Gen Chem 1.1 to 1.2
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Questions and Answers

Which of the following concepts is a direct consequence of the wave-particle duality of matter?

  • It is impossible to know both the position and momentum of an electron with perfect accuracy. (correct)
  • The energy of an electron is continuously variable and not restricted to discrete levels.
  • Atomic nuclei are composed of protons and neutrons.
  • Electrons must exist in specific, quantized orbits around the nucleus.

The Bohr model can accurately predict the energy levels and spectra of multi-electron atoms.

False (B)

According to de Broglie, what properties do moving particles exhibit?

wave-like

The Schrödinger equation incorporates both _________ and _________ behavior to describe the location and behavior of an electron in an atom.

<p>particle, wave</p> Signup and view all the answers

Match the component of the electron wavefunction with what it describes:

<p>Radial part = How far away the electron is from the nucleus Angular part = The angle from the nucleus to the electron</p> Signup and view all the answers

The Heisenberg Uncertainty Principle states that:

<p>It is impossible to simultaneously know both the position and momentum of an electron with perfect accuracy. (A)</p> Signup and view all the answers

Which of the following is a limitation of the Bohr model of the atom?

<p>It can only explain the spectra of single-electron species. (D)</p> Signup and view all the answers

In the context of quantum mechanics, what does the wavefunction ($\psi$) of an electron describe?

<p>The probability amplitude of finding the electron at a particular location. (C)</p> Signup and view all the answers

According to Bohr's model, what happens to the distance between an electron's orbit and the nucleus as the energy level (n) increases?

<p>The distance increases. (C)</p> Signup and view all the answers

Niels Bohr proposed that electrons can orbit the nucleus at any energy level, similar to a solar system.

<p>False (B)</p> Signup and view all the answers

What term is used to describe the most stable energy level (n=1) in the Bohr model?

<p>ground state</p> Signup and view all the answers

The energy of electrons is ____________, meaning they can only exist in certain energy levels.

<p>quantized</p> Signup and view all the answers

What does the variable 'n' represent in the context of the Bohr model?

<p>An orbit or energy level of an electron (D)</p> Signup and view all the answers

What happens to the proximity of energy levels as 'n' increases in the Bohr model?

<p>They get closer and closer together. (A)</p> Signup and view all the answers

Atoms and molecules can have any energy value.

<p>False (B)</p> Signup and view all the answers

In the Bohr model of the hydrogen atom, what does the equation $E_n = - \frac{R_H}{n^2}$ typically calculate?

<p>The energy of an electron in orbit 'n'. (B)</p> Signup and view all the answers

According to Bohr's model, what causes the emission of radiation by an energized hydrogen atom?

<p>An electron transitioning from a higher energy orbit to a lower energy orbit. (C)</p> Signup and view all the answers

In Bohr's model, absorption involves an electron transitioning from a higher energy level to a lower energy level.

<p>False (B)</p> Signup and view all the answers

What fundamental concept did Bohr's model introduce regarding the existence of electrons within an atom?

<p>energy levels</p> Signup and view all the answers

According to Bohr's model, when electrons transition between energy levels, ________ is exchanged.

<p>energy</p> Signup and view all the answers

Which of the following equations correctly represents the energy of a photon emitted or absorbed during an electronic transition, according to the provided information? (Where $R_h$ is Rydberg's constant)

<p>$DE = R_h(\frac{1}{n_f^2} - \frac{1}{n_i^2})$ (D)</p> Signup and view all the answers

What is the value of Planck's constant ($h$) according to the provided information?

<p>$6.626 \times 10^{-34}$ J s (B)</p> Signup and view all the answers

Quantum mechanics provides a less comprehensive understanding of the atom compared to the Bohr model.

<p>False (B)</p> Signup and view all the answers

What is the term used to describe the 'quantum' of energy emitted in the form of light when an electron transitions between energy levels?

<p>photon</p> Signup and view all the answers

According to Bohr's model, which scenario describes energy absorption?

<p>$E_f &gt; E_i$ (C)</p> Signup and view all the answers

Match the term with the description:

<p>Emission = Electron transitions to lower energy levels Absorption = Electron transitions to higher energy levels Planck's constant = Relates energy of photon to its frequency</p> Signup and view all the answers

Flashcards

Wave-particle duality

The concept that particles (like electrons) can exhibit wave-like properties, and waves can exhibit particle-like properties.

Quantization of energy

Energy is not continuous but exists in discrete packets called quanta. Energy changes occur in specific, defined amounts.

Heisenberg Uncertainty Principle

It is fundamentally impossible to know both the position and momentum of a particle (like an electron) with perfect accuracy.

Limitation of Bohr model

Bohr's model accurately predicted the behavior of hydrogen atoms, it falters when applied to atoms with multiple electrons, systems with one electron only

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De Broglie's assertion

A moving particle also exhibits wave-like properties.

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Schrödinger equation

An equation that describes the location and behavior of an electron in an atom by using both particle and wave behavior (wavefunctions).

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Radial part of wavefunction

Describes how far away the electron is from the nucleus.

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Angular part of wavefunction

Describes the electron's position in three-dimensional space relative to the nucleus and helps define shapes of atomic orbitals.

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Planck's Constant (h)

Fundamental constant linking energy and frequency of a photon; 6.626 x 10^-34 J*s.

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Emission

Emission occurs when an electron transitions from a higher to lower energy level, releasing energy as a photon.

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Absorption

Absorption occurs when an electron transitions from a lower to higher energy level by absorbing a photon.

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Ef

In Bohr's model, this is the final energy level of an electron after a transition.

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Ei

In Bohr's model, this is the initial energy level of an electron before a transition.

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ΔE (Change in Energy)

Difference in energy levels (final minus initial) during electron transition, dictating photon energy.

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Energy Equation (Bohr)

Mathematical expression to determine the discrete energy values for electrons.

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Electron Energy Levels

Bohr's model introduced the concept that electrons exist in specific, quantized energy levels.

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Energy Exchange

Bohr's model successfully explained the hydrogen atomic spectra by linking electron transitions and energy exchange.

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Quantum Mechanics

More modern theory of atomic structure, accounts for phenomena that Bohr's model could not, more complex.

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Line Emission Spectra

Specific light wavelengths emitted by excited atoms.

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Quantized Energy Levels

Electrons can only exist in certain energy levels.

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Energy Levels

Allowable, discrete states atoms/molecules can have.

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Ground State (n=1)

The most stable, lowest energy state of an electron.

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Excited State

Any energy level higher than the ground state (n>1).

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Distance vs. 'n'

As 'n' increases, distance increases.

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Energy Level Proximity

Energy levels get closer together.

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Electron Energy

The energy of an electron in Orbit 'n' (%)

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Study Notes

  • Atomic structure and the birth of quantum mechanics are covered.
  • The topics include the nature of light, atomic spectroscopy and the Bohr model, the wave nature of matter, and quantum mechanics and the atom.

A History of the Atom: Theories and Models

  • This graphic looks at atomic models and how they developed.
  • In 1803, John Dalton drew upon the Ancient Greek idea of atoms and his theory stated that atoms are indivisible, those of a given element are identical, and compounds are combinations of different types of atoms.
  • In 1904, J.J. Thomson discovered electrons in atoms in 1897, for which he won a Nobel Prize, produced the 'plum pudding' model which shows the atom as composed of electrons scattered throughout a spherical cloud of positive charge.
  • In 1911, Ernest Rutherford fired positively charged alpha particles at a thin sheet of gold foil, and realized positive charge was localized in the nucleus of an atom.
  • In 1913, Niels Bohr modified Rutherford's model of the atom by stating that electrons moved around the nucleus in orbits of fixed sizes and energies with electron energy was quantised.
  • In 1926, Erwin Schrödinger stated that electrons do not move in set paths around the nucleus, but in waves and it is impossible to know the exact location of the electrons.

The Electronic Structure of Atoms

  • Continuous vs. (atomic) line emission spectra are discussed.
  • In 1913, Niels Bohr proposed that electrons do NOT whirl around the nucleus like a solar system, but instead can only occupy certain “orbits” of specific energies.
  • The energy of electrons is quantized, and atoms and molecules have only certain allowable, discrete energy levels.
  • Unique for each atom / ion / molecule / system.

The Bohr Model

  • "n" represent an “orbit”, or “energy level".
  • n=1 is the ground state.
  • n>1 is the excited state.
  • As "n" increases distance from the nucleus increases as n increases and energy levels get closer and closer in proximity (exponential function).
  • For an electron in the Hydrogen atom: En = the energy of an electron in orbit "n" (J).
  • R = 3.29 x 10^15 s^-1.
  • h = Planck's constant = 6.626 x 10^-34 J*s.
  • Bohr attributed the emission of radiation by an energized hydrogen atom to an electron transitioning from a higher energy orbit to a lower energy orbit, emitting a "quantum" (photon) of energy in the form of light.

Importance and Limitations of the Bohr Model

  • The importance of the Bohr model is that it introduced the concept that electrons exist in energy levels.
  • As electrons transition between levels, energy is exchanged.
  • Limitations of the Bohr model are that it describes electrons in specific orbits, like books on a shelf, in an exact position and explains the Hydrogen atom EXACTLY, but is applicable for only one electron systems.
  • De Broglie asserted that a moving particle (such as an electron) also has wave-like properties.
  • Quantum mechanics is a more comprehensive way to understand the structure of the atom, which accounts for wave-particle duality, the quantization of energy, and the Heisenberg Uncertainty Principle.
  • Heisenberg uncertainty principle: it is impossible to simultaneously know both the position and momentum of an electron.

Quantum Mechanics and the Schrödinger Equation

  • In 1926, Erwin Schrodinger formulated an equation that describes the location and behavior of an electron in an atom.
  • Incorporates both particle behavior (mass) and wave behavior (wavefunctions, ψ).
  • Electron wavefunction in radial coordinates ψ(r,θ,φ) can be separated into a radial and an angular part.
  • Energy states and wave functions (ψ) of an electron are characterized by a set of quantum numbers.
  • Four quantum numbers describe the distribution and behavior of electrons in an atom.
    1. Principal quantum number (n).
    1. Angular momentum quantum number (1)→ distribution] "Orbital".
    1. Magnetic quantum number (mℓ).
    1. Magnetic spin quantum number (Ms).

Quantum Numbers: Atomic Orbitals, Nodes, and Radial Distribution Plots

Quantum Numbers

  • Principal quantum number (n) designates the size and energy and is referred to as energy level or shell.
  • Higher n value = larger shell = further from nucleus, with allowed integer values.
  • Angular momentum quantum number (ℓ), or subshell, primarily designates the shape of an orbital.
  • Allowed values depend on n can be n=0 to n=-1 with numbers corresponding to letter designations: 0 → s, 1 → p, 2 → d, 3 → f.

Quantum Numbers

  • Magnetic quantum number (m₁) is referred to as orbital, and primarily designates the orientation in space (x, y, z).
  • Allowed values depend on l and can be -l... 0...+l.
  • The wave function of an electron in an atom is a depiction of the physical region around the nucleus that encloses 90% of the total electron probability.
  • Magnetic spin quantum number (ms) describes the spin of an electron within an orbital and only two possible values + 1/2 or -1/2 (spin up or spin down).
  • The maximum number of electrons per orbital = 2.

Nodes

  • A node is a point in which the probability of finding electron density in an atom is zero.
  • The position on a standing wave where the amplitude is zero.
  • The total number of nodes for an orbital = n-1.
  • Two types: planar (angular) and radial.
  • Planar (angular) nodes (nodes that are planar) are dictated by orbital shape and the # of planar nodes = ℓ.
  • Radial nodes (spherical) are dictated by shape (l) and size (n), and the # radial nodes = n-l-1.

s-orbitals

  • As n increases, the number of nodes increases.

p-orbitals

  • px, py, and pz orbitals are shown.

d-orbitals

  • There is electron density on these axes/between ones on that plane.

Chemistry Across the Periodic Table

  • The chemistry of Main Group elements depends strongly on the s, p-orbitals.
  • The chemistry of Transition Metals elements depends strongly on the d-orbitals.

Quantum Numbers

  • Summary of allowable combinations of quantum numbers are provided.

Quantum Numbers

  • There are several practice questions related to providing a plausible set of 4 quantum numbers for an electron in each orbital. The questions are:
    • How many orbitals are there in the subshell designated ℓ = 2?
    • How many electrons can be contained in a 4d subshell?
    • Provide a plausible name for an atomic orbital with the following set of quantum numbers: n = 4, I = 1, mℓ = -1, m₃ = + ½.

Graphical Interpretation of Wavefunctions

  • (1) ψ = wavefunctions are solutions of the Schrodinger equation.
  • Crossing x-axis indicates a change in phase or amplitude.
  • (2) ψ² = probability density; the probability of finding an electron near distance (r), at location (x, y, z)
  • Amplitude is always positive.
  • Radial wavefunctions for 1s, 2s, and 3s orbitals are provided.

Radial Probability Distribution Functions

  • (3) Ψ²r² = radial probability distribution function: Probability of finding an electron at a given radius, summed over all directions (x,y,z) of an atom (accounting for volume). The number of times the curve touches the x-axis = # of radial nodes.
  • As n increases, the probability of finding an electron further away from the nucleus increases.
  • It's probable to find an electron near the nucleus but not in the nucleus.

Practice

  • Practice exam-like questions are provided given radial distribution plots and orbital shape, and what the orbital name is.
  • The bonus question is to provide a plausible set of 4 quantum numbers for an electron in each orbital.

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Explore the fundamental concepts of quantum mechanics. Questions cover wave-particle duality, the Schrödinger equation, the Heisenberg Uncertainty Principle, and the Bohr model. Test your knowledge of quantum mechanics.

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