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Related Concept Videos

Estimation of the Physical Quantities01:05

Estimation of the Physical Quantities

On many occasions, physicists, other scientists, and engineers need to make estimates of a particular quantity. These are sometimes referred to as guesstimates, order-of-magnitude approximations, back-of-the-envelope calculations, or Fermi calculations. The physicist Enrico Fermi was famous for his ability to estimate various kinds of data with surprising precision. Estimating does not mean guessing a number or a formula at random. Instead, estimation means using prior experience and sound...
Gauss's Law: Spherical Symmetry01:26

Gauss's Law: Spherical Symmetry

A charge distribution has spherical symmetry if the density of charge depends only on the distance from a point in space and not on the direction. In other words, if the system is rotated, it doesn't look different. For instance, if a sphere of radius R is uniformly charged with charge density ρ0, then the distribution has spherical symmetry. On the other hand, if a sphere of radius R is charged so that the top half of the sphere has a uniform charge density ρ1 and the bottom half has a uniform...
Ostwald’s Dilution Law01:25

Ostwald’s Dilution Law

Consider a binary electrolyte AB with a concentration ‘c’ that reversibly dissociates into its constituent ions. The degree of this dissociation is represented by ⍺. This means that the equilibrium concentration of each ionic species can be expressed as ⍺c. As well as this, the fraction of the electrolyte that remains undissociated at equilibrium is given by (1−⍺). The corresponding equilibrium concentration for this undissociated portion is then calculated as (1−⍺)c. For such solutions,...
Gravitation Between Spherically Symmetric Masses01:14

Gravitation Between Spherically Symmetric Masses

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Schwarzschild Radius and Event Horizon01:21

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No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
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Maxwell-Boltzmann Distribution: Problem Solving01:20

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Individual molecules in a gas move in random directions, but a gas containing numerous molecules has a predictable distribution of molecular speeds, which is known as the Maxwell-Boltzmann distribution, f(v).
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Updated: Jun 10, 2026

An Efficient and Flexible Cell Aggregation Method for 3D Spheroid Production
07:46

An Efficient and Flexible Cell Aggregation Method for 3D Spheroid Production

Published on: March 27, 2017

Approximation to extinction efficiency for randomly oriented spheroids.

G R Fournier, B T Evans

    Applied Optics
    |August 12, 2010
    PubMed
    Summary
    This summary is machine-generated.

    A new approximation for light extinction efficiency in spheroids offers a 10,000x speedup. This method accurately models various particle sizes and refractive indices, validating its broad applicability in scattering calculations.

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    Scattering And Absorption of Light in Planetary Regoliths
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    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Area of Science:

    • Light scattering and radiative transfer
    • Computational physics and optics
    • Atmospheric and aerosol science

    Background:

    • Accurate calculation of extinction efficiency (Q(ext)) for spheroids is crucial for understanding light interaction with matter.
    • Existing methods like the extended boundary condition (EBC) or T-matrix methods are computationally intensive.
    • A need exists for faster, yet accurate, approximations for Q(ext) in diverse applications.

    Purpose of the Study:

    • To develop and validate a semiempirical approximation for the extinction efficiency of randomly oriented spheroids.
    • To significantly accelerate the computation of Q(ext) compared to established numerical methods.
    • To assess the accuracy and limitations of the proposed approximation across various physical parameters.

    Main Methods:

    • Extension of the anomalous diffraction formula to approximate Q(ext) for spheroids.
    • Comparison of the approximation with results from the extended boundary condition (EBC) method and the T-matrix method.
    • Verification of the approximation for a range of complex refractive indices (1.01 ≤ n ≤ 2.00, 0 ≤ k ≤ 1) and aspect ratios (0.5 to 4).

    Main Results:

    • The proposed semiempirical approximation provides a computational speedup exceeding 10^4 times over previous methods.
    • The approximation demonstrates good agreement with EBC and T-matrix methods for the tested ranges of refractive indices and aspect ratios.
    • The formula exhibits correct asymptotic behavior in both the Rayleigh scattering and large particle limits.

    Conclusions:

    • The developed semiempirical approximation offers a computationally efficient and accurate alternative for calculating spheroid extinction efficiency.
    • The approximation is believed to be uniformly valid across all size parameters and aspect ratios.
    • This advancement facilitates faster and more extensive studies in fields reliant on light scattering by non-spherical particles.