Modelling high-energy pulsar light curves from first principles

By B. Cerutti, A. Philippov, A. Spitkovsky. 2015

150 citations recorded by the source corpus.

Current models of gamma-ray lightcurves in pulsars suffer from large uncertainties on the precise location of particle acceleration and radiation. Here, we present an attempt to alleviate these difficulties by solving for the electromagnetic structure of the oblique magnetosphere, particle acceleration, and the emission of radiation self-consistently, using 3D spherical particle-in-cell simulations. We find that the low-energy radiation is synchro-curvature radiation from the polar-cap regions within the light cylinder. In contrast, the high-energy emission is synchrotron radiation that originates exclusively from the Y-point and the equatorial current sheet where relativistic magnetic reconnection accelerates particles. In most cases, synthetic high-energy lightcurves contain two peaks that form when the current sheet sweeps across the observer's line of sight. We find clear evidence of caustics in the emission pattern from the current sheet. High-obliquity solutions can present up to two additional secondary peaks from energetic particles in the wind region accelerated by the reconnection-induced flow near the current sheet. The high-energy radiative efficiency depends sensitively on the viewing angle, and decreases with increasing pulsar inclination. The high-energy emission is concentrated in the equatorial regions where most of the pulsar spindown is released and dissipated. These results have important implications for the interpretation of gamma-ray pulsar data.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/e0f22e1dec81984274e8bd6609faff9cb51fa399

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In Astronomy and Astrophysics

1. A. Philippov
2. A. Spitkovsky
3. L. Sironi
4. J. Arons
5. D. Giannios
6. A. N. Timokhin
7. M. Petropoulou
8. B. Cerutti

In Nuclear and High Energy Physics

1. A. Philippov
2. A. Spitkovsky
3. L. Sironi
4. J. Arons
5. D. Giannios
6. M. Petropoulou
7. Bing Zhang
8. U. Keshet

Citations in the corpus

• Ab-initio Pulsar Magnetosphere: Particle Acceleration in Oblique Rotators and High-energy Emission Modeling (2017, background): “In agreement with earlier expectations (Cerutti et al. 2016), particle acceleration in current sheets is not limited by synchrotron cooling, since energetic particles are focused deep inside the layer, where losses can be neglected.”