Unveiling the Physics of High-Density Relativistic Pair Plasma Jets in the Laboratory
Unveiling the Physics of High-Density Relativistic Pair Plasma Jets in the Laboratory
批准号:
EP/Y035038/1
负责人:
Gianluca Gregori
金额:
$269.73万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2024
资助国家:
英国
项目状态:
未结题
起止时间:
2024 至 --
中文摘要
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英文摘要
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 observedon 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 observedelectromagnetic emission?We will provide a new window in high energy astrophysics using novel Earth-based laboratory experiments.
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依托单位:
国内基金
海外基金
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