  ATHENA, with a launch foreseen in 2028 towards the L2 orbit, addresses the
science theme "The Hot and Energetic Universe", coupling a high-performance
X-ray Telescope with two complementary focal-plane instruments. One of these,
the X-ray Integral Field Unit (X-IFU) is a TES based kilo-pixel array providing
spatially resolved high-resolution spectroscopy (2.5 eV at 6 keV) over a 5
arcmin FoV. The background for this kind of detectors accounts for several
components: the diffuse Cosmic X-ray Background, the low energy particles
(<~100 keV) focalized by the mirrors and reaching the detector from inside the
field of view, and the high energy particles (>~100 MeV) crossing the
spacecraft and reaching the focal plane from every direction. Each one of these
components is under study to reduce their impact on the instrumental
performances. This task is particularly challenging, given the lack of data on
the background of X-ray detectors in L2, the uncertainties on the particle
environment to be expected in such orbit, and the reliability of the models
used in the Monte Carlo background computations. As a consequence, the
activities addressed by the group range from the reanalysis of the data of
previous missions like XMM-Newton, to the characterization of the L2
environment by data analysis of the particle monitors onboard of satellites
present in the Earth magnetotail, to the characterization of solar events and
their occurrence, and to the validation of the physical models involved in the
Monte Carlo simulations. All these activities will allow to develop a set of
reliable simulations to predict, analyze and find effective solutions to reduce
the particle background experienced by the X-IFU, ultimately satisfying the
scientific requirement that enables the science of ATHENA. While the activities
are still ongoing, we present here some preliminary results already obtained by
the group.
