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Energy Level - Bohr's Atomic Model

Energy Level - Bohr's Atomic Model

Edited By Vishal kumar | Updated on Jul 02, 2025 07:01 PM IST

Niels Bohr's atomic model, proposed in 1913, revolutionized our understanding of atomic structure by introducing the concept of quantized energy levels. According to Bohr's model, electrons orbit the nucleus at specific, fixed distances, corresponding to discrete energy levels. This quantization explains why atoms emit or absorb light at characteristic wavelengths, a principle foundational to spectroscopy. In real life, Bohr's model is crucial for technologies like lasers and fluorescent lights, where precise control of electron transitions produces specific colours of light. In this article we will understand that energy levels also underpin the operation of various electronic devices, from semiconductors to imaging systems, demonstrating the profound impact of Bohr's atomic model on both science and technology.

This Story also Contains
  1. The Energy of an Electron in the nth Orbit
  2. Excitation Energy and Excitation Potential
  3. Now, what is Excitation?
  4. Excitation Energy
  5. Solved Examples Based on Energy Level - Bohr's Atomic Model
  6. Summary

The Energy of an Electron in the nth Orbit

In Bohr's atomic model, the energy levels of an electron in an atom are quantized. This means that electrons can only occupy specific, discrete energy levels and cannot exist in between these levels. The potential energy is always negative, indicating that the electron is bound to the nucleus. The energy levels of the electron are quantized, and the total energy is the sum of kinetic and potential energies.

Potential Energy

An electron possesses some potential energy because it is found in the field of the nucleus potential energy of an electron in $n^{\text {th }}$ orbit of the radius $r_{n}$ is given by

$U=k \frac{(Z e)(-e)}{r_n}=-\frac{k Z e^2}{r_n}$

Kinetic Energy

Electrons possess kinetic energy because of their motion. Closer orbits have greater kinetic energy than
outer ones. As we know $\frac{m v^2}{r_n}=\frac{k(Z e)(e)}{r_n^2}$

Kinetic energy $K=\frac{k Z e^2}{2 r_s}=\frac{|U|}{2}$

Total Energy

Total energy E is the sum of potential energy and kinetic energy ie. $E=K+U$
$
\begin{aligned}
& \Rightarrow \quad E=-\frac{k Z e^2}{2 r_n} \quad{ }_{\text {also }} r_n=\frac{n^2 h^2 \varepsilon_0}{z \pi m e^2} \\
& \text { Hence } E=-\left(\frac{m e^4}{8 \varepsilon_0^2 h^2}\right) \frac{z^2}{n^2}=-\left(\frac{m e^4}{8 \varepsilon_0^2 c h^3}\right) \operatorname{ch} \frac{z^2}{n^2} \\
& =-R \operatorname{ch} \frac{Z^2}{n^2}=-13.6 \frac{Z^2}{n^2} \mathrm{eV} \\
&
\end{aligned}
$
where $R=\frac{m e^4}{8 e^2 c^3 h^3}=$ Rydberg's constant $=1.09 \times 10^7 \mathrm{~m}^{-1}$

The Energy Level for Hydrogen

The energy of $\underline{n}^{\text {th }}$ level of hydrogen atom $(z=1)$ is given as :
$
E_n=-\frac{z^2 13.6}{n^2} \mathrm{eV}=-\frac{13.6}{n^2} \mathrm{eV} \quad(\because z=1)
$

Energy of Ground $\operatorname{state}(n=1)=E_1=-\frac{13.6}{1} \mathrm{eV}=-13.6 \mathrm{eV}$
Energy of first excited state $(n=2)=E_2=-\frac{13.6}{4} \mathrm{eV}=-3.4 \mathrm{eV}$
Energy of second excited state $(n=3)=E_3=-\frac{13.6}{9} \mathrm{eV}=-1.51 \mathrm{eV}$
Energy of third excited state $(n=4)=E_4=-\frac{13.6}{16} \mathrm{eV}=-0.85 \mathrm{eV}$

Binding Energy(B.E.) of nth orbit

The binding energy of an electron in the n-th orbit of a hydrogen atom refers to the energy required to remove the electron from that orbit to infinity, essentially ionizing the atom. In the context of the Bohr model, the binding energy of an electron in the n-th orbit can be expressed as:

The energy required to move an electron from $n^{\text {th }}$ orbit to $n=\infty$ is called the Binding energy of $\underline{n}^{\text {th }}$ orbit

OR
The binding energy of $\underline{\underline{t}}^{\text {th }}$ orbit is the negative of the total energy of that orbit
$
E_{\text {Binding }}=E_{\infty}-E_n=-E_n=\frac{13.6 Z^2}{n^2} \mathrm{eV}
$

Ionization Energy

The total energy of a hydrogen atom corresponds to infinite separation between electron and nucleus. Total positive energy implies that the atom is ionized and the electron is in an unbound (isolated) state moving with certain kinetic energy. The minimum energy required to move an electron from the ground state(n=1) to $n=\infty$ is called the ionization energy of the atom or ion.

The formula for the ionization energy is -

$E_{\text {ionisition }}=E_{\infty}-E_1=-E_1=13.6 Z^2 \mathrm{eV}$

On the basis of ionization energy, we can define the ionization potential also -

Ionization Potential

The potential difference through which a free electron must be accelerated from rest such that its kinetic energy becomes equal to the ionization energy of the atom is called the ionization potential of the atom.

$V_{\text {ionisation }}=\frac{E_{\text {Ionisation }}}{e}=13.6 Z^2 \mathrm{~V}$

Now let us discuss Excitation energy and Excitation potential

Excitation Energy and Excitation Potential

Excitation Energy and Excitation Potential are related concepts in atomic physics, referring to the energy required to move an electron from a lower energy state to a higher one within an atom.

Now, what is Excitation?

The process of absorption of energy by an electron so as to raise it from a lower energy level to some higher energy level is called excitation.

Excited State

When an atom or molecule absorbs energy, an electron can move from the ground state to a higher energy level. This higher energy level is called an excited state.

The states of an atom other than the ground state are called its excited states. Examples are mentioned below -
$n=2, \quad$ first excited state
$n=3, \quad$ second excited state
$n=4, \quad$ third excited state
$n=n_0+1, \quad n_0$ th excited state


Excitation Energy

The energy required to move an electron from the ground state of the atom to any other excited state of the atom is called the Excitation energy of that state.

$E_{\text {cxcitation }}=E_{\text {higher }}-E_{\text {lower }}$

Excitation potential can also be defined on the basis of excitation energy. So the excitation potential is the potential difference through which an electron must be accelerated from rest so that its kinetic energy becomes equal to the excitation energy of any state is called the excitation potential of state.

$V_{\text {excitation }}=\frac{E_{\text {excritation }}}{e}$

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Solved Examples Based on Energy Level - Bohr's Atomic Model

Example 1: If the series limit frequency of the Lyman series is νL, then the series limit frequency of the Pfund series is :

1) νL/25

2) 25 νL

3) 16 νL

4) νL/16

Solution:

P-fund Series

$
\frac{1}{\lambda}=R\left(\frac{1}{5^2}-\frac{1}{n^2}\right)_{\text {(infrared) }}
$
wherein
$
n=6,7,8-\cdots
$

When an electron jumps from a higher orbital to $\mathrm{n}=5$ energy level
Lyman series
$
\frac{1}{\lambda}=R\left(\frac{1}{1^2}-\frac{1}{n^2}\right)_{\text {(UV region ) }}
$
wherein
$
n=2,3,4,-----
$

When an electron jumps from a higher orbital to $1^{\text {st }}$ energy level i.e. ground state
For Lyman $\quad h \nu_L=13.6 \mathrm{ev}$

For p-fund
$
h \nu_p=\frac{13.6}{5^2}=\frac{13.6}{25}
$
therefore, $\frac{v_L}{v_P}=25 \quad$ or $\quad v_p=\frac{\nu_L}{25}$

Hence, the answer is the option 1.

Example 2: Arrange the following electromagnetic radiations per quantum in the order of increasing energy :

A: Blue light B: Yellow light
C: X-ray D: Radiowave.

1) D, B, A, C

2) A, B, D, C

3) C, A, B, D

4) B, A, D, C

Solution:

Balmer series

Balmer series
$
\frac{1}{\lambda}=R\left(\frac{1}{2^2}-\frac{1}{n^2}\right)
$
(visible light)
wherein
$
n=3,4,5----
$

When an electron jumps from a higher orbital to an n=2 energy level

Radio wave < Yellow light < Blue light < X-ray

Hence, the answer is the option 1.

Example 3: The amount of energy required (in eV) to excite an electron from the 3rd to 4th orbit of the hydrogen atom:

1) 0.66

2) 0.77

3) 0.88

4) 0.99

Solution:
From Paschen Series,

$
\frac{1}{\lambda}=R\left(\frac{1}{3^2}-\frac{1}{n^2}\right)
$
(infrared)
$
\begin{aligned}
\Delta E= & \frac{h c}{\lambda}=R h c\left(\frac{1}{3^2}-\frac{1}{4^2}\right) \\
& =13.6\left(\frac{1}{9}-\frac{1}{16}\right) \mathrm{eV} \\
& =13.6 \frac{7}{144} \mathrm{eV}=0.66 \mathrm{eV}
\end{aligned}
$

Hence, the correct answer is 0.66 eV.

Example 4: Brackett series of lines are produced when electrons excited to a high energy level make the transition to the n=4 level, the wavelength (in nm) corresponding to the transition from nf =6 to ni=4 is:

1) 2630

2) 6025

3) 3858

4) 4051

Solution:

From the Brackett Series,

$
\begin{aligned}
& \frac{1}{\lambda}=R\left(\frac{1}{4^2}-\frac{1}{n^2}\right) \\
& (\text { infrared })
\end{aligned}
$
wherein
$
n=5,6,7----
$

When an electron jumps from a higher orbital to $n=4$ energy level
$
\begin{aligned}
\frac{1}{\lambda} & =R\left(\frac{1}{4^2}-\frac{1}{n^2}\right)=R\left(\frac{1}{16}-\frac{1}{36}\right) \\
\lambda & =\frac{144}{5 R} \\
\lambda & =\frac{144}{5} \times 91 \mathrm{~nm}=2630 \mathrm{~nm}
\end{aligned}
$

Hence, the answer is option (1).

Example 5: The first member of the Balmer series of hydrogen atoms has a wavelength of 6561 \AA. The wavelength of the second member of the Balmer series (in nm ) is _______.

1) 486

2) 972

3) 986

4) 586

Solution:

$\begin{aligned} \frac{1}{\lambda} & =\mathrm{R} Z^2\left(\frac{1}{n_1^2}-\frac{1}{n_2^2}\right) \\ \frac{1}{\lambda_1} & =R(1)^2\left(\frac{1}{2^2}-\frac{1}{3^2}\right)=\frac{5 \mathrm{R}}{36} \\ \frac{1}{\lambda_2} & =\mathrm{R}(1)^2\left(\frac{1}{2^2}-\frac{1}{4^2}\right)=\frac{3 \mathrm{R}}{16} \\ \frac{\lambda_2}{\lambda_1} & =\frac{20}{27} \\ \lambda_2 & =\frac{20}{27} \times 6561 \mathrm{~A}=4860 \mathrm{~A} \\ & =486 \mathrm{~nm}\end{aligned}$

Hence, the answer is option (1).

Summary

Niels Bohr's 1913 atomic model introduced quantized energy levels, explaining why atoms emit or absorb light at specific wavelengths. This model is fundamental to spectroscopy and underpins technologies like lasers and fluorescent lights. The energy of an electron in a given orbit, the binding energy, and the ionization energy are crucial for understanding atomic transitions. Excitation energy refers to the energy required to move an electron from a lower to a higher energy state, while excitation potential is the corresponding voltage needed. Practical examples include determining the frequency of spectral lines and energy transitions in various atomic series.

Frequently Asked Questions (FAQs)

1. How does Bohr's model incorporate Planck's quantum theory?
Bohr's model incorporates Planck's quantum theory by assuming that electrons can only exist in discrete energy states, not in a continuum of energies. It applies the idea that energy is quantized (comes in discrete packets) to the structure of atoms. When electrons transition between these quantized energy levels, they absorb or emit energy in discrete amounts (quanta) as proposed by Planck. This integration of quantum concepts into atomic structure was a crucial step in the development of quantum mechanics.
2. What is the Rydberg formula and how does it relate to Bohr's model?
The Rydberg formula is an equation that predicts the wavelengths of spectral lines in many chemical elements, particularly hydrogen. It's closely related to Bohr's model as it calculates the energy difference between two energy levels. The formula uses the principal quantum numbers of the initial and final energy levels to determine the wavelength of emitted or absorbed light. Bohr's model provided a theoretical basis for this empirical formula, explaining why it works and connecting it to the concept of quantized energy levels.
3. How does Bohr's model explain the Balmer series in hydrogen's spectrum?
Bohr's model explains the Balmer series in hydrogen's spectrum by attributing it to electron transitions from higher energy levels to the second energy level (n=2). Each line in the Balmer series corresponds to a specific transition: from n=3 to n=2, n=4 to n=2, and so on. The model accurately predicts the wavelengths of these spectral lines using the energy level differences, providing strong evidence for the quantized nature of electron energy levels in atoms.
4. What is the Bohr frequency condition?
The Bohr frequency condition is a fundamental principle in Bohr's model that relates the frequency of emitted or absorbed light to the energy difference between two electron energy levels. It states that the frequency of light emitted or absorbed when an electron transitions between energy levels is proportional to the energy difference between those levels. Mathematically, it's expressed as ΔE = hf, where ΔE is the energy difference, h is Planck's constant, and f is the frequency of light.
5. What is the significance of the ionization energy in Bohr's model?
Ionization energy in Bohr's model is the energy required to remove an electron from its ground state to infinity (essentially freeing it from the atom). It's significant because it represents the strongest binding of an electron to the atom and helps in understanding atomic properties and chemical behavior. In Bohr's model, the ionization energy is directly related to the energy of the outermost occupied energy level, providing insights into an element's reactivity and its position in the periodic table.
6. How does the principal quantum number relate to energy levels in Bohr's model?
The principal quantum number (n) in Bohr's model directly relates to the energy levels. It's a positive integer (1, 2, 3, etc.) that identifies each energy level or shell. As n increases, the energy of the level increases, and its distance from the nucleus also increases. The energy of an electron in a given level is proportional to -1/n^2, meaning higher n values correspond to higher (less negative) energies.
7. Why are energy levels in Bohr's model called "quantized"?
Energy levels in Bohr's model are called "quantized" because they exist only in discrete, specific values. Electrons can't have any arbitrary energy between these levels. This quantization means that electrons can only gain or lose energy in fixed amounts, corresponding to jumps between these discrete levels. This concept was revolutionary as it contradicted classical physics, which assumed energy could change continuously.
8. What is Bohr's atomic model and how does it relate to energy levels?
Bohr's atomic model is a theoretical representation of the atom proposed by Niels Bohr in 1913. It describes electrons orbiting the nucleus in fixed, circular orbits called energy levels or shells. Each energy level corresponds to a specific amount of energy an electron can have. The model explains that electrons can only exist in these discrete energy levels and can jump between them by absorbing or emitting specific amounts of energy.
9. What is the ground state in Bohr's atomic model?
The ground state in Bohr's atomic model is the lowest energy level an electron can occupy in an atom. It's the most stable state, where electrons tend to remain unless excited by external energy. In the ground state, electrons occupy the innermost available energy levels according to the atom's electron configuration. Understanding the ground state is crucial for predicting an atom's behavior and chemical properties.
10. How does the concept of stationary states in Bohr's model differ from classical physics?
The concept of stationary states in Bohr's model fundamentally differs from classical physics. In Bohr's model, electrons exist in stable, non-radiating orbits (stationary states) around the nucleus, contrary to classical electromagnetic theory which predicts that accelerating charges (like orbiting electrons) should continuously emit radiation and spiral into the nucleus. This stability of electron orbits was a revolutionary idea that helped explain why atoms don't collapse and laid the groundwork for quantum mechanics.
11. How do electrons move between energy levels in Bohr's model?
In Bohr's model, electrons move between energy levels by absorbing or emitting specific amounts of energy, usually in the form of photons (light particles). When an electron absorbs energy, it jumps to a higher energy level. When it releases energy, it falls to a lower energy level. The energy of the absorbed or emitted photon exactly matches the energy difference between the two levels involved in the transition.
12. How does Bohr's model explain the emission spectrum of hydrogen?
Bohr's model explains the emission spectrum of hydrogen by relating spectral lines to electron transitions between energy levels. When excited hydrogen atoms release energy, electrons fall from higher to lower energy levels, emitting photons with specific wavelengths. These wavelengths correspond to the colored lines in hydrogen's emission spectrum. The model accurately predicts the wavelengths of these spectral lines, providing strong support for the concept of quantized energy levels.
13. How does Bohr's model explain the stability of atoms?
Bohr's model explains the stability of atoms by proposing that electrons orbit the nucleus in fixed energy levels without radiating energy. This stability contradicts classical physics, which predicts that orbiting electrons should continuously lose energy and collapse into the nucleus. By introducing the concept of stationary states where electrons don't radiate energy, Bohr's model provides a mechanism for atoms to maintain their structure over time, explaining their observed stability in nature.
14. How does Bohr's model explain the concept of quantum jumps?
Bohr's model explains quantum jumps as the discrete transitions of electrons between energy levels. Unlike classical physics, where energy changes can be continuous, Bohr proposed that electrons can only move between specific, allowed energy states. These jumps occur instantaneously when an electron absorbs or emits a photon with energy exactly equal to the difference between two energy levels. This concept of discrete, instantaneous transitions was a radical departure from classical physics and a key feature of early quantum theory.
15. Why does Bohr's model work well for hydrogen but not for other elements?
Bohr's model works well for hydrogen because it's the simplest atom with only one electron. For multi-electron atoms, the model fails to account for electron-electron repulsions and more complex quantum mechanical effects. It doesn't explain the fine structure of spectral lines or the behavior of electrons in orbitals. Despite these limitations, Bohr's model remains valuable for understanding basic atomic concepts and as a stepping stone to more advanced quantum mechanical models.
16. What is the Bohr radius and why is it significant?
The Bohr radius is the distance between the nucleus and the electron in the ground state of a hydrogen atom in Bohr's model. It's significant because it serves as a fundamental unit of length in atomic physics, approximately equal to 5.29 × 10^-11 meters. The Bohr radius helps in understanding atomic sizes and in calculations involving atomic orbitals and energy levels in more complex atoms.
17. What is the relationship between an electron's energy and its orbital radius in Bohr's model?
In Bohr's model, an electron's energy is inversely related to its orbital radius. As the orbital radius increases, the electron's energy increases (becomes less negative). This relationship is described by the equation E = -k/r^2, where E is the energy, k is a constant, and r is the orbital radius. This means that electrons in higher energy levels (larger n) have larger orbital radii and higher (less negative) energies, while those in lower energy levels are closer to the nucleus and have lower (more negative) energies.
18. What is the shell structure in Bohr's model and how does it relate to the periodic table?
The shell structure in Bohr's model refers to the arrangement of electrons in concentric circular orbits around the nucleus, each corresponding to a different energy level. These shells are labeled K, L, M, N, etc., corresponding to principal quantum numbers 1, 2, 3, 4, and so on. This structure relates to the periodic table by explaining the periodicity of chemical properties. Elements in the same row of the periodic table have their outermost electrons in the same shell, leading to similar chemical properties.
19. What is the limitation of Bohr's model in explaining the spectra of multi-electron atoms?
Bohr's model is limited in explaining the spectra of multi-electron atoms because it doesn't account for electron-electron interactions or the three-dimensional nature of electron orbitals. It assumes that each electron moves independently in a circular orbit, which is an oversimplification for atoms with more than one electron. As a result, while it works well for hydrogen-like atoms, it fails to accurately predict the complex spectral patterns observed in multi-electron atoms, where electron-electron repulsion and more complex quantum effects play significant roles.
20. How does the concept of angular momentum quantization feature in Bohr's model?
Angular momentum quantization is a key feature of Bohr's model. Bohr proposed that the angular momentum of an electron in its orbit around the nucleus is quantized, meaning it can only take on certain discrete values. Specifically, he postulated that the angular momentum must be an integer multiple of ℏ (h-bar, which is Planck's constant divided by 2π). This quantization condition leads directly to the discrete energy levels and is crucial for explaining why electrons can only exist in specific orbits.
21. What is the physical significance of the quantum condition in Bohr's model?
The quantum condition in Bohr's model, which states that the angular momentum of an electron must be an integer multiple of ℏ, has profound physical significance. It explains why electrons can only exist in certain discrete energy levels rather than in a continuum of energies. This condition leads to the stability of atoms by preventing electrons from spiraling into the nucleus. It also provides a theoretical basis for the observed spectral lines of atoms, linking the macroscopic world of observable spectra to the microscopic world of atomic structure.
22. How does Bohr's model explain the concept of excited states?
Bohr's model explains excited states as configurations where one or more electrons occupy higher energy levels than their ground state. When an atom absorbs energy (e.g., from light or collision), electrons can jump to these higher levels, creating an excited state. These states are unstable, and electrons tend to quickly return to lower energy levels, emitting photons in the process. This concept is crucial for understanding atomic spectra, fluorescence, and many other phenomena in atomic physics and chemistry.
23. What is the role of Coulomb's law in Bohr's atomic model?
Coulomb's law plays a crucial role in Bohr's atomic model by describing the electrostatic force between the positively charged nucleus and the negatively charged electron. This attractive force is what keeps the electron in orbit around the nucleus. Bohr used Coulomb's law to calculate the energy of the electron in different orbits, balancing the electrostatic attraction with the centripetal force needed for circular motion. This application of classical electrostatics within a quantum framework was a key innovation of Bohr's model.
24. How does Bohr's model explain the difference in spectra between different elements?
Bohr's model explains the difference in spectra between elements by considering the different nuclear charges and electron configurations. Each element has a unique number of protons in its nucleus, resulting in different electrostatic forces on the electrons. This leads to unique energy level spacings for each element. Consequently, the energy transitions between these levels, which produce spectral lines, are unique to each element. This explains why each element has its own characteristic spectrum, serving as a kind of "fingerprint" for identification.
25. What is the significance of the Bohr magneton in atomic physics?
The Bohr magneton is a physical constant of magnetic moment that naturally arises from Bohr's model. It represents the magnetic moment of an electron orbiting in the ground state of a hydrogen atom. The Bohr magneton is significant because it serves as a fundamental unit for expressing the magnetic moments of electrons in more complex atoms and molecules. It plays a crucial role in understanding magnetic properties of materials and in fields like electron spin resonance spectroscopy.
26. How does Bohr's model relate to the concept of quantized angular momentum?
Bohr's model directly incorporates the concept of quantized angular momentum. It postulates that the angular momentum of an electron in its orbit can only take on discrete values, specifically integer multiples of ℏ. This quantization is a fundamental aspect of the model and leads to the discrete energy levels. It represents a departure from classical physics, where angular momentum can have any value, and is a key step towards the development of quantum mechanics, where quantization of various physical properties becomes a central theme.
27. What is the relationship between the Bohr model and the concept of wave-particle duality?
While Bohr's model predates the full development of wave-particle duality, it inadvertently incorporates aspects of this concept. The model treats electrons as particles orbiting the nucleus, yet the quantization of energy levels hints at their wave-like nature. The fact that electrons can only exist in specific energy states aligns with the later development of electron waves in quantum mechanics. Bohr's model thus serves as a bridge between classical particle-based physics and the wave-particle duality central to quantum theory.
28. How does Bohr's model explain the stability of electron orbits?
Bohr's model explains the stability of electron orbits by proposing that electrons can only exist in specific, allowed energy states. Unlike in classical physics, where orbiting charges should continuously emit energy and spiral into the nucleus, Bohr's electrons in these "stationary states" do not radiate energy. This stability is ensured by the quantization condition, which only allows certain orbits. While this explanation was later superseded by quantum mechanics, it provided a crucial first step in understanding atomic stability.
29. What is the significance of the Lyman series in relation to Bohr's model?
The Lyman series is a set of spectral lines in the ultraviolet part of hydrogen's emission spectrum. In Bohr's model, these lines correspond to electron transitions from higher energy levels down to the ground state (n=1). The model accurately predicts the wavelengths of these lines, providing strong support for Bohr's theory. The Lyman series is significant because it demonstrates the model's predictive power beyond the visible spectrum and reinforces the concept of quantized energy levels in atoms.
30. How does Bohr's model explain the concept of electron shells?
Bohr's model introduces the concept of electron shells as distinct, concentric circular orbits around the nucleus. Each shell corresponds to a specific energy level, with the innermost shell having the lowest energy. The model proposes that electrons fill these shells from the inside out, with each shell having a maximum number of electrons it can hold. This concept of shells helps explain the periodic trends in chemical properties of elements and laid the groundwork for understanding electron configurations in more advanced atomic models.
31. What is the role of Planck's constant in Bohr's atomic model?
Planck's constant plays a crucial role in Bohr's atomic model. It appears in the quantization condition for angular momentum and in the equation relating energy transitions to the frequency of emitted or absorbed light. The presence of Planck's constant in these equations signifies the quantum nature of the model, distinguishing it from classical physics. It ensures that energy and angular momentum are quantized, leading to discrete energy levels and explaining the observed spectral lines of atoms.
32. How does Bohr's model explain the concept of atomic excitation and de-excitation?
Bohr's model explains atomic excitation as the process where an electron absorbs energy and jumps to a higher energy level, creating an excited state. De-excitation occurs when an electron in a higher energy level falls back to a lower level, emitting a photon in the process. The energy of the emitted or absorbed photon exactly matches the energy difference between the two levels involved. This mechanism provides a clear explanation for the discrete spectral lines observed in atomic spectra.
33. What is the significance of the Rydberg constant in Bohr's model?
The Rydberg constant is a fundamental physical constant that appears in the Rydberg formula, which describes the wavelengths of spectral lines in many chemical elements. In Bohr's model, this constant is directly related to fundamental properties like the electron mass, charge, and Planck

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