Related Experiment Video
Updated: Mar 30, 2026

07:11
ARL Spectral Fitting as an Application to Augment Spectral Data via Franck-Condon Lineshape Analysis and Color Analysis
Published on: August 19, 2021
3.1K
Lévy flights with power-law absorption
Luca Cattivelli1, Elena Agliari2, Fabio Sartori3
1Scuola Normale Superiore, Pisa, Italy.
Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics
|November 14, 2015
Summary
A particle
Area of Science:
- Statistical physics
- Stochastic processes
- Condensed matter physics
Background:
- Stochastic particle motion is fundamental in various physical phenomena.
- Understanding target-trapping dynamics is crucial for processes like diffusion and reaction kinetics.
Purpose of the Study:
- To investigate the trapping probability of a particle undergoing power-law distributed stochastic motion in a 1D lattice.
- To analyze the influence of target distribution on the trapping dynamics.
Main Methods:
- Analytical derivation of trapping probability.
- Numerical simulations of particle trajectories.
- Analysis of power-law distributions for jump lengths and target locations.
Main Results:
- A finite probability of never being trapped exists if the jump length exponent (μ) is less than the target distribution exponent (α).
- Power-law target distributions significantly impact trapping dynamics.
- Simulations confirm analytical findings and reveal slow searching times in finite systems.
Conclusions:
- The interplay between particle motion and target distribution determines the ultimate trapping of a stochastic walker.
- The study provides insights into conditions where a particle might evade capture indefinitely in a 1D system.
- Findings have implications for understanding diffusion-limited reactions and search processes in complex environments.
Related Concept Videos
UV–Vis Spectroscopy: Beer–Lambert Law
8.2K
The Beer-Lambert law describes the relationship between absorbance and concentration, which combines the principles established by scientists Johann Heinrich Lambert and August Beer. Lambert's law states that when light passes through a medium, the loss in intensity is directly proportional to the original intensity and the path length of the light. Beer's law proposed that the transmittance of a solution remains constant if the product of concentration and path length is constant. The modern...
8.2K
IR Spectroscopy: Hooke's Law Approximation of Molecular Vibration
3.7K
A covalently bonded heteronuclear diatomic molecule can be modeled as two vibrating masses connected by a spring. The vibrational frequency of the bond can be expressed using an equation derived from Hooke's law, which describes how the force applied to stretch or compress a spring is proportional to the displacement of the spring. In this case, the atoms behave like masses, and the bond acts like a spring.
According to Hooke's law, the vibrational frequency is directly proportional to...
According to Hooke's law, the vibrational frequency is directly proportional to...
3.7K
Molecular Spectroscopy: Absorption and Emission
5.4K
Molecules possess discrete energy levels called quantum states. Unlike atoms, which have simpler energy levels, molecules possess additional rotational and vibrational energy levels. Each energy level is separated by an energy gap, with the gaps between adjacent electronic, vibrational, and rotational levels varying significantly. The three types of energy levels in a diatomic molecule are shown in Figure 1.
5.4K
UV–Vis Spectroscopy: Woodward–Fieser Rules
29.6K
UV–Visible absorption spectra of conjugated dienes arise from the lowest energy π → π* transitions. The light-absorbing part of the molecule is called the chromophore, and the substituents directly attached to the chromophore are called auxochromes. A strong correlation exists between the absorption maxima, λmax, and the structure of a conjugated π system. The Woodward–Fieser rules predict the value of λmax for a given structure by adding the...
29.6K
Absorption of Radiation
1.5K
The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
1.5K
Atomic Absorption Spectroscopy: Radiation and Light Sources
1.6K
Atomic absorption spectroscopy (AAS) relies on the Beer-Lambert law, which requires that the radiation source emits a narrow range of wavelengths to match the absorption characteristics of the analyte atom. The primary criteria for choosing an appropriate radiation source in AAS is to provide a precise and intense emission at specific wavelengths that will allow accurate detection of the analyte.
Two common narrow-range 'line' sources used in AAS are hollow-cathode lamps (HCLs) and...
Two common narrow-range 'line' sources used in AAS are hollow-cathode lamps (HCLs) and...
1.6K

