Long Wavelength Cutoff Point Solution

STEP 0: Pre-Calculation Summary
Formula Used
Wavelength Cutoff Point = [hP]*[c]/Bandgap Energy
λc = [hP]*[c]/Eg
This formula uses 2 Constants, 2 Variables
Constants Used
[hP] - Planck constant Value Taken As 6.626070040E-34
[c] - Light speed in vacuum Value Taken As 299792458.0
Variables Used
Wavelength Cutoff Point - (Measured in Meter) - Wavelength Cutoff Point is the point at which is the wavelength at which a material or device ceases to absorb or transmit light efficiently.
Bandgap Energy - (Measured in Joule) - Bandgap Energy of the material, which is the energy difference between the valence band and the conduction band in the material's electronic band structure.
STEP 1: Convert Input(s) to Base Unit
Bandgap Energy: 18 Joule --> 18 Joule No Conversion Required
STEP 2: Evaluate Formula
Substituting Input Values in Formula
λc = [hP]*[c]/Eg --> [hP]*[c]/18
Evaluating ... ...
λc = 1.10358101342875E-26
STEP 3: Convert Result to Output's Unit
1.10358101342875E-26 Meter --> No Conversion Required
FINAL ANSWER
1.10358101342875E-26 1.1E-26 Meter <-- Wavelength Cutoff Point
(Calculation completed in 00.004 seconds)

Credits

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Created by Santhosh Yadav
Dayananda Sagar College Of Engineering (DSCE), Banglore
Santhosh Yadav has created this Calculator and 50+ more calculators!
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Verified by Ritwik Tripathi
Vellore Institute of Technology (VIT Vellore), Vellore
Ritwik Tripathi has verified this Calculator and 100+ more calculators!

25 Optical Detectors Calculators

SNR of Good Avalanche Photodiode ADP Receiver in decibels
​ Go Signal to Noise Ratio = 10*log10((Multiplication Factor^2*Photocurrent^2)/(2*[Charge-e]*Post Detection Bandwidth*(Photocurrent+Dark Current)*Multiplication Factor^2.3+((4*[BoltZ]*Temperature*Post Detection Bandwidth*1.26)/Load Resistance)))
Photocurrent due to Incident Light
​ Go Photocurrent = (Incident Power*[Charge-e]*(1-Reflection Coefficient))/([hP]*Frequency Of Incident Light)*(1-exp(-Absorption Coefficient*Width of Absorption Region))
Probability of Detecting Photons
​ Go Probability of Finding a Photon = ((Variance of Probability Distribution Function^(Number of Incident Photons))*exp(-Variance of Probability Distribution Function))/(Number of Incident Photons!)
Excess Avalanche Noise Factor
​ Go Excess Avalanche Noise Factor = Multiplication Factor*(1+((1-Impact Ionization Coefficient)/Impact Ionization Coefficient)*((Multiplication Factor-1)/Multiplication Factor)^2)
Total Photodiode Current
​ Go Output Current = Dark Current*(exp(([Charge-e]*Photodiode Voltage)/(2*[BoltZ]*Temperature))-1)+Photocurrent
Optical Gain of Phototransistors
​ Go Optical Gain of Phototransistor = (([hP]*[c])/(Wavelength of Light*[Charge-e]))*(Collector Current of Phototransistor/Incident Power)
Average Number of Photons Detected
​ Go Average Number Of Photons Detected = (Quantum Efficiency*Average Received Optical Power*Time Period)/(Frequency Of Incident Light*[hP])
Single Pass Phase Shift through Fabry-Perot Amplifier
​ Go Single-Pass Phase Shift = (pi*(Frequency Of Incident Light-Fabry–Perot Resonant Frequency))/Free Spectral Range of Fabry-Pérot Interferometer
Total Root Mean Square Noise Current
​ Go Total Root Mean Square Noise Current = sqrt(Total Shot Noise^2+Dark Current Noise^2+Thermal Noise Current^2)
Average Received Optical Power
​ Go Average Received Optical Power = (20.7*[hP]*Frequency Of Incident Light)/(Time Period*Quantum Efficiency)
Total Power Accepted by Fiber
​ Go Total Power Accepted by Fiber = Incident Power*(1-(8*Axial Displacement)/(3*pi*Radius of Core))
Multiplied Photocurrent
​ Go Multiplied Photocurrent = Optical Gain of Phototransistor*Responsivity of Photodetector*Incident Power
Temperature Effect on Dark Current
​ Go Dark Current in raised temperature = Dark Current*2^((Changed Temperature-Previous Temperature)/10)
Incident Photon Rate
​ Go Incident Photon Rate = Incident Optical Power/([hP]*Frequency Of Light Wave)
Maximum Photodiode 3 dB Bandwidth
​ Go Maximum 3db Bandwidth = Carrier Velocity/(2*pi*Depletion Layer Width)
Maximum 3dB Bandwidth of Metal Photodetector
​ Go Maximum 3db Bandwidth = 1/(2*pi*Transit Time*PhotoConductive Gain)
Bandwidth Penalty
​ Go Post Detection Bandwidth = 1/(2*pi*Load Resistance*Capacitance)
Long Wavelength Cutoff Point
​ Go Wavelength Cutoff Point = [hP]*[c]/Bandgap Energy
Quantum Efficiency of Photodetector
​ Go Quantum Efficiency = Number of Electrons/Number of Incident Photons
Multiplication Factor
​ Go Multiplication Factor = Output Current/Initial Photocurrent
Electron Rate in Detector
​ Go Electron Rate = Quantum Efficiency*Incident Photon Rate
Transit Time with respect to Minority Carrier Diffusion
​ Go Diffusion Time = Distance^2/(2*Diffusion Coefficient)
Longest Transit Time
​ Go Transit Time = Depletion Layer Width/Drift Velocity
3 dB Bandwidth of Metal Photodetectors
​ Go Maximum 3db Bandwidth = 1/(2*pi*Transit Time)
Detectivity of Photodetector
​ Go Detectivity = 1/Noise Equivalent Power

Long Wavelength Cutoff Point Formula

Wavelength Cutoff Point = [hP]*[c]/Bandgap Energy
λc = [hP]*[c]/Eg

How is long wavelength cutoff point helpful?

It's essential in optics and photonics for characterizing materials, selecting appropriate ones for optical devices, and understanding the behavior of materials in optoelectronic applications like lasers and photodetectors. This equation offers insights into the electronic band structure of materials and the interplay between quantum mechanics and electromagnetism in optical phenomena.

How to Calculate Long Wavelength Cutoff Point?

Long Wavelength Cutoff Point calculator uses Wavelength Cutoff Point = [hP]*[c]/Bandgap Energy to calculate the Wavelength Cutoff Point, Long Wavelength Cutoff Point allows you to calculate the cutoff wavelength for a given material based on its bandgap energy. It's particularly relevant in the design of semiconductor devices and optical components, as the cutoff wavelength determines the range of wavelengths of light that can be efficiently absorbed or transmitted by the material. Wavelength Cutoff Point is denoted by λc symbol.

How to calculate Long Wavelength Cutoff Point using this online calculator? To use this online calculator for Long Wavelength Cutoff Point, enter Bandgap Energy (Eg) and hit the calculate button. Here is how the Long Wavelength Cutoff Point calculation can be explained with given input values -> 1.1E-26 = [hP]*[c]/18.

FAQ

What is Long Wavelength Cutoff Point?
Long Wavelength Cutoff Point allows you to calculate the cutoff wavelength for a given material based on its bandgap energy. It's particularly relevant in the design of semiconductor devices and optical components, as the cutoff wavelength determines the range of wavelengths of light that can be efficiently absorbed or transmitted by the material and is represented as λc = [hP]*[c]/Eg or Wavelength Cutoff Point = [hP]*[c]/Bandgap Energy. Bandgap Energy of the material, which is the energy difference between the valence band and the conduction band in the material's electronic band structure.
How to calculate Long Wavelength Cutoff Point?
Long Wavelength Cutoff Point allows you to calculate the cutoff wavelength for a given material based on its bandgap energy. It's particularly relevant in the design of semiconductor devices and optical components, as the cutoff wavelength determines the range of wavelengths of light that can be efficiently absorbed or transmitted by the material is calculated using Wavelength Cutoff Point = [hP]*[c]/Bandgap Energy. To calculate Long Wavelength Cutoff Point, you need Bandgap Energy (Eg). With our tool, you need to enter the respective value for Bandgap Energy and hit the calculate button. You can also select the units (if any) for Input(s) and the Output as well.
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