[Physics Class Notes] on Planck’s Constant Pdf for Exam

The energy was initially considered to be continuous. However, after a long research Max Planck came to the conclusion that the energy is not continuous in nature it is instead discrete and in small packets which are indicated by the small invisible particles called photons. These particles are the ones that carry the energy and this energy that has been carried is determined by Planck’s Constant. To know more about Planck’s Constant – value, Formula, Symbol, Applications, and Examples students can now check out more about the same via .

The energy that is released in the form of packets or chunks in a discontinuous manner is known as Photons where the energy of each photon is directly proportional to the frequency i.e. E and depends upon f.

                     E  ∝  f,   E = k x  h x u….(1)   (k is no of photons, and is an integer)

Here, ‘h’  is called the Planck’s constant.

On this page, we shall learn about the following:

  • Planck’s constant

  • Value of Planck’s constant

  • Deriving Planck’s constant formula in both MKS and CGS unit

  • Planck’s constant units and dimensional formula

  • Planck’s constant symbol

  • Applications of Planck’s constant with examples

  • Illustrative examples to understand the basics of this topic. 

What is Planck’s Quantum Theory all about?

A German theoretical physicist, Dr. Max Planck had put forth a theory known as Planck’s quantum theory. This theory states: Energy radiated or enwrapped is not perpetual, but in the form of packets called quanta. This energy is known as the “Quantum of energy.” For a single packet, we call it quanta, where quanta is an integer value, unlike continuous energy supply which has varying values: 1 or 1.1 or 1.2…

Packets are units of energy and they are called Quanta in general terms whereas Photons is a term used for packets in terms of visible light.

Consider this equation:

 E = h x c/λ….(2)

 h = 6.626 x 10⁻³⁴

 c = 3 x 10⁸ m/s

Put this value in the above equation(2)

(6.626 x 10⁻³⁴) * (3 x 10⁸)/λ

(19.878 x 10⁻²⁶)/λ  ∽   (2 x 10²⁵)/λ

We get,

M = (2 x 10²⁵)/λ

This is the value for energy of a single photon, and for ‘k’ no of photons, it would be:

The value of E is calculated only when wavelength, λ is given in meters. If λ is given in any other unit let’s say in Angstrom, simply, we can convert 1 Angstrom to meters (1 Angstrom = 10⁻¹⁰m) where h is the Planck’s constant, and h = Energy of a quantum of electromagnetic radiation divided by its frequency.

Planck’s constant ‘h’  is measured in Joule-seconds in the SI system.

       h  = 6.626 x 10⁻³⁴

and Electronvolt or (eV) in the M.K.S system.

1 eV  =  1.6 x 10⁻¹⁹ Joule 

E = (12400/λ) eV for λ in  Å. 

E = (1240/λ) eV for λ in nm.

 

Value for λ when E = 4.13 V 

E = 12400/λ

4.13 = 12400/λ

λ  = 12400/4.13 = 3000 Å

Experiments Used to determine Planck’s Constant:

There were two experiments that were used in order to determine the Planck constant and can be provided as follows:

1.Kibble Balance

2.X-ray crystal density method

  1. Kibble Balance:

It is the accurate weighing machine that was named after its inventor Bryan Kibble in 1975. It is designed to equalize one of the forces that arise with another. In this case, the weight of a test mass is exactly balanced out by a force that is induced when an electrical current is run through a coil of wire that has been immersed in a surrounding magnetic field.

  1. X-ray Crystal Density Method:

This method is a primary method that is used in the determination of Planck’s constant. Here crystals of silicon which are available in high quality and purity by the semiconductor industry are used.

What’s so Special about Planck’s Constant?

A blackbody is an idealized physical body, which assimilates all the electromagnetic radiation. Upon heating, it reflects the light falling on it, but that too of varying amounts of wavelengths.

(Image wil lbe Uploaded Soon)

(Image wil lbe Uploaded Soon)

Here in this graph, we can observe that less is the wavelength, lesser is the emission of waves, then a time comes when we get the maximum wavelength, Vmax, which means maximum emission.

The Vmax is the position shown as a peak in the graph is the visible light.

What happens here is when we go further, the wavelength keeps on increasing, but the emission of waves keeps on decreasing and continues further, we see that the emission of waves is negligible, but not zero. (All the wavelengths of whatever amount and irrespective of frequencies are radiated).

But from theoretical derivation, you must have observed in the curve that from the starting till the point when the wavelength is maximum, the graph shows symmetry, but what happens thereafter? The emission of waves is maximum even when the wavelength is less.

There’s a lot of difference when the wavelength is less. The modification in the above concept was brought up by a great German theoretical physicist, named Dr. Max Planck.

Where he considered light as a form of ‘k’ no of chunks or packets called photons by the relation.

E = k x h x f, k being the no of photons.

After his experimentation, the experimental and theoretical curves which were not symmetrical to each other, got into symmetry infers that the theory given by Dr. Planck was correct.

Summary

  • When an iron rod is heated, lights of all wavelengths are emitted, but a human eye can perceive only that light which is of maximum wavelength Vmax. 

  • We estimate the temperature of stars by observing the Vmax of the light emitted.

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