Contribution of Pulsars to the Gamma-Ray Background and their Observation with the Space Telescopes GLAST and AGILE

Luminosities and fluxes of the expected population of galactic gamma-ray pulsars become foreseeable if physical distributions at birth and evolutive history are assigned. In this work we estimate the contribution of pulsar fluxes to the gamma-ray background, which has been measured by the EGRET experiment on board of the CGRO. For pulsar luminosities we select some of the most important gamma-ray emission models, taking into account both polar cap and outer gap scenarios. We find that this contribution strongly depends upon controversial neutron star birth properties. A comparison between our simulation results and EGRET data is presented for each model, finding an average contribution of about 10%. In addition, we perform the calculation of the number of new gamma-ray pulsars detectable by GLAST and AGILE, showing a remarkable difference between the two classes of models. Finally, we suggest some improvements in the numerical code, including more sophisticated galactic m odels and different populations of pulsars like binaries, milliseconds, anomalous pulsars and magnetars.