Q.Ultraviolet light of wavelength 2271 A˚ from a 100 W mercury source irradiates a photo-cell made of molybdenum metal. If the stopping potential is −1.3 V, estimate the work function of the metal. How would the photo-cell respond to a high intensity (∼105 W m−2) red light of wavelength 6328 A˚ produced by a He-Ne laser?
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🔒 Start your 14-day free trial to unlock the full solution →Concept understanding — Maximum Kinetic Energy
Maximum Kinetic Energy – From Intuition to Precision
Kinetic energy is the energy of motion: the faster something moves, the more kinetic energy it has. In many physical situations there is a maximum possible kinetic energy a particle can reach — set either by energy conservation or by an external energy constraint.
The Precise Statement
Kmax=21mvmax2
Where:
- Kmax = maximum kinetic energy (in joules)
- m = mass of the object (in kg)
- vmax = maximum speed reached (in m/s)
This formula alone doesn't tell you why there's a maximum — the physics lies in energy conservation or in an external constraint that limits the speed.
Where Does the Maximum Come From?
1. Energy conservation (no friction)
In a closed system, total mechanical energy E=K+U is constant, so
Kmax=E−Umin
The maximum kinetic energy occurs when the potential energy U is at its minimum — for example, a falling object is fastest (and U smallest) just before it lands.
2. External constraints (e.g., the photoelectric effect)
In modern physics, electrons in a metal absorb light energy. Each photon delivers a fixed energy hf. The electron must spend part of that energy escaping the metal (the work function ϕ); the rest becomes kinetic energy:
Kmax=hf−ϕ
Here the maximum is set entirely by the photon energy — no matter how intense the light, no single electron can gain more kinetic energy than this.
A Common Mistake
Students often think "maximum kinetic energy" means the fastest speed possible in the universe. It doesn't. The "maximum" is relative to the given system — the highest value under the stated conditions (height, spring compression, photon energy, and so on), not a universal speed limit. …
Why this formula?
Maximum Kinetic Energy — Why the Formula Holds
The idea of "maximum kinetic energy" appears in two very different contexts in your syllabus: photoelectric effect (modern physics) and simple harmonic motion (oscillations). I'll cover both, because the why is different in each case.
1. In the Photoelectric Effect
The formula you must know:
Kmax=hν−ϕ
where h is Planck's constant, ν is the frequency of incident light, and ϕ is the work function of the metal.
Why this formula? It comes from Einstein's photon model and energy conservation.
A single photon carries energy E=hν. When it strikes a metal surface, it can transfer all of its energy to one electron. That electron must first overcome the binding force holding it in the metal — the minimum energy needed for this is the work function ϕ. Any leftover energy becomes the electron's kinetic energy after it escapes.
So:
Photon energy = Energy to escape + Kinetic energy of ejected electron
hν=ϕ+K
If the electron just barely escapes (with zero kinetic energy), the photon frequency is the threshold frequency ν0, where hν0=ϕ.
For a higher frequency, the maximum kinetic energy an ejected electron can have is when it absorbs the photon's full energy and loses nothing to collisions inside the metal. That gives:
Kmax=hν−ϕ
Kmax does not depend on light intensity. Intensity only increases the number of electrons, not their maximum energy. This was the key puzzle that classical physics couldn't explain.
2. In Simple Harmonic Motion (SHM)
For a particle executing SHM, the maximum kinetic energy is:
Kmax=21mω2A2
where m is mass, ω is angular frequency, and A is amplitude.
Why this formula? It follows directly from the velocity equation.
In SHM, displacement is x=Asin(ωt+ϕ). Differentiating gives velocity:
v=dtdx=Aωcos(ωt+ϕ)
The velocity is maximum when cos(ωt+ϕ)=±1, i.e., at the equilibrium position (x=0):
vmax=Aω …
The stopping potential fixes the photoelectrons' maximum kinetic energy, and subtracting that from the UV photon's energy gives the metal's work function; since red light's photon energy turns out to be below this work function, no amount of intensity can trigger photoemission with it. …
From Einstein's equation KEmax=hc/λ−ϕ with the given stopping voltage, ϕ≈4.17 eV. The red laser's photon energy (~1.96 eV) is below this work function, so no photoelectrons are emitted from it regardless of how intense the beam is made — only photon energy (frequency), not intensity, determines whether emission occurs at all.
Step 1 — Energy of the UV photon.
E=λhc=2271×10−10(6.63×10−34)(3×108)=2.271×10−71.989×10−25≈8.76×10−19 J
E≈1.6×10−198.76×10−19≈5.47 eV
Step 2 — Work function from Einstein's photoelectric equation.
The magnitude of the stopping potential gives the maximum kinetic energy directly: KEmax=eV0=1.3 eV.
ϕ=E−KEmax=5.47−1.3≈4.17 eV
(This matches molybdenum's known work function well.)
Step 3 — Would the red He-Ne laser light cause photoemission?
Photon energy of the red light (λ=6328 A˚):
Ered=λhc=6.328×10−71.989×10−25≈3.14×10−19 J≈1.96 eV …
Showing the 12 most recent of 24 on this concept.
- TG EAPCET 2026Set eng-2026-05-09-AN1 markMCQQ.When photons of wavelength 4000 A˚ are incident on a photosensitive material of cut-off wavelength 4800 A˚, the stopping potential is V. If the same photons incident on another photosensitive material of cut off wavelength 6000 A˚, then the stopping potential is (A) 1.5V (B) 0.5V (C) 4V (D) 2V
›Reveal solutionSolution
With fixed incident wavelength, eV=hc(λ1−λ01); the new stopping potential works out to 2V.
Photoelectric equation with incident wavelength λ=4000A˚ and cut-off λ0:
eV=λhc−λ0hc=hc(λ1−λ01)
First material, λ0=4800A˚:
eV=hc(40001−48001)=hc⋅240001 …
- TG EAPCET 2026Set eng-2026-05-10-FN1 markMCQQ.The process of electron emission that takes place in a spark plug is (A) Field emission (B) Photoelectric emission (C) Thermionic emission (D) Secondary emission
›Reveal solutionSolution
The intense electric field generated across the spark plug gap pulls electrons directly from the electrode surface, a process known as field emission, which initiates the spark. The correct option is (A).
Concept and Intuition
A spark plug's primary function is to ignite the air-fuel mixture in an internal combustion engine by creating an electrical spark. This spark is essentially a controlled electrical breakdown of the gas between two electrodes. For this breakdown to occur, electrons must first be emitted from the negative electrode (cathode) into the gas gap. These initial electrons are then accelerated by the strong electric field, collide with gas molecules, and ionize them, leading to an avalanche of charge carriers that forms the visible spark.
The key to understanding the emission process lies in the conditions present in a spark plug:
- High Voltage: The ignition system applies tens of thousands of volts across a small gap (typically 0.6 to 1.5 mm).
- Intense Electric Field: This high voltage across a small gap creates an extremely strong electric field.
- Ambient Temperature: While the engine cylinder can get hot, the initial spark generation, especially during a cold start, does not rely on the electrodes being at a very high temperature.
- No External Light/Particles: There is no external source of high-energy light or bombarding particles to initiate the process.
We need to identify which electron emission mechanism is best suited to these conditions.
Step-by-step Analysis
Let's examine each type of electron emission:
-
Field Emission:
- Concept: Field emission occurs when a very strong electric field (typically 107 V/m to 109 V/m) is applied to a metal surface. This intense field distorts the potential energy barrier at the metal surface, making it thin enough for electrons to "tunnel" through it and escape the metal, even at low temperatures.
- Relevance to Spark Plug: A spark plug generates extremely high voltages. For example, if 20,000 V is applied across a 1 mm gap, the average electric field is E=dV=1×10−3 m20,000 V=2×107 V/m. Local field enhancements at sharp points or irregularities on the electrode surface can make the actual field much higher, easily reaching the threshold for field emission. These emitted electrons are crucial for initiating the gas breakdown and forming the spark.
- Conclusion: This is a highly plausible mechanism for initiating the spark.
-
Photoelectric Emission:
- Concept: Photoelectric emission is the ejection of electrons from a metal surface when light of sufficient frequency (and thus photon energy) strikes it.
- Relevance to Spark Plug: There is no external light source of sufficient energy (like ultraviolet light) directed at the spark plug electrodes to cause electron emission.
- Conclusion: This is not the mechanism.
-
Thermionic Emission: …
- TG EAPCET 2026Set eng-2026-05-11-FN1 markMCQQ.When monochromatic photons incident on a photosensitive material of work function 1.8 eV, photoelectrons are emitted with a maximum kinetic energy of 2.2 eV. If the frequency of the incident photons is doubled, then the maximum kinetic energy of the emitted photoelectrons is (A) 7.2 eV (B) 6.2 eV (C) 4.4 eV (D) 3.6 eV
›Reveal solutionSolution
Using Einstein’s photoelectric equation, the incident photon energy is found from the given work function and maximum kinetic energy; doubling the frequency doubles the photon energy, and the new kinetic energy is that doubled energy minus the work function, giving 6.2 eV.
The key idea is Einstein’s photoelectric equation:
Kmax=hf−ϕ
where Kmax is the maximum kinetic energy of emitted electrons, hf is the energy of an incident photon, and ϕ is the work function (the minimum energy needed to eject an electron).
We are given ϕ=1.8 eV and Kmax=2.2 eV for the original frequency f. This lets us find the original photon energy. Then, if the frequency is doubled, the new photon energy is h(2f)=2hf. The new kinetic energy is simply that new photon energy minus the same work function.
- Find the original photon energy From Kmax=hf−ϕ:
hf=Kmax+ϕ=2.2 eV+1.8 eV=4.0 eV
- Double the frequency The new photon energy is:
h(2f)=2×(hf)=2×4.0 eV=8.0 eV
- Compute the new maximum kinetic energy Using the same equation with the new photon energy:
- TG EAPCET 2026Set ap-2026-05-04-FN1 markMCQQ.The slope of the graph drawn by taking the frequency (in 1015 Hz) of light incident on a photosensitive material on x-axis and the stopping potential (in volt) on y-axis is nearly (A) 8.250 (B) 2.420 (C) 4.125 (D) 3.175
›Reveal solutionSolution
The slope of the stopping potential vs. frequency graph in the photoelectric effect is h/e, and its numerical value is approximately 4.125×10−15 V⋅s, which matches option (C).
The photoelectric effect equation is the key here. Einstein’s photoelectric equation relates the stopping potential V0, the frequency f of incident light, the work function ϕ, and Planck’s constant h:
eV0=hf−ϕ
Here e is the electron charge. Rearranging for V0 as a function of f:
V0=ehf−eϕ
This is a straight line of the form y=mx+c, where y=V0, x=f, the slope m=h/e, and the intercept c=−ϕ/e. So the slope of the graph is simply Planck’s constant divided by the electronic charge.
Now, the problem gives frequency in units of 1015 Hz and stopping potential in volts. That means the x-axis is actually f×10−15 Hz — but the slope we compute must account for this scaling. Let’s work it out step by step.
- Recall the known constants Planck’s constant h=6.626×10−34 J⋅s Electron charge e=1.602×10−19 C The slope in SI units (V/Hz) is:
eh=1.602×10−196.626×10−34≈4.135×10−15 V/Hz
- Account for the x-axis scaling The x-axis uses frequency in units of 1015 Hz. That means if the actual frequency is f Hz, the graph plots f/1015 on the x-axis. So the slope read from the graph (change in V0 per unit change on the scaled axis) is:
slopegraph=Δ(f/1015)ΔV0=1015×ΔfΔV0=1015×eh
- Compute the numerical value Using h/e≈4.135×10−15 V/Hz: …
- TG EAPCET 2025Set eng-2025-05-03-AN1 markMCQQ.When photons incident on a photosensitive material of work function 1.5 eV, the maximum velocity of the emitted photoelectrons is 8×105 ms−1. The stopping potential of the photoelectrons is (Mass of the electron =9×10−31 kg and charge of the electron =1.6×10−19 C) (A) 1.8 V (B) 1.5 V (C) 2.1 V (D) 2.4 V
›Reveal solutionSolution
The stopping potential is found by equating the maximum kinetic energy of the photoelectrons to the work done by the stopping voltage. Using Kmax=21mvmax2 and Kmax=eVs, we get Vs≈1.8V, so the correct option is (A).
The key idea here is that the stopping potential is the voltage that just barely stops the fastest photoelectrons from reaching the other electrode. That means the electrical work done on the electron (charge × voltage) exactly equals its maximum kinetic energy. So we don’t even need the work function or the photon energy — the maximum speed alone gives us the stopping potential directly.
- Write the relation between kinetic energy and stopping potential. The stopping potential Vs is defined by:
eVs=Kmax
where e=1.6×10−19C is the electron charge and Kmax is the maximum kinetic energy of the emitted photoelectrons.
- Compute the maximum kinetic energy from the given speed. The maximum speed is vmax=8×105m/s and the electron mass is m=9×10−31kg.
Kmax=21mvmax2=21×(9×10−31)×(8×105)2
First square the speed: (8×105)2=64×1010=6.4×1011.
Then:
Kmax=21×9×10−31×6.4×1011=21×57.6×10−20=28.8×10−20J
So Kmax=2.88×10−19J.
- Convert this energy to electronvolts (optional but helpful for intuition). Since 1eV=1.6×10−19J, Kmax=1.6×10−192.88×10−19=1.8eV …
- TG EAPCET 2025Set eng-2025-05-03-FN1 markMCQQ.When photons incident on a photosensitive material of work function 1.5 eV, the maximum velocity of the emitted photoelectrons is 8×105 ms−1. The stopping potential of the photoelectrons is (Mass of the electron =9×10−31 kg and charge of the electron =1.6×10−19 C) (A) 2.1 V (B) 2.4 V (C) 1.5 V (D) 1.8 V
›Reveal solutionSolution
The stopping potential is found by equating the maximum kinetic energy of the photoelectrons to the work done by the stopping voltage. Using Kmax=21mvmax2 and Kmax=eVs, we get Vs≈1.8 V, so the correct option is (D).
The key idea here is that the stopping potential is the voltage that just barely stops the fastest photoelectrons from reaching the other electrode. In the photoelectric effect, the maximum kinetic energy of the emitted electrons is given by Einstein’s equation:
Kmax=hf−ϕ
But we don’t know the photon frequency f directly. However, we do know the maximum speed of the electrons, so we can compute Kmax from classical mechanics. Then, because the stopping potential Vs is defined by Kmax=eVs (the electron’s charge times the voltage), we can solve for Vs directly — no need for the work function or photon energy at all in this step.
- Compute the maximum kinetic energy from the given speed. The maximum speed is vmax=8×105 m/s. The electron mass is m=9×10−31 kg.
Kmax=21mvmax2=21×(9×10−31)×(8×105)2
First square the speed: (8×105)2=64×1010=6.4×1011.
Then multiply:
21×9×10−31×6.4×1011=21×57.6×10−20=28.8×10−20 J
So Kmax=2.88×10−19 J.
- Relate kinetic energy to stopping potential. The stopping potential Vs is defined such that the work done by the electric field equals the maximum kinetic energy:
eVs=Kmax
where e=1.6×10−19 C.
Thus:
Vs=eKmax=1.6×10−192.88×10−19=1.8 V
- Check consistency with the work function (optional). …
- TG EAPCET 2025Set eng-2025-05-04-AN1 markMCQQ.In a photoelectric experiment, the slope of the graph drawn between stopping potential along y-axis and frequency of incident radiation along x-axis is (Planck’s constant = 6.6×10−34 Js) (A) 2.42×1015 Js C−1 (B) 10.56×10−15 Js C−1 (C) 4.125×10−15 Js C−1 (D) 6.25×10−20 Js C−1
›Reveal solutionSolution
The slope of the stopping potential vs. frequency graph is Planck’s constant divided by the elementary charge, giving 4.125×10−15 Js C−1, so the correct option is (C).
The key idea here is the photoelectric equation:
eV0=hf−ϕ
where V0 is the stopping potential, f is the frequency, h is Planck’s constant, e is the electron charge, and ϕ is the work function.
If you plot V0 (y-axis) against f (x-axis), the equation becomes
V0=ehf−eϕ
which is a straight line of the form y=mx+c.
The slope m is therefore eh.
We are given h=6.6×10−34 Js, and the elementary charge e=1.6×10−19 C (a standard constant you must recall).
-
Identify the slope from the equation
From V0=ehf−eϕ, the slope is eh.
No other quantity affects the slope — the work function only shifts the intercept.
-
Plug in the numbers
slope=1.6×10−196.6×10−34 Js C−1
- Perform the division
1.66.6=4.125
and for the powers of ten:
10−1910−34=10−15
So the slope is 4.125×10−15 Js C−1. …
-
- TG EAPCET 2025Set eng-2025-05-04-FN1 markMCQQ.In a photoelectric experiment, the slope of the graph drawn between stopping potential along y-axis and frequency of incident radiation along x-axis is (Planck’s constant = 6.6×10−34 Js) (A) 6.25×10−20 JsC−1 (B) 10.56×10−15 JsC−1 (C) 4.125×10−15 JsC−1 (D) 2.42×1015 JsC−1
›Reveal solutionSolution
The slope of the stopping potential vs. frequency graph is Planck’s constant divided by the elementary charge, h/e. Using h=6.6×10−34 Js and e=1.6×10−19 C, the slope is 4.125×10−15 JsC−1, which corresponds to option (C).
The key concept here is the photoelectric equation:
eV0=hf−ϕ
where V0 is the stopping potential, f is the frequency of incident light, h is Planck’s constant, e is the elementary charge, and ϕ is the work function. Rearranging:
V0=ehf−eϕ
This is a straight line of the form y=mx+c, with y=V0, x=f, slope m=h/e, and intercept c=−ϕ/e. So the slope of the graph is simply h/e, independent of the material.
Now, let’s compute it step by step.
-
Identify the known constants
Planck’s constant: h=6.6×10−34 Js
Elementary charge: e=1.6×10−19 C (standard value, since not given explicitly but implied by the units in the options).
-
Write the slope expression
Slope =eh=1.6×10−196.6×10−34 JsC−1
-
Perform the division
First, divide the numbers: 6.6/1.6=4.125
Then, divide the powers of ten: 10−34/10−19=10−15
So slope =4.125×10−15 JsC−1
-
Match with the options …
-
- TG EAPCET 2024Set eng-2024-05-09-FN1 markMCQQ.If Planck’s constant is 6.63×10−34 Js, then the slope of a graph drawn between cut off voltage and frequency of incident light in a photoelectric experiment is (A) 4.14×10−15 Vs (B) 19.776×10−15 Vs (C) 2.198×10−15 Vs (D) 1.337×10−15 Vs
›Reveal solutionSolution
The slope of the cut‑off voltage vs. frequency graph equals Planck’s constant divided by the electron charge, h/e. Using h=6.63×10−34 Js and e=1.6×10−19 C, the slope is 4.14×10−15 Vs, which matches option (A).
The key idea comes from Einstein’s photoelectric equation:
eV0=hf−ϕ
Here V0 is the cut‑off (stopping) voltage, f is the frequency of incident light, h is Planck’s constant, e is the electron charge, and ϕ is the work function of the metal. Rearranging:
V0=ehf−eϕ
This is a straight line of the form y=mx+c when we plot V0 (on the y‑axis) against f (on the x‑axis). The slope m is therefore h/e, a universal constant independent of the metal. So we just need to compute h/e with the given h.
-
Identify the slope
From V0=ehf−eϕ, the slope is eh.
-
Write down the given constants
- Planck’s constant: h=6.63×10−34 J⋅s
- Electron charge: e=1.6×10−19 C (standard value; not given but essential)
-
Compute the slope
eh=1.6×10−196.63×10−34=1.66.63×10−15
1.66.63=4.14375≈4.14 …
-
- TG EAPCET 2024Set eng-2024-05-11-FN1 markMCQQ.The work functions of two photosensitive metal surfaces A and B are in the ratio 2:3. If x and y are the slopes of the graphs drawn between the stopping potential and frequency of incident light for the surfaces A and B respectively, then x : y = (A) 1 : 1 (B) 2 : 3 (C) 4 : 9 (D) 2 : 5
›Reveal solutionSolution
The slope of the stopping potential vs. frequency graph is always h/e (Planck’s constant divided by electron charge), independent of the work function. Therefore the ratio of slopes for any two surfaces is 1:1.
Concept & Intuition
The photoelectric effect equation is eVs=hf−ϕ, where Vs is the stopping potential, f the frequency, ϕ the work function, h Planck’s constant, and e the electron charge. Rearranging:
Vs=ehf−eϕ.
This is a straight line with slope h/e and intercept −ϕ/e. The slope depends only on fundamental constants h and e, not on the metal’s work function. So no matter what the work functions are, the slopes of the Vs-vs-f graphs are identical for all photosensitive surfaces.
Step-by-step reasoning
- Write the photoelectric equation in linear form The stopping potential Vs satisfies
eVs=hf−ϕ⇒Vs=ehf−eϕ.
This is of the form y=mx+c with x=f, y=Vs.
- Identify the slope The slope m is the coefficient of f:
m=eh.
It contains only Planck’s constant h and the elementary charge e — both universal constants.
- Apply to surfaces A and B For surface A, slope x=h/e. …
- TG EAPCET 2023Set ap-2023-05-11-AN1 markMCQQ.When light radiation of frequency 6.97×1014 Hz is incident on a metal surface, then the electrons are ejected from the surface with a maximum speed of 6.6×105 ms−1. The threshold frequency of the metal surface is (take h=6.6×10−34 Js; mass of electron =9×10−31 kg) (A) 5×1014 Hz (B) 4×1014 Hz (C) 3×1014 Hz (D) 1×1014 Hz
›Reveal solutionSolution
The photoelectric equation links the incident photon energy to the electron’s kinetic energy and the work function. Using the given data, the threshold frequency comes out to be 4×1014 Hz, which is option (B).
The core idea here is Einstein’s photoelectric equation. When a photon strikes a metal surface, its energy is used first to overcome the binding energy (the work function) of the electron, and any leftover energy becomes the electron’s kinetic energy. The threshold frequency is the minimum frequency needed to just eject an electron — at that frequency, the kinetic energy is zero.
We are given the incident frequency, the maximum speed of the ejected electrons, and the constants. So we can compute the kinetic energy, subtract it from the incident photon energy, and find the work function. From the work function, the threshold frequency follows directly.
- Write Einstein’s photoelectric equation The energy of an incident photon is hν. Part of it goes into the work function ϕ=hν0 (where ν0 is the threshold frequency), and the rest becomes the maximum kinetic energy of the ejected electron:
hν=hν0+21mvmax2
-
Plug in the given numbers
- h=6.6×10−34 Js
- ν=6.97×1014 Hz
- m=9×10−31 kg
- vmax=6.6×105 m/s
First, the incident photon energy:
hν=(6.6×10−34)(6.97×1014)=4.6002×10−19 J
Next, the maximum kinetic energy:
21mvmax2=21(9×10−31)(6.6×105)2
Compute vmax2=(6.6×105)2=4.356×1011 …
- TG EAPCET 2023Set eng-2023-05-13-AN1 markMCQQ.A photon released by the transition of an electron from the second excited state to the ground state of Hydrogen atom is incident on the surface of a metal of work function 3.1 eV. The de Broglie wavelength of the most energetic electron emitted from that metal surface is nearly (A) 2.6A˚ (B) 4A˚ (C) 6A˚ (D) 7A˚
›Reveal solutionSolution
The key idea is to find the kinetic energy of the most energetic photoelectron by subtracting the work function from the photon energy (which comes from the hydrogen transition), then use the de Broglie relation to get its wavelength. The result is about 4 Å, so option (B) is correct.
Concept & Intuition
This problem combines two classic ideas:
- Atomic transitions in hydrogen — the photon energy equals the difference between two energy levels.
- Photoelectric effect — the maximum kinetic energy of an emitted electron is Kmax=hf−ϕ, where ϕ is the work function. Then, for that most energetic electron, we find its de Broglie wavelength: λ=h/p, and since the electron is non‑relativistic here, p=2meK.
The trick is to keep units consistent (eV, Å, etc.) and to remember that the “second excited state” means n=3 (ground is n=1).
Step‑by‑step solution
- Identify the hydrogen transition The ground state is n=1. The second excited state is n=3 (first excited is n=2). The energy levels of hydrogen are
En=−n213.6 eV.
So
E1=−13.6 eV,E3=−913.6 eV≈−1.51 eV.
- Photon energy from the transition The photon energy is the difference:
Ephoton=E3−E1=(−1.51)−(−13.6)=12.09 eV.
(More precisely, 13.6×(1−1/9)=13.6×8/9≈12.09 eV.)
- Maximum kinetic energy of the photoelectron The work function of the metal is ϕ=3.1 eV. By Einstein’s photoelectric equation:
Kmax=Ephoton−ϕ=12.09−3.1=8.99 eV≈9.0 eV.
- Convert kinetic energy to joules 1 eV=1.602×10−19 J, so
K=9.0×1.602×10−19≈1.442×10−18 J.
- Find the electron’s momentum For a non‑relativistic electron (9 eV is tiny compared to its rest energy 511 keV),
p=2meK,
with me=9.11×10−31 kg.
p=2×9.11×10−31×1.442×10−18≈2.627×10−48…
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