The ionisation energy of hydrogen atom is 13.6 eV. Following Bohr’s theory, the energy corresponding to a transition between 3rd and 4th orbit is
(1992)
The energy of the nth orbit is $E_n = -\frac{13.6}{n^2} eV$. For $n=3$, $E_3 = -1.51 eV$, and for $n=4$, $E_4 = -0.85 eV$. The energy difference is $\Delta E = E_4 - E_3 = -0.85 - (-1.51) = 0.66 eV$.
According to Bohr's second postulate, the electron revolves only in those orbits for which its angular momentum is an integral multiple of $h/(2\pi)$. Hence, it assumes that the angular momentum of electrons is quantized.
The ground state energy of H-atom is 13.6 eV. The energy needed to ionize H-atom from its second excited state is:
(1991)
The second excited state corresponds to $n=3$. The energy of this state is $E_3 = -\frac{13.6}{3^2} = -1.51 eV$. The energy required to remove the electron to infinity (ionization) is $0 - (-1.51) = 1.51 eV$.
In which of the following systems will be radius of the first orbit (n = 1) be minimum:
(2003)
The radius of the nth orbit in a hydrogen-like species is given by $r_n \propto \frac{n^2}{Z}$. For the first orbit ($n=1$), the radius is inversely proportional to the atomic number $Z$. Doubly ionised lithium ($Li^{2+}$) has the maximum $Z=3$, thus it has the minimum radius.
The energy of hydrogen atom in $n^{th}$ orbit is $E_n$ then the energy in $n^{th}$ orbit of singly ionised helium atom will be:
(2001)
Energy of an electron in a hydrogen-like atom is $E \propto Z^2$. For hydrogen $Z=1$, $E = E_n$. For singly ionised helium ($He^+$), $Z=2$. Therefore, the energy in the same orbit is $2^2 E_n = 4 E_n$.
Maximum frequency of emission is obtained for the transition:
(2000)
Frequency $\nu \propto \Delta E$. Emission occurs when transitioning from a higher to a lower energy state. The energy difference between $n=2$ and $n=1$ ($10.2 eV$) is the largest among the given emission transitions.
When an electron do transition from $n = 4$ to $n = 2$, then emitted line in spectrum will be:
(2000)
Transitions ending at $n=2$ belong to the Balmer series. The transition $n=3 \rightarrow 2$ is the first line, and $n=4 \rightarrow 2$ is the second line of the Balmer series.
In the Bohr model of H-atom, an electron (e) is revolving around a proton (p) with velocity v, if r is the radius of orbit and m is mass and $\epsilon_0$ is vacuum permittivity, the value of v is:
(1998)
The necessary centripetal force is provided by the electrostatic force of attraction. Thus, $\frac{mv^2}{r} = \frac{1}{4\pi\epsilon_0} \frac{e^2}{r^2}$. Solving for velocity yields $v = \frac{e}{\sqrt{4\pi\epsilon_0 m r}}$.
The energy of the ground electronic state of hydrogen atom is $-13.6 eV$. The energy of the first excited state will be
(1997)
The energy of the nth state is given by $E_n = \frac{-13.6}{n^2} eV$. The first excited state corresponds to $n=2$. Therefore, $E_2 = \frac{-13.6}{2^2} = -3.4 eV$.
When hydrogen atom is in its first excited level, its radius isΒ of the Bohr radius.
(1997)
The radius of the nth Bohr orbit is $r_n = r_0 n^2$, where $r_0$ is the Bohr radius. For the first excited level ($n=2$), $r_2 = r_0(2^2) = 4r_0$. Hence, it is 4 times the Bohr radius.