Cosmic rays and the Monogem supernova remnant

Recent findings indicate that the Monogem Ring and the associated pulsar PSR B0656 + 14 may be the `Single Sourceʹ responsible for the formation of the sharp knee in the cosmic ray energy spectrum at ∼3 PeV. The energy spectrum of cosmic rays expected for the Monogem Ring supernova remnant (SNR) from our SNR acceleration model [J. Phys. G: Nucl. Part. Phys. 27 (2001) 941] has been published by us elsewhere [J. Phys. G: Nucl. Part. Phys. 29 (2003) 709] . In this paper we go on to estimate the contribution of the pulsar B0656 + 14 to the cosmic rays in the PeV region. We conclude that although the pulsar can contribute to the formation of the knee, it cannot be the dominant source of it and an SNR is still needed. o examine the possibility of the pulsar giving the peak of the extensive air shower (EAS) intensity observed from the region inside the Monogem Ring [ApJ Lett. 597 (2003) L129]. The estimates of the gamma-ray flux produced by cosmic ray particles from this pulsar indicate that it can be the source of the observed peak, if the particles were confined within the SNR during a considerable fraction of its total age. The flux of gamma quanta at PeV energies has a high sensitivity to the duration of the confinement. The estimates of this time and of the following diffusion of cosmic rays from the confinement volume turn out to be in remarkable agreement with the time needed for these cosmic rays to propagate to the solar system and to form the observed knee in the cosmic ray energy spectrum. possible mechanisms for the production of particles which could give rise to the observed narrow peak in the EAS intensity were also examined. Electrons scattered on the microwave background or on X-rays, emitted by SNR, cannot be responsible for the gamma-quanta in the peak. Neutrons produced in PP-collisions or released from the disintegration of accelerated nuclei seem to be also unable to create the peak since they cannot give the observed flux. experimental EAS results concerning a point-like source are confirmed, they can be important, since(i) ill give evidence for the acceleration of protons or heavier nuclei by the pulsar; ill give evidence for the existence of a confinement mechanism in SNR; ill confirm that cosmic rays produced by the Monogem Ring SNR and associated pulsar B0656 + 14 were released recently giving rise to the formation of the sharp knee and the observed narrow peak in the EAS intensity; ill give strong support for the Monogem Ring SNR and the associated pulsar B0656 + 14 being identified as the Single Source proposed in our Single Source Model of the knee. er of predictions of the examined mechanism are made.