
pulsation periods
various phenomena related to their rotation.
gptkbp:formed supernova explosions
the collapse of a massive star core
gptkbp:has_radius about 10 kilometers
https://www.w3.org/2000/01/rdf-schema#label Neutron Stars
gptkbp:is_associated_with gamma-ray bursts
gptkbp:is_considered_as exotic states of matter
gptkbp:is_considered_to_be a key to understanding the universe's evolution
the remnants of massive stars
gptkbp:is_essential_for understanding nuclear physics
gptkbp:is_found_in binary systems
gptkbp:is_observed_in various wavelengths
gptkbp:is_part_of gptkb:supernova_remnants
gptkbp:is_studied_for their role in cosmic evolution
gptkbp:is_studied_in astrophysics
gravitational lensing
observations of their emissions
gptkbp:mass 1.4 times the mass of the Sun
gptkbp:population_density about 4 x 10^17 kg/m^3
gptkbp:bfsParent gptkb:The_Stars
gptkbp:bfsLayer 5