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gptkbp:instance_of
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gptkb:astronomy
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gptkbp:applies_to
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gptkb:white_dwarf_stars
gptkb:white_dwarfs
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gptkbp:can_lead_to
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supernova explosions
supernova or neutron star formation
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gptkbp:concept
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theoretical astrophysics
stellar astrophysics
experimentally validated
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gptkbp:defines
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maximum mass of a stable white dwarf star
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gptkbp:describes
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maximum mass of a stable white dwarf star
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gptkbp:developed_by
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gptkb:Quantum_Mechanics
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https://www.w3.org/2000/01/rdf-schema#label
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Chandrasekhar limit
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gptkbp:is_a_concept_that_has_historical_significance_in
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the study of stellar evolution.
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gptkbp:is_a_critical_concept_in
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stellar dynamics
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gptkbp:is_a_critical_value_for
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stellar collapse
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gptkbp:is_a_factor_in_determining
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the end states of stars
|
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gptkbp:is_a_framework_for
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understanding stellar collapse mechanisms
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gptkbp:is_a_fundamental_limit_for
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degenerate matter
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gptkbp:is_a_limit_that_affects
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the evolution of binary star systems
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gptkbp:is_a_limit_that_can_lead_to
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black hole formation
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gptkbp:is_a_limit_that_influences
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the formation of neutron stars
|
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gptkbp:is_a_limit_that_is_often_referenced_in
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astrophysical models
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gptkbp:is_a_subject_of
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theoretical astrophysics
|
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gptkbp:is_a_theoretical_limit_for
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stellar remnants
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gptkbp:is_a_threshold_for
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neutron star formation
core collapse
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gptkbp:is_analyzed_in
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compact objects
fate of massive stars
|
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gptkbp:is_approximately
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1.4 solar masses
|
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gptkbp:is_associated_with
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gptkb:Type_Ia_supernovae
|
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gptkbp:is_described_as
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the lifecycle of stars
the fate of stars
|
|
gptkbp:is_discussed_in
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astrophysical literature
|
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gptkbp:is_essential_for
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stellar evolution
understanding stellar evolution
|
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gptkbp:is_exceeded_by
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massive stars
|
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gptkbp:is_influenced_by
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gravitational wave astronomy
temperature and pressure conditions
|
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gptkbp:is_related_to
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electron degeneracy pressure
mass-radius relationship of white dwarfs
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gptkbp:is_significant_for
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gptkb:cosmology
|
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gptkbp:is_studied_in
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modern astrophysics
|
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gptkbp:is_used_in_calculations_of
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stellar mass distributions
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gptkbp:key_concept
|
astrophysics
|
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gptkbp:named_after
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gptkb:Subrahmanyan_Chandrasekhar
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gptkbp:performance
|
stellar mass measurements
|
|
gptkbp:proposed_by
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gptkb:Subrahmanyan_Chandrasekhar
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gptkbp:related_to
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gptkb:white_dwarf_stars
|
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gptkbp:values
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approximately 1.4 solar masses
|
|
gptkbp:was_a_factor_in
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stellar nucleosynthesis
supernova explosions
the stability of white dwarfs
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gptkbp:was_a_result_of
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Pauli exclusion principle
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gptkbp:bfsParent
|
gptkb:S._Chandrasekhar
gptkb:White_Dwarfs
gptkb:Subrahmanyan_Chandrasekhar
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gptkbp:bfsLayer
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5
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