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# Solution - A Mercury Lamp is a Convenient Source for Studying Frequency Dependence of Photoelectric Emission, since It Gives a Number of Spectral Lines Ranging from the Uv to the Red End of the Visible Spectrum. in Our Experiment with Rubidium Photo-cell, the Following Lines from a Mercury Source Were Used: - Experimental Study of Photoelectric Effect

ConceptExperimental Study of Photoelectric Effect

#### Question

A mercury lamp is a convenient source for studying frequency dependence of photoelectric emission, since it gives a number of spectral lines ranging from the UV to the red end of the visible spectrum. In our experiment with rubidium photo-cell, the following lines from a mercury source were used:

λ1 = 3650 Å, λ2= 4047 Å, λ3= 4358 Å, λ4= 5461 Å, λ5= 6907 Å,

The stopping voltages, respectively, were measured to be:

V01 = 1.28 V, V02 = 0.95 V, V03 = 0.74 V, V04 = 0.16 V, V05 = 0 V

Determine the value of Planck’s constant h, the threshold frequency and work function for the material.

[Note: You will notice that to get from the data, you will need to know (which you can take to be 1.6 × 10−19 C). Experiments of this kind on Na, Li, K, etc. were performed by Millikan, who, using his own value of (from the oil-drop experiment) confirmed Einstein’s photoelectric equation and at the same time gave an independent estimate of the value of h.]

#### Solution

Einstein’s photoelectric equation is given as:

eV0 = hν− phi_0

V_0 = h/e v - phi_0/e  ...(1)

Where,

V0 = Stopping potential

h = Planck’s constant

e = Charge on an electron

phi_0 = Work function of a material

It can be concluded from equation (1) that potential V0 is directly proportional to frequency ν.

Frequency is also given by the relation:

v = "Speed of light (c)"/"Wavelenght (λ)"

This relation can be used to obtain the frequencies of the various lines of the given wavelengths.

v_1 = c/lambda_1 = (3xx 10^8)/(3650 xx 10^(-10)) = 8.219 xx 10^14 Hz

v_2 = c/lambda_2 = (3xx10^8)/(4047 xx 10^(-10)) = 7.412 xx 10^14 Hz

v_3 = c/lambda_3 = (3xx10^8)/(4358 xx 10^(-10)) = 6.884 xx 10^14 Hz

v_4 = c/lambda_4 = (3 xx 10^8)/(5461 xx 10^(-10)) = 5.493 xx 10^14 Hz

v_5 = c/lambda_5  = (3xx10^8)/(6907 xx 10^(-10)) = 4.343 xx 10^14 Hz

The given quantities can be listed in tabular form as:

0.16

 Frequency × 1014 Hz 8.219 7.412 6.884 5.493 4.343 Stopping potential V0 1.28 0.95 0.74 0.16 0

The following figure shows a graph between νand V0.

It can be observed that the obtained curve is a straight line. It intersects the ν-axis at 5 × 1014 Hz, which is the threshold frequency (ν0) of the material. Point D corresponds to a frequency less than the threshold frequency. Hence, there is no photoelectric emission for the λ5 line, and therefore, no stopping voltage is required to stop the current.

Slope of the straight line  = "AB"/"CB" = (1.28 - 0.16)/((8.214 - 5.493) xx 10^14)

From equation (1), the slope h/e can be written as:

h/e = (1.28 - 0.16)/((8.214 - 5.493) xx 10^14)

:. h = (1.12 xx 1.6 xx 10^(-19))/(2.726 xx 10^(14))

= 6.573 xx 10^(-34) Js

The work function of the metal is given as:

phi_0 = hν0

= 6.573 × 10−34 × 5 × 1014

= 3.286 × 10−19 J

=(3.286 xx 10^(-19))/(1.6 xx 1^(-18))= 2.054 eV

Is there an error in this question or solution?

#### APPEARS IN

NCERT Physics Textbook for Class 12 Part 2
Chapter 11: Dual Nature of Radiation and Matter
Q: 28 | Page no. 410

#### Reference Material

Solution for question: A Mercury Lamp is a Convenient Source for Studying Frequency Dependence of Photoelectric Emission, since It Gives a Number of Spectral Lines Ranging from the Uv to the Red End of the Visible Spectrum. in Our Experiment with Rubidium Photo-cell, the Following Lines from a Mercury Source Were Used: concept: Experimental Study of Photoelectric Effect. For the courses CBSE (Arts), CBSE (Commerce), CBSE (Science)
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