An electron of a hydrogen like atom, having \(Z=4\), jumps from \(4^{\text {th }}\) energy state to \(2^{\text {nd }}\) energy state. The energy released in this process, will be :
\((\) Given Rch \(=136 eV )\)
Where \(R =\) Rydberg constant
\(c =\) Speed of light in vacuum
\(h =\) Planck's constant
Step 1: Recall the Formula for Energy Levels in Hydrogen-like Atoms
The energy of an electron in a hydrogen-like atom is given by:
\( E_n = -13.6 \frac{Z^2}{n^2} \, \text{eV} \)
where \( Z \) is the atomic number and \( n \) is the principal quantum number.
Step 2: Calculate the Energy Difference
The energy released (\( \Delta E \)) when an electron jumps from an initial state (\( n_i \)) to a final state (\( n_f \)) is given by the difference in energy levels:
\( \Delta E = E_{n_i} - E_{n_f} = 13.6 Z^2 \left( \frac{1}{n_f^2} - \frac{1}{n_i^2} \right) \, \text{eV} \)
In this case, \( Z = 4 \), \( n_i = 4 \), and \( n_f = 2 \). Substituting these values, we get:
\( \Delta E = 13.6 \times (4^2) \left( \frac{1}{2^2} - \frac{1}{4^2} \right) \, \text{eV} \)
\( \Delta E = 13.6 \times 16 \left( \frac{1}{4} - \frac{1}{16} \right) \, \text{eV} \)
\( \Delta E = 13.6 \times 16 \left( \frac{4 - 1}{16} \right) \, \text{eV} \)
\( \Delta E = 13.6 \times 16 \times \frac{3}{16} \, \text{eV} \)
\( \Delta E = 13.6 \times 3 = 40.8 \, \text{eV} \)
Conclusion: The energy released in the process is 40.8 eV (Option 1).
A hydrogen atom consists of an electron revolving in a circular orbit of radius r with certain velocity v around a proton located at the nucleus of the atom. The electrostatic force of attraction between the revolving electron and the proton provides the requisite centripetal force to keep it in the orbit. According to Bohr’s model, an electron can revolve only in certain stable orbits. The angular momentum of the electron in these orbits is some integral multiple of \(\frac{h}{2π}\), where h is the Planck’s constant.
Ion | Q4+ | Xb+ | Yc+ | Zd+ |
---|---|---|---|---|
Radius (pm) | 53 | 66 | 40 | 100 |
Q4+, Xb+, Yc+, Zd+ are respectively
Let $ P_n = \alpha^n + \beta^n $, $ n \in \mathbb{N} $. If $ P_{10} = 123,\ P_9 = 76,\ P_8 = 47 $ and $ P_1 = 1 $, then the quadratic equation having roots $ \alpha $ and $ \frac{1}{\beta} $ is:
Niels Bohr introduced the atomic Hydrogen model in 1913. He described it as a positively charged nucleus, comprised of protons and neutrons, surrounded by a negatively charged electron cloud. In the model, electrons orbit the nucleus in atomic shells. The atom is held together by electrostatic forces between the positive nucleus and negative surroundings.
Read More: Bohr's Model of Hydrogen Atom
A hydrogen-like atom consists of a tiny positively-charged nucleus and an electron revolving around the nucleus in a stable circular orbit.
If 'e,' 'm,' and 'v' be the charge, mass, and velocity of the electron respectively, 'r' be the radius of the orbit, and Z be the atomic number, the equation for the radii of the permitted orbits is given by r = n2 xr1, where 'n' is the principal quantum number, and r1 is the least allowed radius for a hydrogen atom, known as Bohr's radius having a value of 0.53 Å.
The Bohr Model was an important step in the development of atomic theory. However, it has several limitations.