Wavelength of a proton or a neutron, λ ≈ 10-15 m Rest mass energy of an electron: moc2 = 0.511 MeV = 0.511 x 106x 1.6 x 10⁻19 = 0.8176 x 10⁻13 J Planck's constant, h = 6.6 x 10⁻34Js Speed of light, c = 3x 10s m/s The momentum of a proton or a neutron is given as: p=h/λ = (6.6 x 10⁻34)/ 10-15 = 6.6 xRead more
Wavelength of a proton or a neutron, λ ≈ 10-15 m
Rest mass energy of an electron:
moc2 = 0.511 MeV = 0.511 x 106x 1.6 x 10⁻19 = 0.8176 x 10⁻13 J
Planck’s constant, h = 6.6 x 10⁻34Js
Speed of light, c = 3x 10s m/s
The momentum of a proton or a neutron is given as:
p=h/λ = (6.6 x 10⁻34)/ 10-15
= 6.6 x 10⁻19 kg m/s
The relativistic relation for energy (E) is given as:
E = p²c² + m²oc⁴
= (6.6 x 10⁻19 x 3 x 10⁸ )²+ (0.8176 x 10⁻13)²= 392.04 x 10⁻²² + 0.6685 x 10⁻²6
≈392.04 x 10⁻²²
Therefore ,E = 1.98 x 10⁻¹⁰
= ( 1.98 x 10⁻¹⁰ )/(1.6 x 10⁻19) = 1.24 x 10⁹ eV
= 1.24 BeV
Thus, the electron energy emitted from the accelerator at Stanford, USA might be of the order of 1.24 BeV.
Electrons are accelerated by a voltage, V = 50 kV = 50 x 103 V Charge on an electron, e = 1.6 x 10-19 C Mass of an electron, me = 9.11 x 10⁻31 kg Wavelength of yellow light = 5.9 x 10⁻7 m The kinetic energy of the electron is given as: E = eV = 1.6 x 10⁻¹⁹ x 50 x 103 = 8 x 10⁻15 J De Broglie wavelenRead more
Electrons are accelerated by a voltage, V = 50 kV = 50 x 103 V
Charge on an electron, e = 1.6 x 10-19 C
Mass of an electron, me = 9.11 x 10⁻31 kg
Wavelength of yellow light = 5.9 x 10⁻7 m
The kinetic energy of the electron is given as:
E = eV = 1.6 x 10⁻¹⁹ x 50 x 103 = 8 x 10⁻15 J
De Broglie wavelength is given by the relation:
λ = h/√[2meE] = (6.6 x 10⁻34) /√[2 x 9.11 x 10⁻31x 8 x 10⁻15]
= 5.467 x 10⁻¹² m
This wavelength is nearly 105 times less than the wavelength of yellow light.
The resolving power of a microscope is inversely proportional to the wavelength of light used.
Thus, the resolving power of an electron microscope is nearly 105 times that of an optical microscope.
Ans (a). De Broglie wavelength = 2.327 x 10-12 m; neutron is not suitable for the diffraction experiment Kinetic energy of the neutron, K = 150 eV = 150 x 1.6 x 10-19 = 2.4 x 10-17 J Mass of a neutron ,mn=1.675 x 10-27 kg The kinetic energy of the neutron is given by the relation: K = 1/2 mnv2 =>Read more
Ans (a).
De Broglie wavelength = 2.327 x 10-12 m; neutron is not suitable for the diffraction experiment
Kinetic energy of the neutron, K = 150 eV = 150 x 1.6 x 10-19 = 2.4 x 10-17 J
Mass of a neutron ,mn=1.675 x 10-27 kg
The kinetic energy of the neutron is given by the relation:
K = 1/2 mnv2
=> mnv = √(2Kmn)
Where,v = Velocity of the neutron
mnv = Momentum of the neutron
De-Broglie wavelength of the neutron is given as:
λ =h/mnv = h/√(2Kmn)
It is clear that wavelength is inversely proportional to the square root of mass.
Hence. wavelength decreases with increase in mass and vice versa.
λ = (6.6 x 10⁻34)/√ [2(2.4 x 10-17)(1.675 x 10-27)]
= 2.327 x 10⁻¹² m
It is given in the previous problem that the inter-atomic spacing of a crystal is about 1 Aº, i.e., 10-10 m. Hence, the inter-atomic spacing is about a hundred times greater. Hence, a neutron beam of energy 150 eV is not suitable for diffraction experiments.
Ans (b).
De Broglie wavelength = 1.447 x 10-10 m
Room temperature, T = 27°C = 27 + 273 = 300 K
The average kinetic energy of the neutron is given as:
E= 3/2 kT
Where, k = Boltzmann constant = 1.38 x 10⁻23 J mol-1 K⁻1 The wavelength of the neutron is given as:
λ = h/√(2Emn) = h/√(3KmnT )
= (6.6 x 10⁻34)/√[3 x (1.675 x 10⁻27 )x (1.38 x 10⁻23 )x 300]
= 1.447 x 10⁻10 m
This wavelength is comparable to the inter-atomic spacing of a crystal. Hence, the high energy neutron beam should first be thermalised, before using it for diffraction.
An X-ray probe has a greater energy than an electron probe for the same wavelength. Wavelength of light emitted from the probe, λ = 1 Aº = 10⁻¹⁰ m Mass of an electron, me = 9.11 x 10-31 kg Planck's constant, h = 6.6 x 10⁻34 Js Charge on an electron, e = 1.6 x 10-19 C The kinetic energy of the electrRead more
An X-ray probe has a greater energy than an electron probe for the same wavelength.
Wavelength of light emitted from the probe, λ = 1 Aº = 10⁻¹⁰ m
Mass of an electron, me = 9.11 x 10-31 kg
Planck’s constant, h = 6.6 x 10⁻34 Js
Charge on an electron, e = 1.6 x 10-19 C
The kinetic energy of the electron is given as:
E = 1/2 mev²
=>mev = √ (2Eme)
Where,
v = Velocity of the electron
mev = Momentum (p) of the electron
According to the de Broglie principle, the de Broglie wavelength is given as:
λ = h/p = h/mev = h/√ (2Eme)
Therefore , E = h²/(2λ²me) 2
= (6.6 x 10⁻34)² /2 x ( 10⁻¹⁰)² x(9.11 x 10-31 ) = 2.39 x 10⁻¹⁷ J
= ( 2.39 x 10⁻¹⁷ )/(1.6 x 10-19) = 149 .375 eV
Energy of a photon,E’ =hc/λ e eV
= (6.6 x 10⁻34) x (3 x 10⁸ ) /( 10⁻¹⁰) (1.6 x 10-19)
= 12.375 x 10³ eV =12.375 keV
Hence, a photon has a greater energy than an electron for the same wavelength.
Intensity of incident light, I = 10-5 W m⁻2 Surface area of a sodium photocell, A = 2 cm2 = 2 x 10-4 m2 and incident power of the light, P = I x A = 10⁻5 x 2 x 10-4 = 2 x 10-9 W Work function of the metal, φO = 2 eV = 2 x 1.6 x 10-19 = 3.2 x 10-19 J Number of layers of sodium that absorbs the incideRead more
Intensity of incident light, I = 10-5 W m⁻2
Surface area of a sodium photocell, A = 2 cm2 = 2 x 10-4 m2
and incident power of the light, P = I x A = 10⁻5 x 2 x 10-4 = 2 x 10-9 W
Work function of the metal, φO = 2 eV = 2 x 1.6 x 10-19 = 3.2 x 10–19 J
Number of layers of sodium that absorbs the incident energy, n = 5
We know that the effective atomic area of a sodium atom, Ae is 10-20 m2.
Hence, the number of conduction electrons in n layers is given as:
n’ = n x A/Ae = 5 x (2 x 10-4) /(10-20) = 10¹⁷
The incident power is uniformly absorbed by all the electrons continuously. Hence, the amount of energy absorbed per second per electron is:
E = P/n’
= 5 x (2 x 10-9)/(10¹⁷) = 2 x 10⁻²⁶ J/s
Time required for photoelectric emission:
t = φO/E = (3.2 x 10–19) /( 2 x 10⁻²⁶)
=1.6 x 107 s ≈ 0.507 years
The time required for the photoelectric emission is nearly half a year, which is not practical. Hence, the wave picture is in disagreement with the given experiment.
Mo and Ni will not show photoelectric emission in both cases Wavelength for a radiation, λ = 3300 Aº = 3300 x 10⁻10 m and Speed of light, c = 3 x 108 m/s Planck’s constant, h = 6.6 x 10-34Js The energy of incident radiation is given as: E = hc/ λ = (6.6 x 10-34) x ( 3 x 10⁸)/(3300 x 10⁻10) = 6 x 10⁻Read more
Mo and Ni will not show photoelectric emission in both cases
Wavelength for a radiation, λ = 3300 Aº = 3300 x 10⁻10 m and Speed of light, c = 3 x 108 m/s
Planck’s constant, h = 6.6 x 10-34Js
The energy of incident radiation is given as:
E = hc/ λ = (6.6 x 10-34) x ( 3 x 10⁸)/(3300 x 10⁻10)
= 6 x 10⁻¹⁹J
= (6 x 10⁻¹⁹) /(1.6 x 10⁻¹⁹)
= 3.158 eV
It can be observed that the energy of the incident radiation is greater than the work function of Na and K only. It is less for Mo and Ni. Hence, Mo and Ni will not show photoelectric emission.
If the source of light is brought near the photocells and placed 50 cm away from them, then the intensity of radiation will increase. This does not affect the energy of the radiation. Hence, the result will be the same as before. However, the photoelectrons emitted from Na and K will increase in proportion to intensity.
Wavelength of the monochromatic radiation, λ = 640.2 nm = 640.2 x 10⁻9 m Stopping potential of the neon lamp, Vo = 0.54 V Charge on an electron, e = 1.6 x 10⁻19 C Planck's constant, h = 6.6 x 10-34 Js Let φO be the work function and v be the frequency of emitted light. We have the photo-energy relatRead more
Wavelength of the monochromatic radiation,
λ = 640.2 nm = 640.2 x 10⁻9 m
Stopping potential of the neon lamp, Vo = 0.54 V
Charge on an electron, e = 1.6 x 10⁻19 C
Planck’s constant, h = 6.6 x 10-34 Js
Let φO be the work function and v be the frequency of emitted light.
We have the photo-energy relation from the photoelectric effect as: eV0 = hv — φO,
φO = hc/λ – eV0
= ( 6.6 x 10-34) x ( 3 x 10⁸ ) /( 640.2 x 10⁻9) – (1.6 x 10⁻19) x 0.54
= 3.093 x 10⁻19 -0.864 x 10⁻19= 2.229 x10⁻19 J
= (2.229 x10⁻19) /(1.6 x 10⁻19) = 1.39 eV
Wavelength of the radiation emitted from an iron source,
λ’ = 427.2 nm = 427.2 x 10-9 m
Let V0 be the new stopping potential. Hence, photo-energy is given as:
eV0′ = hc/λ’- φO
=(6.6 x 10-34) x (3 x 10⁸ ) /(427.2 x 10-9) – (2.229 x10⁻19)n
Wavelength of ultraviolet light, λ = 2271 Aº = 2271 x 10⁻10 m Stopping potential of the metal, Vo = 1.3 V Planck's constant, h = 6.6 x 10⁻34 J Charge on an electron, e = 1.6 x 10-19 C Work function of the metal = φO Frequency of light = v We have the photo-energy relation from the photoelectric effeRead more
Wavelength of ultraviolet light, λ = 2271 Aº = 2271 x 10⁻10 m
Stopping potential of the metal, Vo = 1.3 V
Planck’s constant, h = 6.6 x 10⁻34 J
Charge on an electron, e = 1.6 x 10-19 C
Work function of the metal = φO
Frequency of light = v
We have the photo-energy relation from the photoelectric effect as:
φO= hv – eVo
= (6.6 x 10⁻34) x ( 3 x 10⁸ ) /(2271 x 10⁻10) – ( 1.6 x 10-19) x 1.3
= 8.72 x 10-19 – 2.08 x 10-19
= 6.64 x 10-19 J
= (6.64 x 10-19 ) /(1.6 x 10-19) = 4.15 eV
Let vo be the threshold frequency of the metal .Therefore , φO=hv0
=>v0 = φO/h = (6.64 x 10-19)/(6.6 x 10⁻34) = 1.006 x 10¹⁵ Hz
Wavelength of red light,
λr = 6328 Aº = 6328 x 10⁻10
Therefore ,the frequency of red light ,
vr = c/λr = (3 x 10⁸) /(6328 x 10⁻10) = 4.74 x 10¹4 Hz
Since vo> vr, the photocell will not respond to the red light produced by the laser.
Ans (a) . Power of the medium wave transmitter, P = 10 kW = 104W = 104 J/s Hence, energy emitted by the transmitter per second, E = 104 and wavelength of the radio wave, λ= 500 m The energy of the wave is given as: E₁ = hc/λ Where, h = Planck’s constant = 6.6 x 10⁻34 Js and c = Speed of light = 3 xRead more
Ans (a) .
Power of the medium wave transmitter, P = 10 kW = 104W = 104 J/s
Hence, energy emitted by the transmitter per second, E = 104 and
wavelength of the radio wave, λ= 500 m
The energy of the wave is given as:
E₁ = hc/λ
Where, h = Planck’s constant = 6.6 x 10⁻34 Js and c = Speed of light = 3 x 10⁸ m/s
Therefore, E₁ = (6.6 x 10⁻34) x (3 x 10⁸) /(500) = 3.96 x 10⁻²⁸ J
Let n be the number of photons emitted by the transmitter.
Therefore , nE₁ = E
n = E/E₁
= 10⁴/(3.96 x 10⁻²⁸ ) = 2.525 x 10³¹
≈ 3 x 10³¹
The energy (E1) of a radio photon is very less, but the number of photons (n) emitted per second in a radio wave is very large.
The existence of a minimum quantum of energy can be ignored and the total energy of a radio wave can be treated as being continuous.
Ans (b).
Intensity of light perceived by the human eye, I = 10⁻10 W m-2
Area of a pupil, A = 0.4 cm2 = 0.4 * 10⁻4 m2
Frequency of white light, v= 6 x 1014 Hz
The energy emitted by a photon is given as:
E = hv Where,
h = Planck’s constant = 6.6 x 10-34 Js
Therefore, E = 6.6 x 10-34 x 6 x 1014 = 3.96 x 10⁻19 J
Let n be the total number of photons falling per second, per unit area of the pupil.
The total energy per unit for n falling photons is given as:
E = n x 3.96 x 10-19 J s⁻1 m⁻²
The energy per unit area per second is the intensity of light.
Therefore, E = I
n x 3.96 x 10–19 = 10–10
n =10–10/3.96 x 10–19
= 2.52 x 108 m2 s–1
The total number of photons entering the pupil per second is given as:
nA = n x A = 2.52 x 108 x 0.4 x 10–4 = 1.008 x 104 s–1
This number is not as large as the one found in problem (a), but it is large enough for the human eye to never see the individual photons.
Total energy of two y-rays: E = 10. 2 BeV = 10.2 x 109 eV = 10.2 x 109 x 1.6 x 10⁻¹⁹ J Hence, the energy of each γ-ray: E' = E/2 = (10.2 x 10⁻¹⁰)/2 = 8.16 x 10⁻¹⁰ J Planck’s constant, h = 6.626 x 10 ⁻³4 Js Speed of light, c = 3 x 10⁸ m/s Energy is related to wavelength as: E' = hc/λ Therefore , λ =Read more
Total energy of two y-rays: E = 10. 2 BeV = 10.2 x 109 eV = 10.2 x 109 x 1.6 x 10⁻¹⁹ J
Hence, the energy of each γ-ray:
E’ = E/2 = (10.2 x 10⁻¹⁰)/2 = 8.16 x 10⁻¹⁰ J
Planck’s constant, h = 6.626 x 10 ⁻³4 Js
Speed of light, c = 3 x 10⁸ m/s
Energy is related to wavelength as:
E’ = hc/λ
Therefore , λ = hc/E’
= (6.626 x 10⁻34 x 3 x 10⁸)/( 8.16 x 10⁻¹⁰)
= 2.436 x 10-16 m
Therefore, the wavelength associated with each γ-ray is 2.436 x 10-16 m.
The wavelength of a probe is roughly a measure of the size of a structure that it can probe in some detail. The quark structure of protons and neutrons appears at the minute length-scale of 10⁻¹⁵ m or less. This structure was first probed in early 1970’s using high energy electron beams produced by a linear accelerator at Stanford, USA. Guess what might have been the order of energy of these electron beams. (Rest mass energy of electron = 0.511 MeV.)
Wavelength of a proton or a neutron, λ ≈ 10-15 m Rest mass energy of an electron: moc2 = 0.511 MeV = 0.511 x 106x 1.6 x 10⁻19 = 0.8176 x 10⁻13 J Planck's constant, h = 6.6 x 10⁻34Js Speed of light, c = 3x 10s m/s The momentum of a proton or a neutron is given as: p=h/λ = (6.6 x 10⁻34)/ 10-15 = 6.6 xRead more
Wavelength of a proton or a neutron, λ ≈ 10-15 m
Rest mass energy of an electron:
moc2 = 0.511 MeV = 0.511 x 106x 1.6 x 10⁻19 = 0.8176 x 10⁻13 J
Planck’s constant, h = 6.6 x 10⁻34Js
Speed of light, c = 3x 10s m/s
The momentum of a proton or a neutron is given as:
p=h/λ = (6.6 x 10⁻34)/ 10-15
= 6.6 x 10⁻19 kg m/s
The relativistic relation for energy (E) is given as:
E = p²c² + m²oc⁴
= (6.6 x 10⁻19 x 3 x 10⁸ )²+ (0.8176 x 10⁻13)² = 392.04 x 10⁻²² + 0.6685 x 10⁻²6
≈392.04 x 10⁻²²
Therefore ,E = 1.98 x 10⁻¹⁰
= ( 1.98 x 10⁻¹⁰ )/(1.6 x 10⁻19) = 1.24 x 10⁹ eV
= 1.24 BeV
Thus, the electron energy emitted from the accelerator at Stanford, USA might be of the order of 1.24 BeV.
See lessAn electron microscope uses electrons accelerated by a voltage of 50 kV. Determine the de Broglie wavelength associated with the electrons. If other factors (such as numerical aperture, etc.) are taken to be roughly the same, how does the resolving power of an electron microscope compare with that of an optical microscope which uses yellow light?
Electrons are accelerated by a voltage, V = 50 kV = 50 x 103 V Charge on an electron, e = 1.6 x 10-19 C Mass of an electron, me = 9.11 x 10⁻31 kg Wavelength of yellow light = 5.9 x 10⁻7 m The kinetic energy of the electron is given as: E = eV = 1.6 x 10⁻¹⁹ x 50 x 103 = 8 x 10⁻15 J De Broglie wavelenRead more
Electrons are accelerated by a voltage, V = 50 kV = 50 x 103 V
Charge on an electron, e = 1.6 x 10-19 C
Mass of an electron, me = 9.11 x 10⁻31 kg
Wavelength of yellow light = 5.9 x 10⁻7 m
The kinetic energy of the electron is given as:
E = eV = 1.6 x 10⁻¹⁹ x 50 x 103 = 8 x 10⁻15 J
De Broglie wavelength is given by the relation:
λ = h/√[2meE] = (6.6 x 10⁻34) /√[2 x 9.11 x 10⁻31x 8 x 10⁻15]
= 5.467 x 10⁻¹² m
This wavelength is nearly 105 times less than the wavelength of yellow light.
The resolving power of a microscope is inversely proportional to the wavelength of light used.
Thus, the resolving power of an electron microscope is nearly 105 times that of an optical microscope.
See less(a) Obtain the de Broglie wavelength of a neutron of kinetic energy 150 eV. As you have seen in Exercise 11.31, an electron beam of this energy is suitable for crystal diffraction experiments. Would a neutron beam of the same energy be equally suitable? Explain. (mn = 1.675 × 10⁻²⁷ kg) (b) Obtain the de Broglie wavelength associated with thermal neutrons at room temperature (27 ºC). Hence explain why a fast neutron beam needs to be thermalised with the environment before it can be used for neutron diffraction experiments.
Ans (a). De Broglie wavelength = 2.327 x 10-12 m; neutron is not suitable for the diffraction experiment Kinetic energy of the neutron, K = 150 eV = 150 x 1.6 x 10-19 = 2.4 x 10-17 J Mass of a neutron ,mn=1.675 x 10-27 kg The kinetic energy of the neutron is given by the relation: K = 1/2 mnv2 =>Read more
Ans (a).
De Broglie wavelength = 2.327 x 10-12 m; neutron is not suitable for the diffraction experiment
Kinetic energy of the neutron, K = 150 eV = 150 x 1.6 x 10-19 = 2.4 x 10-17 J
Mass of a neutron ,mn=1.675 x 10-27 kg
The kinetic energy of the neutron is given by the relation:
K = 1/2 mnv2
=> mnv = √(2Kmn)
Where,v = Velocity of the neutron
mnv = Momentum of the neutron
De-Broglie wavelength of the neutron is given as:
λ =h/mnv = h/√(2Kmn)
It is clear that wavelength is inversely proportional to the square root of mass.
Hence. wavelength decreases with increase in mass and vice versa.
λ = (6.6 x 10⁻34)/√ [2(2.4 x 10-17)(1.675 x 10-27)]
= 2.327 x 10⁻¹² m
It is given in the previous problem that the inter-atomic spacing of a crystal is about 1 Aº, i.e., 10-10 m. Hence, the inter-atomic spacing is about a hundred times greater. Hence, a neutron beam of energy 150 eV is not suitable for diffraction experiments.
Ans (b).
De Broglie wavelength = 1.447 x 10-10 m
Room temperature, T = 27°C = 27 + 273 = 300 K
The average kinetic energy of the neutron is given as:
E= 3/2 kT
Where, k = Boltzmann constant = 1.38 x 10⁻23 J mol-1 K⁻1 The wavelength of the neutron is given as:
λ = h/√(2Emn) = h/√(3KmnT )
= (6.6 x 10⁻34)/√[3 x (1.675 x 10⁻27 )x (1.38 x 10⁻23 )x 300]
= 1.447 x 10⁻10 m
This wavelength is comparable to the inter-atomic spacing of a crystal. Hence, the high energy neutron beam should first be thermalised, before using it for diffraction.
See lessCrystal diffraction experiments can be performed using X-rays, or electrons accelerated through appropriate voltage. Which probe has greater energy? (For quantitative comparison, take the wavelength of the probe equal to 1 Å, which is of the order of inter-atomic spacing in the lattice) (me=9.11 × 10⁻³¹ kg).
An X-ray probe has a greater energy than an electron probe for the same wavelength. Wavelength of light emitted from the probe, λ = 1 Aº = 10⁻¹⁰ m Mass of an electron, me = 9.11 x 10-31 kg Planck's constant, h = 6.6 x 10⁻34 Js Charge on an electron, e = 1.6 x 10-19 C The kinetic energy of the electrRead more
An X-ray probe has a greater energy than an electron probe for the same wavelength.
Wavelength of light emitted from the probe, λ = 1 Aº = 10⁻¹⁰ m
Mass of an electron, me = 9.11 x 10-31 kg
Planck’s constant, h = 6.6 x 10⁻34 Js
Charge on an electron, e = 1.6 x 10-19 C
The kinetic energy of the electron is given as:
E = 1/2 mev²
=>mev = √ (2Eme)
Where,
v = Velocity of the electron
mev = Momentum (p) of the electron
According to the de Broglie principle, the de Broglie wavelength is given as:
λ = h/p = h/mev = h/√ (2Eme)
Therefore , E = h²/(2λ²me) 2
= (6.6 x 10⁻34)² /2 x ( 10⁻¹⁰)² x(9.11 x 10-31 ) = 2.39 x 10⁻¹⁷ J
= ( 2.39 x 10⁻¹⁷ )/(1.6 x 10-19) = 149 .375 eV
Energy of a photon,E’ =hc/λ e eV
= (6.6 x 10⁻34) x (3 x 10⁸ ) /( 10⁻¹⁰) (1.6 x 10-19)
= 12.375 x 10³ eV =12.375 keV
Hence, a photon has a greater energy than an electron for the same wavelength.
Light of intensity 10⁻⁵ W m⁻² falls on a sodium photo-cell of surface area 2 cm² . Assuming that the top 5 layers of sodium absorb the incident energy, estimate time required for photoelectric emission in the wave-picture of radiation. The work function for the metal is given to be about 2 eV. What is the implication of your answer?
Intensity of incident light, I = 10-5 W m⁻2 Surface area of a sodium photocell, A = 2 cm2 = 2 x 10-4 m2 and incident power of the light, P = I x A = 10⁻5 x 2 x 10-4 = 2 x 10-9 W Work function of the metal, φO = 2 eV = 2 x 1.6 x 10-19 = 3.2 x 10-19 J Number of layers of sodium that absorbs the incideRead more
Intensity of incident light, I = 10-5 W m⁻2
Surface area of a sodium photocell, A = 2 cm2 = 2 x 10-4 m2
and incident power of the light, P = I x A = 10⁻5 x 2 x 10-4 = 2 x 10-9 W
Work function of the metal, φO = 2 eV = 2 x 1.6 x 10-19 = 3.2 x 10–19 J
Number of layers of sodium that absorbs the incident energy, n = 5
We know that the effective atomic area of a sodium atom, Ae is 10-20 m2.
Hence, the number of conduction electrons in n layers is given as:
n’ = n x A/Ae = 5 x (2 x 10-4) /(10-20) = 10¹⁷
The incident power is uniformly absorbed by all the electrons continuously. Hence, the amount of energy absorbed per second per electron is:
E = P/n’
= 5 x (2 x 10-9)/(10¹⁷) = 2 x 10⁻²⁶ J/s
Time required for photoelectric emission:
t = φO/E = (3.2 x 10–19) /( 2 x 10⁻²⁶)
=1.6 x 107 s ≈ 0.507 years
The time required for the photoelectric emission is nearly half a year, which is not practical. Hence, the wave picture is in disagreement with the given experiment.
See lessThe work function for the following metals is given: Na: 2.75 eV; K: 2.30 eV; Mo: 4.17 eV; Ni: 5.15 eV. Which of these metals will not give photoelectric emission for a radiation of wavelength 3300 Å from a He-Cd laser placed 1 m away from the photocell? What happens if the laser is brought nearer and placed 50 cm away?
Mo and Ni will not show photoelectric emission in both cases Wavelength for a radiation, λ = 3300 Aº = 3300 x 10⁻10 m and Speed of light, c = 3 x 108 m/s Planck’s constant, h = 6.6 x 10-34Js The energy of incident radiation is given as: E = hc/ λ = (6.6 x 10-34) x ( 3 x 10⁸)/(3300 x 10⁻10) = 6 x 10⁻Read more
Mo and Ni will not show photoelectric emission in both cases
Wavelength for a radiation, λ = 3300 Aº = 3300 x 10⁻10 m and Speed of light, c = 3 x 108 m/s
Planck’s constant, h = 6.6 x 10-34Js
The energy of incident radiation is given as:
E = hc/ λ = (6.6 x 10-34) x ( 3 x 10⁸)/(3300 x 10⁻10)
= 6 x 10⁻¹⁹J
= (6 x 10⁻¹⁹) /(1.6 x 10⁻¹⁹)
= 3.158 eV
It can be observed that the energy of the incident radiation is greater than the work function of Na and K only. It is less for Mo and Ni. Hence, Mo and Ni will not show photoelectric emission.
If the source of light is brought near the photocells and placed 50 cm away from them, then the intensity of radiation will increase. This does not affect the energy of the radiation. Hence, the result will be the same as before. However, the photoelectrons emitted from Na and K will increase in proportion to intensity.
See lessMonochromatic radiation of wavelength 640.2 nm (1nm = 10⁻⁹ m) from a neon lamp irradiates photosensitive material made of caesium on tungsten. The stopping voltage is measured to be 0.54 V. The source is replaced by an iron source and its 427.2 nm line irradiates the same photo-cell. Predict the new stopping voltage.
Wavelength of the monochromatic radiation, λ = 640.2 nm = 640.2 x 10⁻9 m Stopping potential of the neon lamp, Vo = 0.54 V Charge on an electron, e = 1.6 x 10⁻19 C Planck's constant, h = 6.6 x 10-34 Js Let φO be the work function and v be the frequency of emitted light. We have the photo-energy relatRead more
Wavelength of the monochromatic radiation,
λ = 640.2 nm = 640.2 x 10⁻9 m
Stopping potential of the neon lamp, Vo = 0.54 V
Charge on an electron, e = 1.6 x 10⁻19 C
Planck’s constant, h = 6.6 x 10-34 Js
Let φO be the work function and v be the frequency of emitted light.
We have the photo-energy relation from the photoelectric effect as: eV0 = hv — φO,
φO = hc/λ – eV0
= ( 6.6 x 10-34) x ( 3 x 10⁸ ) /( 640.2 x 10⁻9) – (1.6 x 10⁻19) x 0.54
= 3.093 x 10⁻19 -0.864 x 10⁻19 = 2.229 x10⁻19 J
= (2.229 x10⁻19) /(1.6 x 10⁻19) = 1.39 eV
Wavelength of the radiation emitted from an iron source,
λ’ = 427.2 nm = 427.2 x 10-9 m
Let V0 be the new stopping potential. Hence, photo-energy is given as:
eV0′ = hc/λ’- φO
=(6.6 x 10-34) x (3 x 10⁸ ) /(427.2 x 10-9) – (2.229 x10⁻19)n
= 4.63 x 10⁻19 – 2.229 x10⁻19
=2.401 x 10⁻19J
= (2.401 x 10⁻19)/(1.6 x x10⁻19) = 1.5eV
Hence, the new stopping potential is 1.50 eV.
See lessUltraviolet light of wavelength 2271 Å 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 Å produced by a He-Ne laser?
Wavelength of ultraviolet light, λ = 2271 Aº = 2271 x 10⁻10 m Stopping potential of the metal, Vo = 1.3 V Planck's constant, h = 6.6 x 10⁻34 J Charge on an electron, e = 1.6 x 10-19 C Work function of the metal = φO Frequency of light = v We have the photo-energy relation from the photoelectric effeRead more
Wavelength of ultraviolet light, λ = 2271 Aº = 2271 x 10⁻10 m
Stopping potential of the metal, Vo = 1.3 V
Planck’s constant, h = 6.6 x 10⁻34 J
Charge on an electron, e = 1.6 x 10-19 C
Work function of the metal = φO
Frequency of light = v
We have the photo-energy relation from the photoelectric effect as:
φO= hv – eVo
= (6.6 x 10⁻34) x ( 3 x 10⁸ ) /(2271 x 10⁻10) – ( 1.6 x 10-19) x 1.3
= 8.72 x 10-19 – 2.08 x 10-19
= 6.64 x 10-19 J
= (6.64 x 10-19 ) /(1.6 x 10-19) = 4.15 eV
Let vo be the threshold frequency of the metal .Therefore , φO=hv0
=>v0 = φO/h = (6.64 x 10-19)/(6.6 x 10⁻34) = 1.006 x 10¹⁵ Hz
Wavelength of red light,
λr = 6328 Aº = 6328 x 10⁻10
Therefore ,the frequency of red light ,
vr = c/λr = (3 x 10⁸) /(6328 x 10⁻10) = 4.74 x 10¹4 Hz
Since vo> vr, the photocell will not respond to the red light produced by the laser.
See lessEstimating the following two numbers should be interesting. The first number will tell you why radio engineers do not need to worry much about photons! The second number tells you why our eye can never ‘count photons’, even in barely detectable light. (a) The number of photons emitted per second by a Medium wave transmitter of 10 kW power, emitting radiowaves of wavelength 500 m. (b) The number of photons entering the pupil of our eye per second corresponding to the minimum intensity of white light that we humans can perceive (∼10⁻¹⁰ W m⁻²). Take the area of the pupil to be about 0.4 cm² , and the average frequency of white light to be about 6 × 10¹⁴ Hz.
Ans (a) . Power of the medium wave transmitter, P = 10 kW = 104W = 104 J/s Hence, energy emitted by the transmitter per second, E = 104 and wavelength of the radio wave, λ= 500 m The energy of the wave is given as: E₁ = hc/λ Where, h = Planck’s constant = 6.6 x 10⁻34 Js and c = Speed of light = 3 xRead more
Ans (a) .
Power of the medium wave transmitter, P = 10 kW = 104W = 104 J/s
Hence, energy emitted by the transmitter per second, E = 104 and
wavelength of the radio wave, λ= 500 m
The energy of the wave is given as:
E₁ = hc/λ
Where, h = Planck’s constant = 6.6 x 10⁻34 Js and c = Speed of light = 3 x 10⁸ m/s
Therefore, E₁ = (6.6 x 10⁻34) x (3 x 10⁸) /(500) = 3.96 x 10⁻²⁸ J
Let n be the number of photons emitted by the transmitter.
Therefore , nE₁ = E
n = E/E₁
= 10⁴/(3.96 x 10⁻²⁸ ) = 2.525 x 10³¹
≈ 3 x 10³¹
The energy (E1) of a radio photon is very less, but the number of photons (n) emitted per second in a radio wave is very large.
The existence of a minimum quantum of energy can be ignored and the total energy of a radio wave can be treated as being continuous.
Ans (b).
Intensity of light perceived by the human eye, I = 10⁻10 W m-2
Area of a pupil, A = 0.4 cm2 = 0.4 * 10⁻4 m2
Frequency of white light, v= 6 x 1014 Hz
The energy emitted by a photon is given as:
E = hv Where,
h = Planck’s constant = 6.6 x 10-34 Js
Therefore, E = 6.6 x 10-34 x 6 x 1014 = 3.96 x 10⁻19 J
Let n be the total number of photons falling per second, per unit area of the pupil.
The total energy per unit for n falling photons is given as:
E = n x 3.96 x 10-19 J s⁻1 m⁻²
The energy per unit area per second is the intensity of light.
Therefore, E = I
n x 3.96 x 10–19 = 10–10
n =10–10/3.96 x 10–19
= 2.52 x 108 m2 s–1
The total number of photons entering the pupil per second is given as:
nA = n x A = 2.52 x 108 x 0.4 x 10–4 = 1.008 x 104 s–1
This number is not as large as the one found in problem (a), but it is large enough for the human eye to never see the individual photons.
See lessIn an accelerator experiment on high-energy collisions of electrons with positrons, a certain event is interpreted as annihilation of an electron-positron pair of total energy 10.2 BeV into two γ-rays of equal energy. What is the wavelength associated with each γ-ray? (1BeV = 10⁹ eV)
Total energy of two y-rays: E = 10. 2 BeV = 10.2 x 109 eV = 10.2 x 109 x 1.6 x 10⁻¹⁹ J Hence, the energy of each γ-ray: E' = E/2 = (10.2 x 10⁻¹⁰)/2 = 8.16 x 10⁻¹⁰ J Planck’s constant, h = 6.626 x 10 ⁻³4 Js Speed of light, c = 3 x 10⁸ m/s Energy is related to wavelength as: E' = hc/λ Therefore , λ =Read more
Total energy of two y-rays: E = 10. 2 BeV = 10.2 x 109 eV = 10.2 x 109 x 1.6 x 10⁻¹⁹ J
Hence, the energy of each γ-ray:
E’ = E/2 = (10.2 x 10⁻¹⁰)/2 = 8.16 x 10⁻¹⁰ J
Planck’s constant, h = 6.626 x 10 ⁻³4 Js
Speed of light, c = 3 x 10⁸ m/s
Energy is related to wavelength as:
E’ = hc/λ
Therefore , λ = hc/E’
= (6.626 x 10⁻34 x 3 x 10⁸)/( 8.16 x 10⁻¹⁰)
= 2.436 x 10-16 m
Therefore, the wavelength associated with each γ-ray is 2.436 x 10-16 m.
See less