EpiStack

Home

❯

EpiStack v1 — FLF competition

❯

analyses

❯

black holes

❯

hypotheses

❯

H 13 General relativity correctly describes gravity and gravitational radiation even in the strong field regime of a 2 solar mass neutron star

H-13 - General relativity correctly describes gravity and gravitational radiation even in the strong-field regime of a 2-solar-mass neutron star

Properties8
type
hypothesis
id
H-13
state
active
question
Does general relativity remain valid in previously untested strong-field gravity regimes?
statement
General relativity remains an accurate description of gravity - with no significant dipolar gravitational radiation or strong-field scalarization phenomena from long-range extra fields - even at the extreme gravitational binding energies of a ~2-Msun neutron star; short-range deviations (extra fields with mass heavier than ~1e-19 eV/c^2) are not excluded by this system.
cluster
HC-13 - Validity of general relativity in the strong-field regime
source
S-80 - Antoniadis et al. 2013, A Massive Pulsar in a Compact Relativistic Binary
locator
abstract; Discussion §'PSR J0348+0432 as a testbed for gravity'; Fig. 4

Graph View

Show model graphinteractive Bayesian view — separate from the graph above
added after the FLF submission deadline

Backlinks

  • A-22 - Orbital-decay agreement with GR excludes dipolar radiation and significant strong-field deviations for 2-solar-mass neutron stars
  • HC-13 - Validity of general relativity in the strong-field regime
  • S-80 - Antoniadis et al. 2013, A Massive Pulsar in a Compact Relativistic Binary

Created with Quartz v4.5.2 © 2026

  • GitHub
  • FLF competition
  • Built with Quartz