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21.

If alpha particle, proton and electron move with the same momentum, then their respective de-Broglie wavelengths λα, λp, λe are related

  • λα = λp = λe

  • λα < λp < λe

  • λα > λp > λe

  • λp > λe > λα


22.

The velocity of a moving galaxy is 300 kms-1 and the apparent change in wavelength of a spectral line emitted from the galaxy is observed as 0.5 nm. Then, the actual wavelength of the spectral line is

  • 3000 A

  • 5000 A

  • 6000 A

  • 4500 A


23.

The temperature at which protons in proton gas would have enough energy to overcome Coulomb barrier of 4.14 x 10-14 J is (Boltzmann constant = 1.38 x 10-23 JK-1)

  • 2 × 109 K

  • 109 K

  • 6 × 109 K

  • 3 × 109 K


24.

The surface area ofa black body is 5 x 10-4 m2 and its temperature is 727°C. The energy radiated by it per minute is (σ = 5.67 × 10-8 J/m2 s-k4)

  • 1.7 × 103 J

  • 2.5 × 102 J

  • 8 × 103 J

  • 3 × 104 J


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25.

The ratio of the de-Broglie wavelength of an α-particle and a proton of same kinetic energy is

  • 1 : 2

  • 1 : 1

  • 1 : 2

  • 4 : 1


26.

A black body has maximum wavelength λm at 2000 K. Its corresponding wavelength at 3000 K will be

  • 32 λm

  • 23 λm

  • 1681 λm

  • 8116 λm


27.

Band spectrum is also called

  • molecular spectrum

  • atomic spectrum

  • flash spectrum

  • line absorption spectrum


28.

The ionization potential of hydrogen is 13.6 V. The energy required to remove an electron from the second orbit of hydrogen is

  • 3.4 eV

  • 6.8 eV

  • 13.6 eV

  • 1.51 eV


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29.

As the electron in Bohr orbit of hydrogen atom passes from state n = 2 to n= 1, the kinetic energy K and potential energy U change as

  • K two-fold, U four-fold

  • K four-fold, U two-fold

  • K four-fold, U also four-fold

  • K two-fold, U also two-fold


30.

Let the potential energy of hydrogen atom in the ground state be regarded as zero. Then its potential energy in the first excited state will be

  • 20.4 eV

  • 13.6 eV 

  • 10.2 eV

  • 6.8 eV


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