Model-independent constraints expose kinetic-luminosity and induced-Compton optical-depth bottlenecks that rule out or severely limit external-shock and light-cylinder reconnection FRB models while favoring magnetospheric scenarios with in-situ acceleration.
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4 Pith papers cite this work. Polarity classification is still indexing.
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Magnetic inclination alignment with timescale proportional to B to the minus two suppresses observed numbers of strong-field neutron stars, unifying pulsars and magnetars under one log-uniform initial B distribution.
TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible via time-dependent opening angles.
Numerical and analytical modeling of polar-cap processes in magnetic white dwarfs finds pair creation viable only for P ≲ 100 s and B_d ≲ 10^10 G, rendering it difficult to sustain in observed objects.
citing papers explorer
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The kinetic-energy bottleneck in Fast Radio Burst models
Model-independent constraints expose kinetic-luminosity and induced-Compton optical-depth bottlenecks that rule out or severely limit external-shock and light-cylinder reconnection FRB models while favoring magnetospheric scenarios with in-situ acceleration.
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A Log-Uniform Initial Magnetic Field Distribution Explains Pulsar and Magnetar Populations through Magnetic Inclination Alignment
Magnetic inclination alignment with timescale proportional to B to the minus two suppresses observed numbers of strong-field neutron stars, unifying pulsars and magnetars under one log-uniform initial B distribution.
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Constraining the Pulsar Beaming Fraction with TeV-Selected Galactic Pulsar Wind Nebulae and unidentified TeV Sources
TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible via time-dependent opening angles.
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Study for curvature radiation and magnetic pair creation process on polar-cap region of magnetic white dwarf
Numerical and analytical modeling of polar-cap processes in magnetic white dwarfs finds pair creation viable only for P ≲ 100 s and B_d ≲ 10^10 G, rendering it difficult to sustain in observed objects.