Quantum Chemistry Flashcards
(223 cards)
Why was quantum theory developed?
Developed to explain various experimental observations that couldn’t be understood by prevailing ‘classical’ theories of physics
What is quantum theory?
It is based on several principles such as wave particle duality and quantisation.
What were 3 issues which puzzled classical physicists which led to the development of quantum theory?
Black body radiation
Photoelectric effect
Spectroscopic lines
What is a black body?
A black body is an idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency or angle of incidence. It does not reflect or transmit any radiation; instead, it absorbs all incoming radiation and re-emits it.
What was the issue with black body radiation?
The issue with understanding black body radiation in the late 19th and early 20th centuries was the failure of classical physics to explain the observed spectral distribution of the emitted radiation. According to classical electromagnetic theory, it was expected that the energy emitted by a black body would increase without bound as the wavelength of the radiation became shorter (known as the ultraviolet catastrophe).
The ultraviolet catastrophe problem arose because classical physics predicted that the intensity of radiation would increase without limit as the wavelength approached zero, leading to an infinite amount of energy. However, experimental observations, particularly the detailed measurements of black body radiation depicted a different behaviour.
Thus, physicists had to find a solution to the black body radiation
What was Planck’s solution to black body radiation?
He proposed that energy is quantised. This means that electroncs can only possess certain discrete energy values, and values between these quantised values aren’t permitted
He suggested that energy is emitted or absorbed in discrete packets or ‘quanta’, which is proportional to the frequency of radiation.
What was the formula to calculate the energy of a system / electron by Planck?
E = hv
E = energy
h = Planck’s constant
v = frequency of oscillation
What is planck’s constant
6.62607015×10^−34 Js-
What is the photoelectric effect? WHat was the issue with it?
Light / electromagnetic radiation can eject electrons from a metal, but only if its frequency is above a threshold frequency which is characteristic for every different metal. The emission of electrons occurs instantaneously and energy of the emitted electrons depends on the frequency of the incident light rather than intensity
However, this contradicted classical wave theories of light, which predicted a gradual increase in the emission of electrons with increasing light intensity, however intensity of light doesnt affect the energy of the emitted electrons.
What did EInstein propose in 1905?
That light has a particle nature as well as a wave nature. Light is quantised.
What is the formula that EInstein developed from Placnk’s formula? (energy of a photon)
E = hv = h x c /λ –> v = c / λ
E = energy
where v = frequency
c = speed of light = 3.0 x 10^8 ms^01
λ = wavelength
h = Planck’s constant
How did Louis de Broglie build on Einstein’s findings of the photoelectric effect
De Broglie built on this to further propose that if light can behave as a wave and a particle, why can’t matter such as electrons also have wave properties –> idea that electrons act as a wave-particle duality
He further suggested that the momentum (mv) of a particle should be related to its wavelength in the same way as a photon
What is the equation of momentum?
Stems from Einsteins special theory of relativity
p = E / c
Where p is momentum, E is energy and c is the speed of light
How can we combine both the equation of momentum and quantum theory?
To form the equation of :
λ = n / p = n / mv
where m = mass
v = velocity
h = planck’s constant
λ = wavelength
What were spectroscopic lines? WHat was the issue with it?
Spectroscopic lines refer to the discrete, well defined lines observed in a spectrum when light is dispersed. These lines represent specific wavelengths or frequencies of light emitted or absorbed by atoms or molecules.
The issue with spectroscopic lines for classical physicists arose when they attempted to explain the observed patterns using classical electromagnetic theory, which treats light as a continuous wave. This means that a heated object would emit radiation continuously across all wavelengths, forming a smooth and continuous spectrum. However, experimental observations showed distinct and well defined lines instead of a continuous spectrum
How did Bohr address the issue of spectroscopic lines
He further developed the quantum model of the atom through using the knowledge of both Einstein (quantised packets of energy for light) and Planck (quantisation of energy).
He suggested that electrons then exist in discrete energies with quantised electron orbits. The electrons in atoms could only exist in certain allowed energy levels, and transitions between these levels resulted in the emission or absorption of photons with specific energies corresponding to the observed spectral lines. This successfully addressed the issue of the defined spectroscopic lines
What was the Bohr model?
Bohr postulates that there is a set of circular orbits for electrons with specific, discrete radii, and energy (quantised) and that electrons could move in each orbit without radiating energy
What was the formula derived for the energy of an orbit ‘n’ in Bohr’s model?
This was derived by looking at the atomic spectra for hydrogen.
En = - (me^4) / (2h^2n^2) = - Er x 1/n^2
En = energy of a particular orbit ‘n’
h = planck’s constant
n is an integer 1,2,3… corresponding to Bohr’s discrete orbitals
Er = Rydberg’s constant - 2.18 x 10^-18 J
This means that only specifc values of E are allowed. Values between Er (n= 1) and Er (n=2) can’t be observed, etc. Has to be only these integers
What’s wrong with Bohr’s model?
According to classical physics, revolving charged particles radiate energy. Thus, electrons should continually lose energy and spiral into the nucleus
Bohr’s model could only explain the emission spectra of single electron atoms such as Hydrogen. It failed to predict the spectra of multielectron atoms
Bohr couldn’t offer a reason as to why an electron should actually have a discrete orbit or energy
How are changes in energy levels achieved?
They are done through the absorption or emission of photons.
Absorption involves increasing an energy level
Emission involves decreasing an energy level
What can electrons be thought of as?
As 3d standing waves, with an amplitude characterised by a wavefunction (𝚿)
A standing wave is also known as a stationary wave, its a combination of two waves moving in opposite directions, each having the same amplitude and frequency.
What is the lowest energy level of any standing wave called?
The fundamental
What are the energy levels after the fundamental called?
They are called ‘harmonics’ in order of how many waves it is after the fundamental
I.e. n= 1 –> fundamental –> 1 half wavelength
n = 2 –> First Harmonic –> 2 half wavelengths
n = 3 –> Second Harmonic –> 3 half wavelengths
n = 4 –> Third Harmonic –> 4 half wavelengths
And then the pattern continues
Each harmonic adds a half wavelength
WHat is a half wavelength
It is the distance between each node