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I. Inverse Compton origin of pulsar \gamma-ray emission. II. Reconnection model of Crab flares
High Energy Astrophysical Phenomena · Submitted 8 Jul 2013
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim The particles producing Crab flares, and possibly most of the Crab Nebula's high energy emission, are accelerated via reconnection events, and not at shock via Fermi mechanisms.
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The abstract, sentence by sentence
I. There is growing evidence that pulsars' high energy emission is generated via Inverse Compton mechanism. II. The particles producing Crab flares, and possibly most of the Crab Nebula's high energy emission, are accelerated via reconnection events, and not at shock via Fermi mechanisms.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | I. | contribution 0.55 | 0.03 | 0.02 | unclear 1.00 |
| s1 | There is growing evidence that pulsars' high energy emission is generated via Inverse Compton mechanism. II. | background 0.91 | 0.10 | 0.34 | hedged possibility 0.59 |
| s2 | The particles producing Crab flares, and possibly most of the Crab Nebula's high energy emission, are accelerated via reconnection events, and not at shock via Fermi mechanisms. | result 0.75 | 0.32 | 0.47 | asserted 0.85 |
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Original abstract
I. There is growing evidence that pulsars' high energy emission is generated via Inverse Compton mechanism. II. The particles producing Crab flares, and possibly most of the Crab Nebula's high energy emission, are accelerated via reconnection events, and not at shock via Fermi mechanisms.
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