Page 7 - UNAM Forum ED2-2021
P. 7

Front-row view reveals




             exceptional cosmic explosion




                Observation challenges established theory


                                of gamma-ray bursts in the universe































          front row when this gamma-ray  co-author       Edna    Ruiz-Velasco  by separate mechanisms: the
          burst happened,” explains co-     from the Max Planck Institute for  X-ray    component      originates
          author Andrew Taylor from DESY.  Nuclear Physics in Heidelberg. “This   from ultra-fast electrons that are
          The team caught the explosion’s  is what’s so exceptional about this  deflected in the strong magnetic
          afterglow  immediately  when it  gamma-ray burst – it happened in  fields of the burst’s surroundings.
          became visible to the H.E.S.S.  our cosmic backyard where the  This “synchrotron” process is quite
          telescopes. “We could observe  very-high-energy photons were  similar to how particle accelerators
          the afterglow for several days and  not  absorbed in collisions with  on Earth produce bright X-rays for
          to unprecedented gamma-ray  background light on their way to  scientific investigations.
          energies,” reports Taylor.        Earth, as it happens over larger
                                            distances in the cosmos.”          However, according to existing
          The comparatively short distance                                     theories, it seemed very unlikely
          to this gamma-ray burst allowed  The    team    could   follow  the  that even the most powerful
          detailed measurements of the      afterglow up to three days  explosions in the universe could
          afterglow’s spectrum, which is the  after the initial explosion. The  accelerate electrons enough to
          distribution of “colours” or photon  result came as a surprise: “Our  directly produce the observed
          energies of the radiation, in the  observations  revealed   curious  very-high-energy gamma rays. This
          very-high-energy   range.   “We   similarities between the X-ray and  is due to a “burn-off limit”,  which
          could determine GRB 190829A’s  very-high-energy         gamma-ray    is determined by the balance            Image of gamma-ray burst taken by HESS (Credit HESS)
          spectrum up to an energy of 3.3   emission of the burst’s afterglow,”  of acceleration and cooling of
          tera-electronvolts, that’s about  reports Zhu. Established theories  particles within  an accelerator.
          a trillion times as energetic as the  assume that the two emission  Producing         very-high-energy
          photons of visible light,” explains  components must be produced     gamma rays requires electrons

           7   Official Newsletter                                                            ...continued on pg 8
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