Now Reading: ‘Aquila Booster’ challenges theoretical limits of particle acceleration in pulsar wind nebulae
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‘Aquila Booster’ challenges theoretical limits of particle acceleration in pulsar wind nebulae
‘Aquila Booster’ challenges theoretical limits of particle acceleration in pulsar wind nebulae
The Large High Altitude Air Shower Observatory (LHAASO) has detected PeV (1015 eV) gamma-ray emission from a pulsar wind nebula powered by PSR J1849-0001 in the constellation Aquila, marking the discovery of a new PeVatron and posing a challenge to the classical theory of particle acceleration in pulsar wind nebulae.
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