GISAP: Biology, Veterinary Medicine and Agricultural Sciences

4-5

Authors: Samaya Aliyeva

Matters of composing the geoinformation maps in order to promote innovations in the tourism sector of the economy on the studied territory are described in the report.

9-12

Authors: Oleksandr Makarenko

A new phenomenon was discovered - excessive heating of the depths of the large Solar system bodies by their internal energy source of cosmic origin, modulated by the position and direction of the Solar system motion in the Galaxy. This lets us assume the presence of a heat-generating factor in the galactic space. Influence of this factor results in the energy emission in interiors of the cosmic bodies. The dark matter particles may be the probable candidate for such a heat-generating factor. The influence of gravitational factors is also possible.

16-17

Authors: Nagima Akhmetova, Olesya Muzyka

The report is devoted to improvement of the cadastral cost determination technique in relation to agricultural lands in Kazakhstan.

21-22

Authors: Alpasha Nabiyev, Nazim Jafarov, Yahya Gadirov

The authors consider the creation of geoinformation maps of river basins and the database on water resources of Azerbaijan in order to improve water management. Versions of geoinformation cartographic models of river basins and administrative regions of Azerbaijan are compiled with the help of the geographic information system MAPINFO5.

26-30

Authors: Anton Khlopkov, Ilakha Agaeva, Yuriy Khlopkov, Zay Yar Myo Myint

The Higgson (Higgs Boson), a peculiar catalyst of formation of mass of the Universe after the Big Bang, was theoretically predicted by the English physicist Peter Higgs in 1964. July 4, 2012 experiments on the Large Hadron Collider have revealed a mysterious particle with a mass of 125 GeV/s? which appeared to be the Higgs Boson. What are the future ways of development of physics, as well as our Universe? Authors of this report consider several scenarios of this development. According to the Big Bang theory, evolution of the Universe depends on the experimentally measurable parameter – the average density of matter in the modern Universe. There are two evolution scenarios. If the density does not exceed a certain (theoretically known) critical value, the Universe will eternally expand forever. If the density becomes higher than critical, the process of expansion will eventually stop launching the reverse phase of compression returning the Universe to the initial singular state. Modern experimental data concerning the average density value are still insufficiently reliable to make an unambiguous choice between two options of the future of the Universe.