Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth
University of Utah · Los Alamos National Laboratory · +25 more institutions
Abstract
The unexpectedly high flux of cosmic-ray positrons detected at Earth may originate from nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary production. We report the detection, using the High-Altitude Water Cherenkov Observatory (HAWC), of extended tera-electron volt gamma-ray emission coincident with the locations of two nearby middle-aged pulsars (Geminga and PSR B0656+14). The HAWC observations demonstrate that these pulsars are indeed local sources of accelerated leptons, but the measured tera-electron volt emission profile constrains the diffusion of particles away from these sources to be much slower than previously assumed. We demonstrate that the leptons emitted by…
Citation impact
- FWCI
- 69.92
- Percentile
- 100%
- References
- 58
Authors
116Topics & keywords
- Physics
- Cosmic ray
- Cherenkov radiation
- Gamma ray
- Observatory
- Astrophysics
- Pulsar
- Positron
Funding
- NSNational Science FoundationAward: 89233218CNA000001
- UDU.S. Department of EnergyAward: 89233218CNA000001
- CNConsejo Nacional de Ciencia y TecnologíaAwards: 260378, 232656, 281653, 243290, IA102715, 132197, 258865, 271051, 254964, 239762, 271737, 179588
- UNUniversidad Nacional Autónoma de MéxicoAwards: IA102917, IN111716
- BUBenemérita Universidad Autónoma de Puebla
- NNNational Nuclear Security AdministrationAward: 89233218CNA000001
- DGDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoAwards: IA102917, IN111716-3, 109916, IN111315, IA102715, IG100317
- CDCoordinación de la Investigación CientíficaAwards: IA102715, 254964
- LALos Alamos National LaboratoryAward: 89233218CNA000001