356611 The energy (in \(eV\)) required to excite an electron from \(n = 2\) to \(n = 4\) state in hydrogen atom

356612 Hydrogen atom in ground state is excited by a monochromatic radiation of \(\lambda = 975\mathop A\limits^ \circ \) Number of spectral lines in the resulting spectrum emitted will be

356613 Assertion :
The electron in the hydrogen atom passes from energy level \(n = 4\) to the \(n = 1\) level. The maximum number of photons that can be emitted are six.
Reason :
The photons are emitted when electrons make a transition from the higher energy state to the lower energy state.

356614 When an electron jumps from the orbit \(n = 2\) to \(n = 4\), then wavelength of the radiations absorbed will be ( \(R\) is Rydberg’s constant)

356615 The ratio of wavelengths of the last line of Balmer series and the last line of Lyman series is:

356611 The energy (in \(eV\)) required to excite an electron from \(n = 2\) to \(n = 4\) state in hydrogen atom

356612 Hydrogen atom in ground state is excited by a monochromatic radiation of \(\lambda = 975\mathop A\limits^ \circ \) Number of spectral lines in the resulting spectrum emitted will be

356613 Assertion :
The electron in the hydrogen atom passes from energy level \(n = 4\) to the \(n = 1\) level. The maximum number of photons that can be emitted are six.
Reason :
The photons are emitted when electrons make a transition from the higher energy state to the lower energy state.

356614 When an electron jumps from the orbit \(n = 2\) to \(n = 4\), then wavelength of the radiations absorbed will be ( \(R\) is Rydberg’s constant)

356615 The ratio of wavelengths of the last line of Balmer series and the last line of Lyman series is:

356611 The energy (in \(eV\)) required to excite an electron from \(n = 2\) to \(n = 4\) state in hydrogen atom

356612 Hydrogen atom in ground state is excited by a monochromatic radiation of \(\lambda = 975\mathop A\limits^ \circ \) Number of spectral lines in the resulting spectrum emitted will be

356613 Assertion :
The electron in the hydrogen atom passes from energy level \(n = 4\) to the \(n = 1\) level. The maximum number of photons that can be emitted are six.
Reason :
The photons are emitted when electrons make a transition from the higher energy state to the lower energy state.

356614 When an electron jumps from the orbit \(n = 2\) to \(n = 4\), then wavelength of the radiations absorbed will be ( \(R\) is Rydberg’s constant)

356615 The ratio of wavelengths of the last line of Balmer series and the last line of Lyman series is:

356611 The energy (in \(eV\)) required to excite an electron from \(n = 2\) to \(n = 4\) state in hydrogen atom

356612 Hydrogen atom in ground state is excited by a monochromatic radiation of \(\lambda = 975\mathop A\limits^ \circ \) Number of spectral lines in the resulting spectrum emitted will be

356613 Assertion :
The electron in the hydrogen atom passes from energy level \(n = 4\) to the \(n = 1\) level. The maximum number of photons that can be emitted are six.
Reason :
The photons are emitted when electrons make a transition from the higher energy state to the lower energy state.

356614 When an electron jumps from the orbit \(n = 2\) to \(n = 4\), then wavelength of the radiations absorbed will be ( \(R\) is Rydberg’s constant)

356615 The ratio of wavelengths of the last line of Balmer series and the last line of Lyman series is:

356611 The energy (in \(eV\)) required to excite an electron from \(n = 2\) to \(n = 4\) state in hydrogen atom

356612 Hydrogen atom in ground state is excited by a monochromatic radiation of \(\lambda = 975\mathop A\limits^ \circ \) Number of spectral lines in the resulting spectrum emitted will be

356613 Assertion :
The electron in the hydrogen atom passes from energy level \(n = 4\) to the \(n = 1\) level. The maximum number of photons that can be emitted are six.
Reason :
The photons are emitted when electrons make a transition from the higher energy state to the lower energy state.

356614 When an electron jumps from the orbit \(n = 2\) to \(n = 4\), then wavelength of the radiations absorbed will be ( \(R\) is Rydberg’s constant)

356615 The ratio of wavelengths of the last line of Balmer series and the last line of Lyman series is: