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| Format: | Preprint |
| Published: |
2024
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2410.06537 |
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| _version_ | 1866909438802132992 |
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| author | Pirozhkov, A. S. Sagisaka, A. Ogura, K. Vishnyakov, E. A. Shatokhin, A. N. Armstrong, C. D. Esirkepov, T. Zh. Izquierdo, B. Gonzalez Pikuz, T. A. Hadjisolomou, P. Alkhimova, M. A. Arran, C. Tsygvintsev, I. P. Valenta, P. Pikuz, S. A. Yan, W. Jeong, T. M. Singh, S. Finke, O. Grittani, G. Nevrkla, M. Lazzarini, C. Velyhan, A. Hayakawa, T. Fukuda, Y. Koga, J. K. Ishino, M. Kondo, Ko. Miyasaka, Y. Kon, A. Nishikino, M. Nosach, Y. V. Khikhlukha, D. Kolesnikov, A. O. Ragozin, E. N. Gasilov, V. A. Kumar, D. Nejdl, J. Sasorov, P. V. Weber, S. Margarone, D. Kato, Y. Korn, G. Kiriyama, H. Kondo, K. Ridgers, C. Kawachi, T. Kando, M. Bulanov, S. V. |
| author_facet | Pirozhkov, A. S. Sagisaka, A. Ogura, K. Vishnyakov, E. A. Shatokhin, A. N. Armstrong, C. D. Esirkepov, T. Zh. Izquierdo, B. Gonzalez Pikuz, T. A. Hadjisolomou, P. Alkhimova, M. A. Arran, C. Tsygvintsev, I. P. Valenta, P. Pikuz, S. A. Yan, W. Jeong, T. M. Singh, S. Finke, O. Grittani, G. Nevrkla, M. Lazzarini, C. Velyhan, A. Hayakawa, T. Fukuda, Y. Koga, J. K. Ishino, M. Kondo, Ko. Miyasaka, Y. Kon, A. Nishikino, M. Nosach, Y. V. Khikhlukha, D. Kolesnikov, A. O. Ragozin, E. N. Gasilov, V. A. Kumar, D. Nejdl, J. Sasorov, P. V. Weber, S. Margarone, D. Kato, Y. Korn, G. Kiriyama, H. Kondo, K. Ridgers, C. Kawachi, T. Kando, M. Bulanov, S. V. |
| contents | Gamma rays selectively interact with nuclei, induce and mediate nuclear reactions and elementary particle interactions, and exceed x-rays in penetrating power and thus are indispensable for analysis and modification of dense objects. Yet, the available gamma sources lack sufficient power and brightness. The predicted and highly desirable laser-driven gamma flash, from here on termed "Gamma Flash", based on inverse Compton scattering from solid targets at extreme irradiances (>$10^{23}W/cm^2$), would be the highest-power and the brightest terrestrial gamma source with a 30-40% laser-to-gamma energy conversion. However, Gamma Flash remains inaccessible experimentally due to the Bremsstrahlung background. Here we experimentally demonstrate a new interaction regime at the highest effective irradiance where Gamma Flash scaled quickly with the laser power and produced several times the number of Bremsstrahlung photons. Simulations revealed an attosecond, Terawatt Gamma Flash with a nanometre source size achieving a record brightness exceeding $~10^{23}photons/mm^2mrad^2s$ per 0.1% bandwidth at tens of MeV photon energies, surpassing astrophysical Gamma Ray Bursts. These findings could revolutionize inertial fusion energy by enabling unprecedented sub-micrometre/femtosecond resolution radiography of fuel mixing instabilities in extremely-compressed targets. The new gamma source could facilitate significant advances in time-resolved nuclear physics, homeland security, nuclear waste management and non-proliferation, while opening possibilities for spatially-coherent gamma rays. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_06537 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Demonstration of The Brightest Nano-size Gamma Source Pirozhkov, A. S. Sagisaka, A. Ogura, K. Vishnyakov, E. A. Shatokhin, A. N. Armstrong, C. D. Esirkepov, T. Zh. Izquierdo, B. Gonzalez Pikuz, T. A. Hadjisolomou, P. Alkhimova, M. A. Arran, C. Tsygvintsev, I. P. Valenta, P. Pikuz, S. A. Yan, W. Jeong, T. M. Singh, S. Finke, O. Grittani, G. Nevrkla, M. Lazzarini, C. Velyhan, A. Hayakawa, T. Fukuda, Y. Koga, J. K. Ishino, M. Kondo, Ko. Miyasaka, Y. Kon, A. Nishikino, M. Nosach, Y. V. Khikhlukha, D. Kolesnikov, A. O. Ragozin, E. N. Gasilov, V. A. Kumar, D. Nejdl, J. Sasorov, P. V. Weber, S. Margarone, D. Kato, Y. Korn, G. Kiriyama, H. Kondo, K. Ridgers, C. Kawachi, T. Kando, M. Bulanov, S. V. Plasma Physics High Energy Astrophysical Phenomena Optics Gamma rays selectively interact with nuclei, induce and mediate nuclear reactions and elementary particle interactions, and exceed x-rays in penetrating power and thus are indispensable for analysis and modification of dense objects. Yet, the available gamma sources lack sufficient power and brightness. The predicted and highly desirable laser-driven gamma flash, from here on termed "Gamma Flash", based on inverse Compton scattering from solid targets at extreme irradiances (>$10^{23}W/cm^2$), would be the highest-power and the brightest terrestrial gamma source with a 30-40% laser-to-gamma energy conversion. However, Gamma Flash remains inaccessible experimentally due to the Bremsstrahlung background. Here we experimentally demonstrate a new interaction regime at the highest effective irradiance where Gamma Flash scaled quickly with the laser power and produced several times the number of Bremsstrahlung photons. Simulations revealed an attosecond, Terawatt Gamma Flash with a nanometre source size achieving a record brightness exceeding $~10^{23}photons/mm^2mrad^2s$ per 0.1% bandwidth at tens of MeV photon energies, surpassing astrophysical Gamma Ray Bursts. These findings could revolutionize inertial fusion energy by enabling unprecedented sub-micrometre/femtosecond resolution radiography of fuel mixing instabilities in extremely-compressed targets. The new gamma source could facilitate significant advances in time-resolved nuclear physics, homeland security, nuclear waste management and non-proliferation, while opening possibilities for spatially-coherent gamma rays. |
| title | Demonstration of The Brightest Nano-size Gamma Source |
| topic | Plasma Physics High Energy Astrophysical Phenomena Optics |
| url | https://arxiv.org/abs/2410.06537 |