Antiparticles account for a small fraction of cosmic rays and are known to be produced in interactions between cosmic-ray nuclei and atoms in the interstellar medium(1), which is referred to as a 'secondary source'. Positrons might also originate in objects such as pulsars(2) and microquasars(3) or through dark matter annihilation(4), which would be 'primary sources'. Previous statistically limited measurements(5-7) of the ratio of positron and electron fluxes have been interpreted as evidence for a primary source for the positrons, as has an increase in the total electron+positron flux at energies between 300 and 600 GeV (ref. 8). Here we report a measurement of the positron fraction in the energy range 1.5-100 GeV. We find that the positron fraction increases sharply overmuch of that range, in a way that appears to be completely inconsistent with secondary sources. We therefore conclude that a primary source, be it an astrophysical object or dark matter annihilation, is necessary.
|Titolo:||An anomalous positron abundance in cosmic rays with energies 1.5-100 GeV|
|Data di pubblicazione:||2009|
|Citazione:||An anomalous positron abundance in cosmic rays with energies 1.5-100 GeV / Vacchi, Andrea. - In: NATURE. - ISSN 0028-0836. - 458:7238(2009), pp. 607-609.|
|Appare nelle tipologie:||1.1 Articolo in rivista|