13:05  
   08.09.2016  
  
  Source: 
   Herald
  
  
   
An international team of astronomers from the University of Cambridge, which included two Russian researchers, found and successfully tested an elegant method of observation of dark matter, which is able to shed light on the structure of this mysterious substance.
 Their paper  accepted for publication in the journal MNRAS. The  theory predicts that in addition to large clusters  of dark matter in the universe must be present and  smaller pieces, so-called sub-halo with a mass of  “only” in the thousands or millions of  solar masses. To see the traces of the passage of  these clusters, astronomers were able to, noting  gaps in the tidal tail, remaining from the  destruction of globular cluster in our galaxy.
  
 They were able to estimate the mass flown  clots and therefore impose limits on the mass of  dark matter particles themselves. “One way  to understand the nature of dark matter is to  determine the minimum size of the structures which  it forms. Until now, the smallest size were  considered to hundreds of millions of solar masses  (in dwarf galaxies) – said  “Gazeta.ru” co-author Sergei Koposov  opening of the University of Cambridge. –  With the help of stellar streams we can see  bunches weighing just millions of solar masses.  ”
  
 Based on the observations, scientists have  deduced a lower limit on the mass of dark matter  particles – 18 keV. “Times”
  
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