Self-consistent treatment of thermal effects in neutron-star postmerger remnants: Observational implications for third-generation gravitational-wave detectors
output:7846a3cb6a1e4b0b91530a5cThis dossier keeps one entity, its published attributes, every direct edge and the supporting source snapshots under a stable URL.
Identity extends only as far as the published stable identifier or explicit mapping. Similar names are not merged. Missing links mean not observed in the bounded sources—not absent in reality.
identity ≠ name similarity · edge ≠ causalityEvery direct connection and its proof
The relation label and evidence class describe the entire claim. Open the source record before drawing a broader conclusion.
edge:project-output:101086251:7846a3cb6a1e4b0b91530a5cNo additional excerpt published.
Open source ↗Fields retained with this identity
Attributes are descriptive source fields. They do not create cross-dataset identity unless an edge states that join explicitly.
- Citation Count
- 0
- Is Open Access
- true
- Open Aire Id
- doi_dedup___::2c6868ca276f1b9f4870fc34a22120b5
- Output Type
- publication
- Persistent Identifiers
- 2310.20378 · 10.1103/physrevd.111.103030 · 10.48550/arxiv.2310.20378
- Publication Date
- 2025-05-14
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