M. Charlwood

ORCID: 0000-0003-2277-0121
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About
Contact & Profiles
Research Areas
  • Laser Design and Applications
  • Atomic and Molecular Physics
  • Laser-Plasma Interactions and Diagnostics
  • Laser-Matter Interactions and Applications
  • Particle Detector Development and Performance
  • X-ray Spectroscopy and Fluorescence Analysis
  • Laser-induced spectroscopy and plasma
  • Advanced X-ray Imaging Techniques
  • Astrophysical Phenomena and Observations
  • Astrophysics and Cosmic Phenomena
  • Scientific Measurement and Uncertainty Evaluation
  • Laser Material Processing Techniques

Queen's University Belfast
2022-2024

We describe laboratory experiments to generate x-ray photoionized plasmas of relevance accretion-powered sources such as neutron star binaries and quasars, with significant improvements over previous work. A key quantity is referenced, namely the photoionization parameter, defined ξ=4πF/ne where F flux ne electron density. This normally meaningful in an astrophysical steady-state context, but also commonly used literature a figure merit for that are, necessity, time-dependent. demonstrate...

10.1016/j.hedp.2024.101097 article EN cc-by High Energy Density Physics 2024-03-19

We present results from a pilot study, using laser-produced plasma, to identify new lines in the 350 1000 nm spectral region for r-process element gold (Au), of relevance studies neutron star mergers. This was achieved via optical-IR spectroscopy Au with an target high purity (99.95 %) and low vacuum pressure remove any air contamination experimental spectra. Our data were recorded spectrometer 750 mm focal length 1200 mm-1 grating, yielding resolution 0.04 nm. find 54 not previously...

10.1088/1402-4896/ad650f article EN cc-by Physica Scripta 2024-08-01

We describe laboratory experiments to generate X-ray photoionized plasmas of relevance accretion-powered sources such as neutron star binaries and quasars, with significant improvements over previous work. A key quantity is referenced, namely the photoionization parameter. This normally meaningful in an astrophysical steady-state context, but also commonly used literature a figure merit for that are, necessity, time-dependent. demonstrate emission-weighted values {\xi} > 50 ergcm/s using...

10.48550/arxiv.2309.07267 preprint EN other-oa arXiv (Cornell University) 2023-01-01

We describe laboratory experiments to generate x-ray photoionized plasmas of relevance accretion-powered sources such as neutron star binaries and quasars, with significant improvements over previous work. refer a key quantity, the photoionization parameter, defined [[EQUATION]] where F is flux ne electron density. This usually meaningful in steady state context, but commonly used, literature, figure merit for that are, necessity, time dependent. demonstrate we can achieve values erg-cm s-1...

10.2139/ssrn.4608538 preprint EN 2023-01-01

We have employed the VULCAN laser facility to generate a plasma X-ray source for use in photoionization experiments. A nanosecond pulse with an intensity of order 10 15 Wcm −2 was used irradiate thin Ag or Sn foil targets coated onto parylene substrate, and L-shell emission 3.3–4.4 keV range recorded both laser-irradiated nonirradiated sides. Both experimental simulation results show higher conversion yields compared Sn, our simulations indicating approximately factor two than those found...

10.1155/2022/3234804 article EN cc-by Laser and Particle Beams 2022-06-06

We have employed the VULCAN laser facility to generate a plasma X-ray source for use in photoionisation experiments. A nanosecond pulse with an intensity of order ${10}^{15}$ W{cm}$^{-2}$ was used irradiate thin Ag or Sn foil targets coated onto parylene substrate, and L-shell emission $3.3-4.4$ keV range recorded both laser-irradiated non-irradiated sides. Both experimental simulation results show higher conversion yields compared Sn, our simulations indicating approximately factor two than...

10.48550/arxiv.2204.11129 preprint EN cc-by arXiv (Cornell University) 2022-01-01
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