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 Multiple Choice QuestionsMultiple Choice Questions

151.

Assertion: In a metal all the free electrons have same energy.

Reason: : Electrons do not obey Pauli's Exclusion principle

  • If both assertion and reason are true and reason is the correct explanation of assertion

  • If both assertion and reason are true but reason is not the correct explanation of assertion

  • If assertion is true and reason is false

  • If both assertion and reason are false


152.

The ground state energy of hydrogen atom is -13.6 eV. What is the potential energy of the electron in the state?

  • 0 eV

  • -27.2 eV

  • 1 eV

  • 2 eV


153.

Energy required to break one bond in DNA is approximately

  • ∼ 1 eV

  • ∼ 0.1 eV

  • ∼ 0.01 eV

  • ∼ 2.1 eV


154.

Assertion: Bohr had to postulate that the electrons in stationary orbits around the nucleus do not radiate. 

Reason:  According to classical physics all moving electrons radiate.

  • if both assertion and reason are true and the reason is the correct explanation of the assertion

  • if both assertion and reason are true and the reason is not the correct explanation of the assertion

  • if assertion is true but reason is false

  • if both assertion and reason are false statements


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155.

Maximum energy is evolved during which of the following transitions?

  • n = 1 to n= 2

  • n = 2 to n= 6

  • n = 2 to n= 1

  • n = 6 to n= 2


156.

If λand λ2 are the wavelengths of the first members of the Lyman and Paschen series respectively, then λ1 : λ2 is

  • 1 : 3

  • 1 : 30

  • 7 : 50

  • 7 : 108


157.

Electrons in a certain energy level n = n1 can emit 3 spectral lines. When they are in another energy level, n=n2 they can emit 6 spectral lines. The orbital speed of the electrons in the orbits are in the ratio

  • 4 : 3

  • 3 : 4

  • 2 : 1

  • 1 : 2


158.

The ground state energy of H-atom is 13.6 eV. The energy needed to ionize H-atom from its second excited state is

  • 1.51 eV

  • 3.4 eV

  • 13.6 eV

  • 12.1 eV


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159.

Continuous emission spectrum, emitted wavelength about spectrum, the range depends upon:

  • temperature of the source

  • material of the source

  • surface area of the source

  • all of the above


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160.

If the temperature of a black body is doubled, the wavelength at which the spectral radiancy has its maximum, is 

  • doubled

  • halved

  • quadrupled

  • unchanged


B.

halved

From Wein's displacement law,

        λmT = constant 

    λmT  =  λ'mT

    λ'm  =  λmTT'

    λ'm  =  λmT2T

    λ'm  =  λm2

Hence, wavelength will be halved.


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