Bauman Moscow State Technical University,
Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences,
Laboratoire de Physique Nucléaire et de Hautes Energies ( LPNHE - UPMC / IN2P3 / CNRS),
University of Lethbridge, University of British Columbia-Okanagan,
Guidelines for Submission
Manuscripts can be submitted until the expiry of the deadline. Submissions must be previously unpublished and may not be under consideration elsewhere.
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The detection of new particles and their role within modern high-energy-Physics theories as well as their gravitational interactions has been one of the furthest challenges of the last decades in Theoretical Physics. The detection of new phenomena as well as their experimental prediction is therefore looked after within Theoretical Physics, thought experiments and application of the available experimental techniques. The search for the appropriate phenomenological description has to be forecast within the chosen energy scales involved and distances considered. The quantum description has to be regarded to as a possible definition of the structures describing quantum spacetime and its matter content. At the semi-classical level, the corrections for the known phenomena have to be pondered within the appropriate classical limit by keeping examining the quantum version. At large scale distances, the possibility of observation of new Physical phenomena has to be proposed within the framework of planetology by enquiring the opportune Galactical framework and the extragalactical ones, which, on their turn, have not found a complete description yet. The choice of the proper experimental apparati, the design of the thought experiments and of the thought experimental settings and the analysis of the gathered data can support the chosen models under investigation.