Since the federal government cuts donations for research, scientific organizations are faced with a budget crisis. This includes astrophysics and cosmology, in which researchers test theories that are of fundamental importance for our understanding of the universe. A good example is the search for dark matter (DM), which is usually to smash protons in particle accelerators in order to find indications of this hard -to -tune. According to a current study that appeared in the physical review, black holes could represent a cheaper, natural alternative.
The study was made by Dr. Andrew Mummery from the Rudolf Peierls Center for theoretical Physics at the University of Oxford. Joseph Silk, Professor of Physics and Astronomy with the Institut D'Astrophysique de Paris, the Department of Physics and Astronomy by William H. Miller III at the Johns Hopkins University, and the Beecroft Institute of Particle Astrophysics and Cosmology at the University of Oxford.
As Mummery and Silk argue, the use of black holes for scientific research could complement one billion -dollar institutions, the construction of which takes decades. The most remarkable is Cern's great Hadron collider, the world's largest and most powerful particle accelerator in the world. In these facilities, protons and other subatomar particles are put together at speeds that approach the speed of light, which creates subtle energy flashes and debris that could reveal previously undiscovered particles.
This includes potential candidate particles for dark matter, which make up around 85% of all Matteruvlerse Universe. In addition, institutions such as the LHC have contributed to promoting the Internet and researching cancer therapy and high-performance computing. How silk explains in a press release from JHU HUB:
“One of the great hopes for particles like the great Hadron collider is that it will create dark matter particles, but we have not yet seen any evidence. For this reason, there are discussions to build a much more powerful version, a super collider in the next generation.
A schematic map that shows a possible location for the future circular patient. Credit: Cern
Kerr black holes that are very common in the universe have an angle impulse, which means that they quickly turn on their axles. In fact, the acceleration of material leads to these black holes to this impulse. Scientists have also found that super massive black holes (SMBHS) in the center of galaxies release enormous amounts of plasma, probably from their accretion panes and relativistic jets that come from their poles.
As you argue in your study, gas flows that come from a black holes can lead to a “gravitational particle accelerator” with mass energy center from ten to hundreds of teraelectronvolts (TEV). For comparison, the LHC can generate energies of up to 13 TEV, while the proposed future circular patient (FCC) – currently reported in the development of CERN – can report 100 TEV. In short, these collision events around SMBHS could achieve the same results as super collider. Said silk:
“If super massive black holes can produce these particles through high-energy proton collisions, then we can get a signal on earth, some really high energy particles that go through our detectors quickly. which is a bit more a jump, but it is possible.
“Some particles from these collisions go down the neck of the black hole and disappear forever. But because of their energy and their momentum, some come out of the ones that are accelerated to unprecedented high energies. Supercollider that we want to build could definitely provide us with additional results.”
The impression of the artist by a rotating Smbre, surrounded by an accretion disc. Credit: ESO/ESA/Hubble/M. Corn knife/n. Beard man
While the distance is certainly a factor, these particle collisions could be examined using observatories that are currently pursuing supernova and other energetic cosmic events such as neutrino events. Examples are the IceCube Neutrino Observatory at the South Pole or the kilometer-new-neutrino telescope (km3net), a neutrino telescope of the next generation, which is located under the Mediterranean. There is also the Global Neutrino Network (GNN), an international organization that enables closer cooperation between Neutrino observatories worldwide.
There were also suggestions to observe the gamma rays of Burfs (GrBS), which come from the center of the milky possibility to prove possible evidence from DM. These examinations could offer a cost -effective means of testing the standard model for cosmology and physics, which could complement inexpensive research with supercolliders.
Further reading: JHU, physical evaluation letters
