Consider the spectral line resulting from the transition from n= 2 to n = 1, in atoms and ions given below. The shortest wavelength is produced by
hydrogen atom
deuterium atom
doubly ionized lithium
doubly ionized helium
The energy of an electron in excited hydrogen atom is −3.4eV. Then according to Bohr's theory, the angular momentum of the electron is
2.1 × 10-34 J-s
3 × 10-34 J-s
2 × 10-34 J-s
0.5 × 10-34 J-s
The solar spectrum during a complete solar eclipse is
continuous
emission line
dark line
dark band
A particle of mass M at rest decays into two masses m1 and m2 with non zero velocities. The ratio of de-Broglie wavelengths of the particles is
1 : 1
If elements with principal quantum number n > 4 were not allowed in nature, the number of possible elements would have been
32
60
64
4
The spectrum obtained from the chromosphere of the sun at the time of total solar eclipse is
line emission spectrum
band emission spectrum
continuous emission spectrum
line absorption spectrum
Which state of triply ionised Beryllium (Be+++) has the same orbital radius as that of the ground state of hydrogen ?
n = 3
n = 4
n = 1
n = 2
If M is the atomic mass and A is the mass number, packing fraction is given by
B.
The mass excess per nucleon of isotopes of atom is known as packing fraction given by
where M is the actual mass of isotope and A is its atomic mass. Packing fraction is positive for isotope having very low or very high mass number and negative for all others.
Excitation energy of a hydrogen like ion in its first excitation state is 40.8 eV. Energy needed to remove the electron from the ion in ground state is
40.8 eV
27.2 eV
54.4 eV
13.6 eV