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Zero-to ultralow-field nuclear magnetic resonance and its applications 被引量:2
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作者 Min Jiang Ji Bian +6 位作者 Qing Li Ze Wu Haowen Su Minxiang Xu Yuanhong Wang Xin Wang Xinhua Peng 《Fundamental Research》 CAS 2021年第1期68-84,共17页
As a complementary analysis tool to conventional high-field nuclear magnetic resonance(NMR),zero-to ultralow-field(ZULF)NMR detects nuclear magnetization signals in the sub-microtesla regime.Spin-exchange relaxation-f... As a complementary analysis tool to conventional high-field nuclear magnetic resonance(NMR),zero-to ultralow-field(ZULF)NMR detects nuclear magnetization signals in the sub-microtesla regime.Spin-exchange relaxation-free(SERF)atomic magnetometers provide a new generation of sensitive detectors for ZULF NMR.Owing to features such as low cost,high resolution,and portability,ZULF NMR has recently attracted considerable attention in chemistry,biology,medicine,and tests of fundamental physics.This review describes the basic principles,methodology,and recent experimental and theoretical development of ZULF NMR as well as its applications in spectroscopy,quantum control,imaging,NMR-based quantum devices,and tests of fundamental physics.The future prospects of ZULF NMR are also discussed. 展开更多
关键词 zero-to ultralow-field NMR atomic magnetometer SPECTROSCOPY quantum control imaging NMR-based quantum devices tests of fundamental physics
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Some highlights of the Gamma-ray first four years of the Fermi Space Telescope
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作者 Steven Ritz 《Frontiers of physics》 SCIE CSCD 2013年第6期693-713,共21页
The Fermi Gamma-ray Space Telescope, formerly called GLAST, measures the cosmic gamma-ray flux in the energy range 8 keV to 〉 300 GeV. In addition to breakthrough capabilities in energy coverage and localization, the... The Fermi Gamma-ray Space Telescope, formerly called GLAST, measures the cosmic gamma-ray flux in the energy range 8 keV to 〉 300 GeV. In addition to breakthrough capabilities in energy coverage and localization, the very large field of view enables observations of 20~ of the sky at any instant, and the entire sky on a timescale of a few hours. With its launch in 2008, Fermi opens a new and important window on a wide variety of phenomena, including pulsars, black holes and active galactic nuclei, gamma-ray bursts, supernova remnants and the origins of cosmic rays, and searches for hypothetical new phenomena such as particle dark matter annihilations. A brief overview and selected science highlights from the first four years are provided. 展开更多
关键词 high-energy gamma-ray astrophysics dark matter fundamental physics tests spacebased astrophysics space-based particle astrophysics gamma-ray bursts BLAZARS PULSARS
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