Gamma Rays Without Protons express

Original: "Ultrahigh-Energy Gamma-Ray Sources Need Not Be Hadronic PeVatrons"
arXiv:2603.17012 · 2026-03-17 · CC BY 4.0 · 1 min
Ultra-bright gamma-ray bursts aren't always born from heavyweight particles.

Gamma rays with energies above one hundred trillion electronvolts are like stones thrown with incredible force. For a long time, it was believed that only protons, heavy particles accelerated in cosmic accelerators, could launch such 'stones.' But new work shows that sometimes light electrons are enough.

The authors examined three objects: the microquasar SS 433, the center of our Galaxy, and TeV halos — clouds around pulsars. In all three cases, the observations are explained by simple models where electrons, not protons, produce the gamma rays. The model matched especially well with the size of SS 433: the calculated width of the source coincided with the measured one.

Electrons at such energies behave like runners who trip at every step: it's hard for them to accelerate further. Protons, on the other hand, are like marathon runners who are barely hindered by obstacles.

To pinpoint a proton accelerator, additional clues are needed. For example, a burst of neutrinos — particles that are born only together with protons. Or a coincidence of gamma-ray emission with gas clouds: protons colliding with gas produce a characteristic signal.

Ultra-high-energy gamma rays are like the signature of an invisible artist. Previously, it was thought that only protons could leave this signature. Now it's clear: electrons can sign their names too.

The microquasar SS 433 ejects jets of matter at about a quarter of the speed of light, like a giant hose spraying the cosmos.

Scientists
Arthur ComptonEnrico FermiErnest RutherfordAlbert EinsteinBarry BarishKip Thorne
Concepts
ultra high energy gamma ray ultra high energy cosmic ray source Gamma radiation radio source cosmic accelerator tev neutron star light emission fermi telescope jwst red sources central engine neutrino sources pulsar gigaelectronvolt red galactic nuclei nustar germanium detector synchrotron radiation galactic outflow acceleration lhaaso magnetar