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Search: (WFRF:(Miron A)) pers:(Healey S) > (2015)

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1.
  • Kublik, C., et al. (author)
  • Integration over curves and surfaces defined by the closest point mapping
  • 2016
  • In: Research in Mathematical Sciences. - : Springer International Publishing. - 2522-0144 .- 2197-9847. ; 3:1
  • Journal article (peer-reviewed)abstract
    • We propose a new formulation for integrating over smooth curves and surfaces that are described by their closest point mappings. Our method is designed for curves and surfaces that are not defined by any explicit parameterization and is intended to be used in combination with level set techniques. However, contrary to the common practice with level set methods, the volume integrals derived from our formulation coincide exactly with the surface or line integrals that one wishes to compute. We study various aspects of this formulation and provide a geometric interpretation of this formulation in terms of the singular values of the Jacobian matrix of the closest point mapping. Additionally, we extend the formulation—initially derived to integrate over manifolds of codimension one—to include integration along curves in three dimensions. Some numerical examples using very simple discretizations are presented to demonstrate the efficacy of the formulation.
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2.
  • Blanco, Carlos, et al. (author)
  • Models of ultraheavy dark matter visible to macroscopic mechanical sensing arrays
  • 2022
  • In: Physical Review D. - 2470-0010 .- 2470-0029. ; 105:11
  • Journal article (peer-reviewed)abstract
    • In recent years, the sensitivity of optomechanical force sensors has improved leading to increased interest in using these devices as particle detectors. In this study we consider scenarios where dark matter with mass close to the Planck scale may be probed by a large array of optomechanical accelerometers. We motivate a macroscopic mechanical search for ultraheavy dark matter, exemplified by the efforts of the Windchime Collaboration, by providing a survey of the model space that would be visible to such a search. We consider two classes of models, one that invokes a new long-range unscreened force and another that is only gravitationally interacting. We identify significant regions of well-motivated, potentially visible parameter space for versatile models such as Q-balls, composite dark matter, relics of gravitational singularities, and gravitationally produced ultraheavy particles.
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3.
  • Petelina, S., et al. (author)
  • Comparison of the Odin/OSIRIS stratospheric ozone profiles with coincident POAM III and ozonesonde measurements
  • 2004
  • In: Geophysical Research Letters. - 1944-8007 .- 0094-8276. ; 31:7, s. L07104-
  • Journal article (peer-reviewed)abstract
    • We present first statistical comparison results for stratospheric ozone density profiles retrieved from Odin/OSIRIS limb scattered radiance with 1220 coincident POAM III and 205 coincident ozonesonde measurements. Profiles are compared on a monthly basis from November 2001 to October 2002. Most of the time, differences between OSIRIS mean profiles and those measured by POAM III and ozonesondes were 5-7% between 15 km and 32 km, and within 15% above 32 km. In April-July 2002, OSIRIS mean profiles appear shifted downward by ∼1 km, introducing a difference of about 10% with POAM III and about 25% with ozonesonde profiles between 15 km and 32 km. This study demonstrates that outside the April-July 2002 period, the OSIRIS ozone profiles agree well with coincident ozonesonde and POAM III ozone profiles and make a valuable addition to the international ozone database available for research into global ozone change.
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  • Result 1-3 of 3

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