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Gravitational Waves from Neutron Stars: Detection Prospects and Inferences for Two Distinct Types of Remnants
output:1bc7e17b38314c95420f4b5eThis 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:101086251:1bc7e17b38314c95420f4b5eRelationshiphas an observed research output
→ProjectNewFunFiCO · Fundamental Fields and Compact Objects: new opportunities
CORDIS project code
No 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_________::8a14c12e711cb316ea507c1a21ea9242
- Output Type
- publication
- Persistent Identifiers
- 10.5506/aphyspolb.56.5-a1
- Publication Date
- 2025-04-22
Inspect the source snapshots
A source snapshot describes what was available at collection time. Corrections and later publications can change future observations.
german-ai-research-to-transfer-indexdoi_________::8a14c12e711cb316ea507c1a21ea9242 · openaire_research_product_id
↗Open original sourcegerman-ai-research-to-transfer-index101086251:output:1bc7e17b38314c95420f4b5e · cordis_project_code
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