Related Experiment Video
Updated: Feb 5, 2026

05:18
A Rapid and Chemical-free Hemoglobin Assay with Photothermal Angular Light Scattering
Published on: December 7, 2016
10.2K
Angular range, sampling and noise considerations for inverse light scattering analysis of nuclear morphology
Haoran Zhang1, Zachary A Steelman1, Derek S Ho1
1Department of Biomedical Engineering, Duke University, Durham, North Carolina.
Journal of Biophotonics
|September 22, 2018
Summary
Angle-resolved low-coherence interferometry (a/LCI) extracts nuclear morphology for dysplasia detection. Optimizing angular sampling, range, and noise in optical biopsies enhances diagnostic utility and guides future probe design.
Area of Science:
- Biomedical Optics
- Medical Imaging
- Cancer Diagnostics
Background:
- Angle-resolved elastic scattering analyzes nuclear morphology in tissues.
- Angle-resolved low-coherence interferometry (a/LCI) successfully identifies nuclear alterations linked to dysplasia.
- Optical biopsies are limited by collecting only a fraction of the 4π scattering field.
Purpose of the Study:
- To comprehensively characterize the diagnostic impact of angular sampling, range, and noise in inverse light scattering analysis of nuclear morphology.
- To apply these findings to a scanning a/LCI system.
- To inform the design of next-generation optical biopsy probes.
Main Methods:
- Utilized a dataset from 40 patients undergoing a/LCI optical biopsy for cervical dysplasia.
- Analyzed the diagnostic utility of variations in angular sampling, range, and noise.
- Applied results to a benchtop scanning a/LCI system.
Main Results:
- Variations in angular sampling, range, and noise significantly impact the diagnostic utility of inverse light scattering analysis.
- The study identified key parameters for optimizing diagnostic information from limited angular sampling.
- Findings are directly applicable to refining a/LCI system design.
Conclusions:
- Optimizing angular sampling, range, and noise is crucial for maximizing diagnostic information in optical biopsies.
- This research provides essential insights for developing more effective next-generation optical biopsy probes.
- The study enhances the diagnostic capabilities of a/LCI for cervical dysplasia detection.
Related Concept Videos
Nuclear Stability
23.3K
Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
To hold positively charged protons together...
To hold positively charged protons together...
23.3K
Range
14.2K
The range is one of the measures of variation. It can be defined as the difference between a dataset's highest and lowest values. For example, in the study of seven 16-ounce soda cans, the filled volume of soda was measured, thus producing the following amount (in ounces) of soda:
15.9; 16.1; 15.2; 14.8; 15.8; 15.9; 16.0; 15.5
Measurements of the amount of soda in a 16-ounce can vary since different subjects record these measurements or since the exact amount - 16 ounces of liquid, was not...
15.9; 16.1; 15.2; 14.8; 15.8; 15.9; 16.0; 15.5
Measurements of the amount of soda in a 16-ounce can vary since different subjects record these measurements or since the exact amount - 16 ounces of liquid, was not...
14.2K
Nuclear Transmutation
20.7K
Nuclear transmutation is the conversion of one nuclide into another. It can occur by the radioactive decay of a nucleus, or the reaction of a nucleus with another particle. The first manmade nucleus was produced in Ernest Rutherford’s laboratory in 1919 by a transmutation reaction, the bombardment of one type of nuclei with other nuclei or with neutrons. Rutherford bombarded nitrogen-14 atoms with high-speed α particles from a natural radioactive isotope of radium and observed...
20.7K
The Wave Nature of Light
61.4K
The nature of light has been a subject of inquiry since antiquity. In the seventeenth century, Isaac Newton performed experiments with lenses and prisms and was able to demonstrate that white light consists of the individual colors of the rainbow combined together. Newton explained his optics findings in terms of a "corpuscular" view of light, in which light was composed of streams of extremely tiny particles traveling at high speeds according to Newton's laws of motion.
61.4K
Nuclear Fusion
33.9K
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
33.9K
Nuclear Binding Energy
14.8K
The difference between the calculated and experimentally measured masses is known as the mass defect of the atom. In the case of helium-4, the mass defect indicates a “loss” in mass of 4.0331 amu – 4.0026 amu = 0.0305 amu. The loss in mass accompanying the formation of an atom from protons, neutrons, and electrons is due to the conversion of that mass into energy that is evolved as the atom forms. The nuclear binding energy is the energy produced when the atoms’ nucleons are bound...
14.8K

