For the compact pulsar XTE J1814-338, the required core inferred from standard outer-matter physics is large and dense, and simple standard-matter core models fail to reproduce it.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Core-Corona Decomposition of Very Compact (Neutron) Stars: Accounting for Current Data of XTE J1814-338
For the compact pulsar XTE J1814-338, the required core inferred from standard outer-matter physics is large and dense, and simple standard-matter core models fail to reproduce it.