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相关论文: The Proto Type of Shanghai Laser Electron Gamma So…

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Shanghai Laser Electron Gamma Source, a $\gamma$-ray beam line of 10MeV order was proposed recently. The beam line is expected to generate $\gamma$-ray with maximum energy of 22MeV by backward Compton scattering between CO$_2$ laser and…

仪器与探测器 · 物理学 2007-05-23 W. Guo , W. Xu , J. G. Chen , Y. G. Ma , X. Z. Cai , H. W. Wang , Y. Xu , C. B. Wang , G. C. Lu , R. Y. Yuan , J. Q. Xu , Z. Y. Wei , Z. Yan , W. Q. Shen

Photonuclear reactions using a laser Compton scattering (LCS) gamma source provide a new method for producing radioisotopes for medical applications. Compared with the conventional method, this method has the advantages of a high specific…

核实验 · 物理学 2024-02-21 Xuan Pang , Bao-Hua Sun , Li-Hua Zhu , Guang-Hong Lu , Hong-Bo Zhou , Dong Yang

On the basis of an energy-recovery linac, a terahertz (THz) source with kilowatts average power is proposed in Shanghai, which will serve as an effective tool in material and biological sciences. In this paper, the physical design of two…

加速器物理 · 物理学 2011-07-29 Jinhua Dai , Haixiao Deng , Zhimin Dai

A high-brilliance ($\sim10^{24}$~photon.s$^{-1}$.mm$^{-2}$.mrd$^{-2}$/0.1\%) gamma-ray source experiment is currently being planned at Fermilab ($E_\gamma\simeq 1.1$~MeV)~[1]. The source implements a high-repetition-rate inverse Compton…

加速器物理 · 物理学 2017-06-28 D. Mihalcea , A. Murokh , P. Piot , J. Ruan

A design for a compact x-ray light source (CXLS) with flux and brilliance orders of magnitude beyond existing laboratory scale sources is presented. The source is based on inverse Compton scattering of a high brightness electron bunch on a…

Shanghai Coherent Light Facility (SCLF) is a quasi-CW hard X-ray free electron laser user facility which is recently proposed. Due to the high repetition rate, high quality electron beams, it is straightforward to consider an X-ray free…

加速器物理 · 物理学 2018-05-09 Kai Li , Haixiao Deng

The possible association between the microquasar LS 5039 and the EGRET source 3EG J1824-1514 suggests that microquasars could also be sources of high energy gamma-rays. In this paper, we explore, with a detailed numerical model, if this…

天体物理学 · 物理学 2009-11-10 V. Bosch-Ramon , J. M. Paredes

A compact Inverse Compton Light Source (ICLS) design is presented, with flux and brilliance orders of magnitude beyond conventional laboratory-scale sources and other compact ICLS designs. This design utilizes the physics of inverse Compton…

加速器物理 · 物理学 2018-08-29 K. E. Deitrick , G. A. Krafft , B. Terzić , J. R. Delayen

Based on collisions between the 100 PW laser and 8 GeV superconducting linear accelerator constructing at the Shanghai hard X-ray free electron laser system (SHINE), the building of GeV-level $\gamma$-ray as well as positron beams are…

加速器物理 · 物理学 2025-04-21 Wanqing Su , Chunwang Ma , Xiguang Cao , Guoqiang Zhang , Yuting Wang

At Shanghai Jiao Tong University, we have established a research laboratory for advanced acceleration research based on high-power lasers and plasma technologies. In a primary experiment based on the laser wakefield acceleration (LWFA)…

等离子体物理 · 物理学 2014-09-11 Ahmed M. M. Elsied , Nasr A. M. Hafz , Song Li , Mohammad Mirzaie , Thomas Sokollik , Jie Zhang

In this article, a feasible switchyard design is proposed for the Shanghai soft x-ray free electron laser facility. In the proposed scheme, a switchyard is used to transport the electron beam to different undulator lines. Three-dimensional…

加速器物理 · 物理学 2017-05-16 Duan Gu , Zhen Wang , Dazhang Huang , Qiang Gu , Meng Zhang

Differential cross sections for Compton scattering from the proton have been measured at scattering angles of $55^\circ$, $90^\circ$, and $125^\circ$ in the laboratory frame using quasimonoenergetic linearly (circularly) polarized photon…

The rapid cycling synchrotron (RCS) is part of China Spallation Neutron Source (CSNS). The RCS provides 1.6GeV protons with a repetition rate of 25Hz. The RF system in RCS is mainly composed of a ferrite loaded RF cavity, a high power…

加速器物理 · 物理学 2014-04-11 Li Xiao , Sun Hong , Long Wei , Zhao Fa-Cheng , Zhang Chun-Lin

Previous analyses of point sources in the gamma-ray range were done either below 30 MeV or above 100 MeV. Below 30 MeV, the imaging Compton telescope (COMPTEL) onboard NASA's Compton Gamma-Ray Observatory detected 26 steady sources in the…

天体物理仪器与方法 · 物理学 2018-02-09 Giacomo Principe , Dmitry Malyshev , Stefan Funk

We propose and demonstrate that a gamma-gamma collider with W_gg < 12 GeV can be added to the European XFEL with a minimal disruption to its main program. High-energy photons will be obtained by Compton scattering of 0.5 micron laser…

加速器物理 · 物理学 2020-12-30 V. I. Telnov

Gamma-ray luminosities of some quasar-associated blazars imply jet powers reaching values comparable to the accretion power even if assuming very strong Doppler boosting and very high efficiency of gamma-ray production. With much lower…

高能天体物理现象 · 物理学 2015-06-17 Marek Sikora , Mateusz Janiak , Krzysztof Nalewajko , Greg M. Madejski , Rafał Moderski

The response of Low Gain Avalanche Diodes (LGADs), a type of thin silicon detector with internal gain, to X-rays of energies between 6-16~keV was characterized at the Stanford Synchrotron Radiation Lightsource (SSRL). The utilized beamline…

Compton scattering of a laser beam with a relativistic electron beam has been used to generate intense, highly polarized and nearly monoenergetic x-ray or gamma-ray beams at many facilities. The ability to predict the spatial, spectral and…

加速器物理 · 物理学 2011-05-09 Changchun Sun , Ying K. Wu

Recently, the microquasar V4641 Sgr and its surrounding is detected at TeV-PeV gamma-ray band. Interestingly, the spectrum follows a power-law function continuing up to 0.8 PeV as reported by LHAASO, and the morphology of the emission…

高能天体物理现象 · 物理学 2025-12-02 Su-Yu Wan , Jie-shuang Wang , Ruo-Yu Liu

The possible associations between the microquasars LS 5039 and LS I +61 303 and the EGRET sources 3EG J1824-1514 and 3EG J0241+6103 suggest that microquasars could also be sources of high-energy gamma-rays. In this work, we present a…

天体物理学 · 物理学 2014-10-13 V. Bosch-Ramon , J. M. Paredes
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