Search for very high energy gamma radiation from the radio bright region DR4 of the SNR G78.2+2.1

Data from the HEGRA air shower array are used to set an upper limit on the emission of gamma-radiation above 25 (18) TeV from the direction of the radio bright region DR4 within the SNR G78.2 + 2.1 of 2.5 (7.1). 10^-13 cm^-2 sec^-1. The shock front of SNR G78.2 + 2.1 probably recently overtook the molecular cloud Gong 8 which then acts as a target for the cosmic rays produced within the SNR, thus leading to the expectation of enhanced gamma-radiation. Using a model of Drury, Aharonian and Völk which assumes that SNRs are the sources of galactic cosmic rays via first order Fermi acceleration, we calculated a theoretical prediction for the gamma-ray flux from the DR4 region and compared it with our experimental flux limit. Our 'best estimate' value for the predicted flux lies a factor of about 18 above the upper limit for gamma-ray energies above 25 TeV. Possible reasons for this discrepancy are discussed.

Análisis de la reglamentación europea, promulgada a raíz de los accidentes nucleares, y la determinación de la emisión gamma en alimentos importados

Novel scientific and technological progress require to seek new sources of electricity. Such response is, inter alia, nuclear energy. Nuclear power stations currently produce around a third of the electricity and 14% of the energy consumed in the European Union. A thorough aspect in the use and development of nuclear energy as power source is safety. Nuclear facilities are designed so that the probability of an accident that may affect people and environment was very low. Reasonably, preventive emergency plans take place in the own nuclear facilities in order to mitigate and minimize the consequences, and otherwise another emergency nuclear plans take place outside facilities. Monitoring programs are also conducted in the nearby nuclear facilities, according to the Recommendation reached on 8th June 2000 by the European Commission on the application of Article 36 of the Euratom Treaty for the checking of the levels of radioactivity in the environment, in order to assess the exposure to the whole population. The main objectives of these plans are to check the presence and evolution of radioactive elements and the radiation levels in the environment; to determinate the causes of its increase, if succeed; to estimate the radiological risk to the population; to set corrected measures, if necessary; to ensure legal compliance on the premises and; to verify the suitability of effluent monitoring program to detect radionuclides leaks and transfer to the environment...

Search for VHE gamma-ray emission from Geminga pulsar and nebula with the MAGIC telescopes

The Geminga pulsar, one of the brighest gamma-ray sources, is a promising candidate for emission of very-high-energy (VHE > 100 GeV) pulsed gamma rays. Also, detection of a large nebula have been claimed by water Cherenkov instruments. We performed deep observations of Geminga with the MAGIC telescopes, yielding 63 hours of good-quality data, and searched for emission from the pulsar and pulsar wind nebula. We did not find any significant detection, and derived 95% confidence level upper limits. The resulting upper limits of 5.3 × 10^(−13) TeV cm^(−2)s^(−1) for the Geminga pulsar and 3.5 × 10^(−12) TeV cm^(−2)s^(−1) for the surrounding nebula at 50 GeV are the most constraining ones obtained so far at VHE. To complement the VHE observations, we also analyzed 5 years of Fermi-LAT data from Geminga, finding that the sub-exponential cut-off is preferred over the exponential cut-off that has been typically used in the literature. We also find that, above 10 GeV, the gamma-ray spectra from Geminga can be described with a power law with index softer than 5. The extrapolation of the power-law Fermi-LAT pulsed spectra to VHE goes well below the MAGIC upper limits, indicating that the detection of pulsed emission from Geminga with the current generation of Cherenkov telescopes is very difficult.