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Sampath A, Davoine X, Corde S, Gremillet L, Gilljohann M, Sangal M, Keitel CH, Ariniello R, Cary J, Ekerfelt H, Emma C, Fiuza F, Fujii H, Hogan M, Joshi C, Knetsch A, Kononenko O, Lee V, Litos M, Marsh K, Nie Z, O'Shea B, Peterson JR, Claveria PSM, Storey D, Wu Y, Xu X, Zhang C, Tamburini M. Extremely Dense Gamma-Ray Pulses in Electron Beam-Multifoil Collisions. PHYSICAL REVIEW LETTERS 2021; 126:064801. [PMID: 33635713 DOI: 10.1103/physrevlett.126.064801] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/25/2020] [Revised: 12/18/2020] [Accepted: 01/08/2021] [Indexed: 06/12/2023]
Abstract
Sources of high-energy photons have important applications in almost all areas of research. However, the photon flux and intensity of existing sources is strongly limited for photon energies above a few hundred keV. Here we show that a high-current ultrarelativistic electron beam interacting with multiple submicrometer-thick conducting foils can undergo strong self-focusing accompanied by efficient emission of gamma-ray synchrotron photons. Physically, self-focusing and high-energy photon emission originate from the beam interaction with the near-field transition radiation accompanying the beam-foil collision. This near field radiation is of amplitude comparable with the beam self-field, and can be strong enough that a single emitted photon can carry away a significant fraction of the emitting electron energy. After beam collision with multiple foils, femtosecond collimated electron and photon beams with number density exceeding that of a solid are obtained. The relative simplicity, unique properties, and high efficiency of this gamma-ray source open up new opportunities for both applied and fundamental research including laserless investigations of strong-field QED processes with a single electron beam.
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Affiliation(s)
- Archana Sampath
- Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg, Germany
| | - Xavier Davoine
- CEA, DAM, DIF, 91297 Arpajon, France
- Université Paris-Saclay, CEA, LMCE, 91680 Bruyères-le-Châtel, France
| | - Sébastien Corde
- LOA, ENSTA Paris, CNRS, Ecole Polytechnique, Institut Polytechnique de Paris, 91762 Palaiseau, France
| | - Laurent Gremillet
- CEA, DAM, DIF, 91297 Arpajon, France
- Université Paris-Saclay, CEA, LMCE, 91680 Bruyères-le-Châtel, France
| | - Max Gilljohann
- LOA, ENSTA Paris, CNRS, Ecole Polytechnique, Institut Polytechnique de Paris, 91762 Palaiseau, France
| | - Maitreyi Sangal
- Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg, Germany
| | - Christoph H Keitel
- Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg, Germany
| | - Robert Ariniello
- University of Colorado Boulder, Department of Physics, Center for Integrated Plasma Studies, Boulder, Colorado 80309, USA
| | - John Cary
- University of Colorado Boulder, Department of Physics, Center for Integrated Plasma Studies, Boulder, Colorado 80309, USA
| | - Henrik Ekerfelt
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - Claudio Emma
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - Frederico Fiuza
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - Hiroki Fujii
- University of California Los Angeles, Los Angeles, California 90095, USA
| | - Mark Hogan
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - Chan Joshi
- University of California Los Angeles, Los Angeles, California 90095, USA
| | - Alexander Knetsch
- LOA, ENSTA Paris, CNRS, Ecole Polytechnique, Institut Polytechnique de Paris, 91762 Palaiseau, France
| | - Olena Kononenko
- LOA, ENSTA Paris, CNRS, Ecole Polytechnique, Institut Polytechnique de Paris, 91762 Palaiseau, France
| | - Valentina Lee
- University of Colorado Boulder, Department of Physics, Center for Integrated Plasma Studies, Boulder, Colorado 80309, USA
| | - Mike Litos
- University of Colorado Boulder, Department of Physics, Center for Integrated Plasma Studies, Boulder, Colorado 80309, USA
| | - Kenneth Marsh
- University of California Los Angeles, Los Angeles, California 90095, USA
| | - Zan Nie
- University of California Los Angeles, Los Angeles, California 90095, USA
| | - Brendan O'Shea
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - J Ryan Peterson
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
- Stanford University, Physics Department, Stanford, California 94305, USA
| | - Pablo San Miguel Claveria
- LOA, ENSTA Paris, CNRS, Ecole Polytechnique, Institut Polytechnique de Paris, 91762 Palaiseau, France
| | - Doug Storey
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - Yipeng Wu
- University of California Los Angeles, Los Angeles, California 90095, USA
| | - Xinlu Xu
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - Chaojie Zhang
- University of California Los Angeles, Los Angeles, California 90095, USA
| | - Matteo Tamburini
- Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg, Germany
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Collimated ultrabright gamma rays from electron wiggling along a petawatt laser-irradiated wire in the QED regime. Proc Natl Acad Sci U S A 2018; 115:9911-9916. [PMID: 30224456 PMCID: PMC6176611 DOI: 10.1073/pnas.1809649115] [Citation(s) in RCA: 25] [Impact Index Per Article: 3.6] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/04/2022] Open
Abstract
Even though bright X-rays below mega-electron volt photon energy can be obtained from X-ray free electron lasers and synchrotron radiation facilities, it remains a great challenge to generate collimated bright gamma-ray beams over 10 mega-electron volts. We propose a scheme to efficiently generate such beams from submicron wires irradiated by petawatt lasers, where electron accelerating and wiggling are achieved simultaneously. With significant quantum electrodynamics effects existing even with petawatt lasers, our full 3D simulations show that directional gamma rays can be generated with thousand-fold higher brilliance and thousand-fold higher photon energy than those from synchrotron radiation facilities. In addition, the photon yield efficiency approaches 10%, 100,000-fold higher than those typical from betatron radiation and Compton scattering based on laser-wakefield accelerators. Even though high-quality X- and gamma rays with photon energy below mega-electron volt (MeV) are available from large-scale X-ray free electron lasers and synchrotron radiation facilities, it remains a great challenge to generate bright gamma rays over 10 MeV. Recently, gamma rays with energies up to the MeV level were observed in Compton scattering experiments based on laser wakefield accelerators, but the yield efficiency was as low as 10−6, owing to low charge of the electron beam. Here, we propose a scheme to efficiently generate gamma rays of hundreds of MeV from submicrometer wires irradiated by petawatt lasers, where electron accelerating and wiggling are achieved simultaneously. The wiggling is caused by the quasistatic electric and magnetic fields induced around the wire surface, and these are so high that even quantum electrodynamics (QED) effects become significant for gamma-ray generation, although the driving lasers are only at the petawatt level. Our full 3D simulations show that directional, ultrabright gamma rays are generated, containing 1012 photons between 5 and 500 MeV within a 10-fs duration. The brilliance, up to 1027 photons s−1 mrad−2 mm−2 per 0.1% bandwidth at an average photon energy of 20 MeV, is second only to X-ray free electron lasers, while the photon energy is 3 orders of magnitude higher than the latter. In addition, the gamma ray yield efficiency approaches 10%—that is, 5 orders of magnitude higher than the Compton scattering based on laser wakefield accelerators. Such high-energy, ultrabright, femtosecond-duration gamma rays may find applications in nuclear photonics, radiotherapy, and laboratory astrophysics.
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