arXiv (All)
open access
A Finite-History Interpretation of the AMS-02 Positron Spectrum
I examine whether the separation between the characteristic energy scales of cosmic-ray electrons and positrons can be understood as a finite-history effect, without introducing a separate dominant source specifically to generate the high-energy positron feature. In this description the positron ret
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Interpreting the 95 GeV di-photon and di-tau Excesses in the Georgi-Machacek Model#635651
- Interpreting the 95 GeV di-photon and di-tau Excesses in the Georgi-Machacek Model#633302
- Runaway avalanches in plasmas with external electric fields: spatially inhomogeneous case in a perturbation framework#1143760
- The Cosmic Deflector#46494
- Information Relational Manifestation Theory (IRMT): A First-Principles Derivation of the Koide Formula#82647
Record · ID 1052145
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive