Results 11 to 20 of about 154,256 (262)
General L p $L_{p}$ -mixed chord integrals of star bodies
Journal of Inequalities and Applications, 2016 The notion of general mixed chord integrals of star bodies was introduced by Feng and Wang. In this paper, we extend the concept of the general mixed chord integrals to general L p $L_{p}$ -mixed chord integrals of star bodies.
Zhaofeng Li, Weidong Wang
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Asymmetric Orlicz Radial Bodies
Mathematics, 2019 Based on the L p -harmonic radial combination, Li and Wang researched the asymmetric L p -harmonic radial bodies, which belong to the asymmetric L p -Brunn-Minkowski theory initiated by Ludwig, Haberl and Schuster.
Hai Li, Weidong Wang, Tongyi Ma
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FORMULATION AND ANTIBACTERIAL TEST OF STAR ANISE EXTRACT (Illicium verum Hook.F) AS A HAND SANITIZER
BioLink, 2020 The hand becomes one of the body parts that are easily exposed to microorganisms because of their high mobility. Hand sanitizer is a liquid that can be used to kill microbes.
Dhanang Puspita +2 more
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Polar duals of convex and star bodies [PDF]
Journal of Inequalities and Applications, 2012 zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Zhao, C, Cheung, WS, Chen, LY
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ON THE VARIANCE OF LOCAL STEREOLOGICAL VOLUME ESTIMATORS
Image Analysis and Stereology, 2011 In the present paper, the variance of local stereological volume estimators is studied. For isotropic designs, the variance depends on the shape of the body under study and the choice of reference point. It can be expressed in terms of an equivalent star
Eva B Vedel Jensen
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Spontaneous scalarization in proto-neutron stars
European Physical Journal C: Particles and Fields, 2023 Proto-neutron stars are born when a highly evolved and massive star collapses under gravity. In this paper, we investigate the spontaneous scalarization in proto-neutron stars.
Fahimeh Rahimi, Zeinab Rezaei
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A Class of Star-Shaped Bodies [PDF]
Canadian Mathematical Bulletin, 1959 The more important properties of the class κ of all bounded convex bodies in E3 with non-empty interior include: uniform approximability by polyhedra, existence of volume and surface area, and Blaschke's selection principle, [l ], [2 ]. In this note we define and consider a class ℋ of star-shaped bodies in E3, which enjoys many properties of κ, among ...
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Tomography of Convex and Star Bodies
Advances in Mathematics, 1994 The authors generalize the notion of a star body and its radial function and define the \(i\)-chord function of a star set for every real \(i\). They apply these notions to solve many problems of geometric tomography which concern sections. For example, they obtain the following interesting results: Corollary 3.5.
Gardner, R.J., Volcic, A.
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Early-forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly
The Astrophysical Journal, 2023 Feedback from massive stars plays an important role in the formation of star clusters. Whether a very massive star is born early or late in the cluster formation timeline has profound implications for the star cluster formation and assembly processes. We
Sean C. Lewis +10 more
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On Star Duality of Mixed Intersection Bodies [PDF]
Journal of Inequalities and Applications, 2007 zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Leng Gangsong, Lu Fenghong, Mao Weihong
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