Unveiling the Physics of High-Density Relativistic Pair Plasma Jets in the Laboratory
Lead Research Organisation:
University of Oxford
Department Name: Oxford Physics
Abstract
Gamma-ray bursts (GRBs) are among the most energetic events in the Universe. They occur at cosmological distances and are the result of the collapse of massive stars or neutron stars mergers, with emission of relativistic 'fireballs' of electron-positron pairs. From astrophysical observations, a wealth of information has been gleaned about the mechanism that leads to such strong emission of radiation, with leading models predicting that this is due to the disruption of the beam as it blasts through the surrounding plasma. This produces shocks and hydromagnetic turbulence that generate synchrotron emission, potentially accelerating to ultra-high energies the protons which are observed
on Earth as cosmic rays. However, there is no direct evidence of the generation of either magnetic fields or cosmic rays by GRBs. Estimates are often based on crude energy equipartition arguments or idealized numerical simulations that struggle to capture the extreme plasma conditions. We propose to address this lacuna by conducting laboratory experiments at CERN to mimic the jet propagation through its surrounding plasma. Such experiments will enable in situ measurement of the plasma properties, with exquisite details that cannot be achieved elsewhere. The experiments also complement numerical simulations by providing long measurement times extending into the non-linear regime where numerical simulations are not possible today. The proposed experiments will study fundamental physics processes, unveil the microphysics of GRBs, and address the following, yet answered, key questions:
1) What mechanisms drive the energetic beams unstable and their long-term evolution?
2) What is the role of turbulence in the acceleration of particles to the highest energies?
3) What is the interplay between magnetic fields and particles and how does this affect the observed
electromagnetic emission?
We will provide a new window in high energy astrophysics using novel Earth-based laboratory experiments.
on Earth as cosmic rays. However, there is no direct evidence of the generation of either magnetic fields or cosmic rays by GRBs. Estimates are often based on crude energy equipartition arguments or idealized numerical simulations that struggle to capture the extreme plasma conditions. We propose to address this lacuna by conducting laboratory experiments at CERN to mimic the jet propagation through its surrounding plasma. Such experiments will enable in situ measurement of the plasma properties, with exquisite details that cannot be achieved elsewhere. The experiments also complement numerical simulations by providing long measurement times extending into the non-linear regime where numerical simulations are not possible today. The proposed experiments will study fundamental physics processes, unveil the microphysics of GRBs, and address the following, yet answered, key questions:
1) What mechanisms drive the energetic beams unstable and their long-term evolution?
2) What is the role of turbulence in the acceleration of particles to the highest energies?
3) What is the interplay between magnetic fields and particles and how does this affect the observed
electromagnetic emission?
We will provide a new window in high energy astrophysics using novel Earth-based laboratory experiments.
Organisations
People |
ORCID iD |
| Gianluca Gregori (Principal Investigator) |