Scheme of the electrical equipment of the car VAZ 2106, 21061, 21063, 21065 (1988-2001). Free Technical Library article

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Scheme of the electrical equipment of the car VAZ 2106, 21061, 21063, 21065 (1988-2001)

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Encyclopedia of radio electronics and electrical engineering / Automobile. Electronic devices

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Wiring diagram VAZ 2106, 21061, 21063, 21065 1988-2001

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Publication: cxem.net

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Search for axions by a dark matter hurricane 24.11.2018

A team of scientists from King's College London, the British Astronomical Institute and the University of Zaragoza, Spain, have found that the dark matter 'hurricane' that's passing through our solar system right now provides a great chance to detect axions. We remind our readers that axions are elementary particles that are one of the candidates for the title of dark matter particles, and their detection and study will allow scientists to understand the phenomenon of dark matter and related phenomena.

Modern science already has a number of fairly reliable indirect evidence of the existence of dark matter, despite the lack of the ability to see and "feel" it live. And it is quite natural that scientists continue to look for new ways and technologies that will allow them to touch the "dark secret".

Specialists have focused on the S1 stellar stream, consisting of approximately 30 stars, which moves along a trajectory that indicates that the stars of this stream were once part of a dwarf galaxy swallowed by the Milky Way. The S1 stream was discovered just last year by a team of astronomers studying data collected by the Gaia space telescope. Note that S1 is not the first stellar stream known to scientists, but it is the first and only one whose trajectory of motion intersects with the space of the solar system.

According to the assumptions of scientists, the flow S1 is kept in the form of a single cosmic object by the forces of gravity of the dark matter contained in it. And now this mass of dark matter is moving through the solar system, moving at a speed of about 500 kilometers per second, which, in turn, gives scientists a unique chance to detect and study dark matter particles.

Now scientists have already created a number of mathematical models that demonstrate the distribution of mass and density of moving dark matter. The data obtained during the calculations of these models can serve as a hint for other scientists, according to these data, it is possible to identify areas in which the chance of detecting dark matter increases several times. In addition, the calculation data of the models contains information about what exactly and how it will be necessary to search.

According to the results of calculations, the chance of detecting WIMP particles, which are also candidates for the title of dark matter particles, is extremely small. But the chance of detecting axins in this case is much higher than under normal conditions. This is due to the fact that in the dark matter stream moving together with the stellar stream S1, there may be axions with a wide range of values of their mass and energy.

Unfortunately, the recording scientific equipment available today is not capable of registering axions, despite the wide energy spectrum of their flux. But the S1 stellar stream will cross the space of the solar system for a very long time, and it is likely that until this is over, scientists will have time to develop and use next-generation particle detection systems with the necessary level of their sensitivity.

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