Child sexual abuse has been a focus of concern for feminist writers for over a decade, and social work and probation practitioners are spending an increasing amount of time undertaking intervention with men who sexually abuse children. This paper uses a review of feminist literature which identifies three contested areas in the feminist discussion: theory, power and the fixity of gender, and discusses whether these debates are reflected in any way in the interventions being undertaken with men who sexually abuse children. The conclusion reached is of a distance between theory which draws on a radical patriarchal analysis of child sexual abuse and the practice of those who attempt to work with the perpetrators of such abuse. Although some workers frame their intervention in terms of a patriarchal understanding of society and of the nature of power within this – to this extent following a radical feminist approach – there is a sense in which practitioners’ use of feminist theory is only partial. Thus feminist theory is often presented as unitary and there is a sense in which practitioners who say they are espousing feminism are not in touch with the subtleties of feminist analysis revealed in the literature review. In addition, the logic of the radical feminist perspective is not followed through in practice as there is evidence of a sensitivity to difference which may be aligning practitioners with a post‐modern/post‐structural interpretation of men’s sexual violence towards children.
The KM3NeT Collaboration is constructing a km 3 -volume neutrino telescope in the Mediterranean sea, called ARCA (Astroparticle Research with Cosmics in the Abyss), that will achieve an unprecedented sensitivity to high-energy cosmic neutrinos. This telescope will be able to reconstruct the arrival direction of the neutrinos with a precision of 0.1 • . The configuration of ARCA makes it sensitive to neutrinos in a wide energy range, from sub-TeV up to tens of PeV. Moreover, this detector has a large field of view and a very high duty cycle, allowing for full-sky (and all-flavours) searches. All these features make ARCA an excellent instrument to study transient neutrino sources. Atmospheric muons and neutrinos, produced by primary cosmic rays, constitute the main background for ARCA. This background can be several orders of magnitude higher than the expected cosmic neutrino flux. In this work, we introduce an event selection which reduces the background up to a negligible level inside the region of interest and within the search time window. The ARCA performance to detect a transient neutrino flux, including the effective area, sensitivity and discovery potential, are provided for a given test source, and for different time windows.
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