Complex Numbers and Quantum Mechanics ... Quantum mechanics (on an atomic scale) attempts to solve for

Complex Numbers and Quantum Mechanics ... Quantum mechanics (on an atomic scale) attempts to solve for

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  • Quantum Mechanics

    Complex Numbers and Quantum Mechanics Julian Stetzler and David Shoup

    Department of Math and Science, Alvernia University, 400 St. Bernardine St., Reading, PA 19607

    Introduction to Complex Numbers

    Acknowledgements This work was funded by Alvernia University’s Student Undergraduate Research Fellows (SURF) Program and the Math and Science Department.

    Applications of Quantum Theories References

    Click to add text

    Complex numbers can be written in the form π‘Žπ‘Ž + 𝑏𝑏𝑏𝑏 where 𝑏𝑏 = βˆ’1. So real numbers exist in the complex plane with imaginary part 𝑏𝑏 = 0. Complex analysis has provided many important theorems that allow us to solve difficult problems easily.

    Leonard Euler developed the relationship between trigonometric functions (wave functions) and complex numbers:

    π‘’π‘’π‘–π‘–πœƒπœƒ = cos πœƒπœƒ + 𝑏𝑏 sin πœƒπœƒ

    This equation gives an understanding of solutions to SchrΓΆdinger’s equation, which is the foundation of quantum mechanics.

    1. Griffiths, David and Schroeter, Darrell, β€œIntroduction to Quantum Mechanics”, 3rd Edition, Cambridge Univ Press, 2018

    2. Matthews, John, and Howell, Russell, β€œComplex Analysis for Mathematics and Engineering”, 5th Edition, Jones and Bartlett, 2006

    3. Welch, Kerri, β€œThe Texture of Time; The Meaning of Imaginary Time”, https://textureoftime.wordpress.com/2015/07/15/the-meaning-of- imaginary-time/

    4. Up and Atom, β€œWhat is the Schrodinger Equation, Actually?”, July 2018, retrieved from https://www.youtube.com/watch?v=QeUMFo8sODk

    One of the most well-known theories from quantum mechanics is the Heisenberg uncertainty principle. This principle states

    𝜎𝜎π‘₯π‘₯πœŽπœŽπ‘π‘ β‰₯ ℏ 2

    where 𝜎𝜎π‘₯π‘₯ is the standard deviation of position, πœŽπœŽπ‘π‘ is the standard deviation of the momentum, and ℏ is plank’s constant over 2Ο€. This means that the uncertainty of the position and momentum must always be greater than or equal to some positive real number. Thus, no matter how precise the measurements, there always exists some level of uncertainty. We cannot have both position and momentum of a quantum particle well-defined simultaneously, because gaining certainty about one quantity necessarily involves losing certainty about the other.

    Heisenberg's uncertainty principle is a specific case of a more general theory of uncertainty. The more general principle takes the form

    𝜎𝜎𝐴𝐴𝜎𝜎𝐡𝐡 β‰₯ 1 2𝑏𝑏

    [�̂�𝐴, �𝐡𝐡 2

    and states that overall uncertainty in the two incompatible observables must always exceed a particular threshold. For example, energy and time exhibit this property

    Δ𝑑𝑑Δ𝐸𝐸 β‰₯ ℏ 2

    Classical mechanics predicts the behavior of some mass π‘šπ‘š being acted upon by a force 𝐹𝐹(π‘₯π‘₯, 𝑑𝑑). Given initial conditions, we can determine β€’ Position π‘₯π‘₯(𝑑𝑑) β€’ Velocity 𝑣𝑣 𝑑𝑑 = 𝑑𝑑π‘₯π‘₯

    𝑑𝑑𝑑𝑑 β€’ Momentum 𝑝𝑝 𝑑𝑑 = π‘šπ‘š οΏ½ 𝑣𝑣(𝑑𝑑) β€’ Kinetic Energy 𝑇𝑇 𝑑𝑑 = 1

    2 οΏ½ π‘šπ‘š οΏ½ 𝑣𝑣(𝑑𝑑)2

    β€’ Other variables of interest

    Quantum mechanics (on an atomic scale) attempts to solve for the likely behavior of a particle subject to SchrΓΆdinger’s equation

    𝑏𝑏ℏ πœ•πœ•Ρ° πœ•πœ•π‘‘π‘‘

    = βˆ’ ℏ2

    2π‘šπ‘š πœ•πœ•2Ξ¨ πœ•πœ•π‘₯π‘₯2

    + 𝑉𝑉Ψ

    β€’ Ξ¨ π‘₯π‘₯, 𝑑𝑑 is the particle’s wave function, which determines the likelihood of finding the particle at a point π‘₯π‘₯ at a given time 𝑑𝑑. The probability is found by determining the area under the graph of |Ξ¨ π‘₯π‘₯, 𝑑𝑑 |2.

    β€’ ℏ is Planck's constant over 2Ο€ β€’ π‘šπ‘š is the mass of the particle β€’ 𝑏𝑏 = βˆ’1 β€’ 𝑉𝑉 is the potential energy function

    The Uncertainty Principle

    Solving the SchrΓΆdinger Equation The SchrΓΆdinger equation can be solved by separation of variables. We first assume solutions of the form

    Ξ¨ π‘₯π‘₯, 𝑑𝑑 = πœ“πœ“(π‘₯π‘₯)πœ‘πœ‘(𝑑𝑑) and while this seems restrictive, we will be able to patch together the separate solutions πœ“πœ“(π‘₯π‘₯) and πœ‘πœ‘(𝑑𝑑) to arrive at the more general solution. Essentially, we must solve both

    π‘‘π‘‘πœ‘πœ‘ 𝑑𝑑𝑑𝑑

    = βˆ’ 𝑏𝑏𝐸𝐸 Δ§ πœ‘πœ‘

    which is easily solvable as an ordinary differential equation with solution

    πœ‘πœ‘ 𝑑𝑑 = 𝑒𝑒 βˆ’π‘–π‘–π‘–π‘–π‘–π‘– Δ§

    and the equation

    βˆ’ Δ§2

    2π‘šπ‘š 𝑑𝑑2πœ“πœ“ 𝑑𝑑π‘₯π‘₯2

    + π‘‰π‘‰πœ“πœ“ = πΈπΈπœ“πœ“ which depends on the potential function 𝑉𝑉(π‘₯π‘₯) in the problem. This differential equation yields an infinite collection of solutions πœ“πœ“1 π‘₯π‘₯ ,πœ“πœ“2 π‘₯π‘₯ , … ,πœ“πœ“π‘›π‘› π‘₯π‘₯ , … , but the linear combination of these solutions multiplied by πœ‘πœ‘ 𝑑𝑑 and summed together yields the general solution to the SchrΓΆdinger equation. All of this provides us with β€’ Stationary states (long term solutions) that are independent of time. β€’ States of definite total energy: unlike classical mechanics where matter can take on any energy level,

    including zero, particles on the quantum level are bound to specific energy levels, and thus may never remain still.

    β€’ A general solution that allows us to compute the likely location of the particle given the potential energy of the system.

    And the

    As an example, consider the infinite square well, consisting of infinite potential outside some finite zone (0,π‘Žπ‘Ž), and zero potential within the zone. In the classical mechanics sense, this is similar to a car on a frictionless track bouncing between two bumpers at constant speed. The car is equally likely to be found anywhere within the zone. But the quantum case is quite different.

    Using this particular potential 𝑉𝑉(π‘₯π‘₯), solutions of SchrΓΆdinger’s equation with initial conditions πœ“πœ“ 0 = πœ“πœ“ π‘Žπ‘Ž = 0 take the form of sine waves

    πœ“πœ“π‘›π‘› π‘₯π‘₯ = 2 π‘Žπ‘Ž

    sin π‘›π‘›πœ‹πœ‹ π‘Žπ‘Ž π‘₯π‘₯ , 𝑛𝑛 = 1,2,3, …

    which provide solutions for the various energy levels.

    The Atom Since quantum particles, such as electrons, can only exist in certain energy states, as determined by SchrΓΆdinger's equation and the effective potential of the atom being studied, we can accurately map the likely location of these particles as they orbit the nucleus.

    The easiest case is the hydrogen atom, which consists of only one electron orbiting a single proton. Solutions to SchrΓΆdinger's equation accurately model the orbital behavior of the electron as studied by chemists.

    2s orbital, with two bands corresponding to two peaks of the corresponding graph.

    Using complex numbers, physicists can use quantum theory to solve problems related to chemistry, optics, computing, telecommunications, medical imaging, and global positioning systems. As technology continues to improve, the demand for an understanding of the behavior of subatomic particles increases.

    2p orbital.

    Here the graph of |Ξ¨ π‘₯π‘₯, 𝑑𝑑 |2 provides the likeliest location of electrons, in terms of distance from the nucleus, for the 2s and 2p orbital energy levels. The actual orbital shapes are shown below. The darker areas represent high probabilities of finding the electron and the white space indicates no probability.

    Quantum Tunneling In classical mechanics if an object does not have enough energy to cross a potential barrier, it will not pass. In quantum mechanics, particles have a positive probability of passing through any finite potential barrier even if they do not have enough energy.

    https://textureoftime.wordpress.com/2015/07/15/the-meaning-of-imaginary-time/ https://www.youtube.com/watch?v=QeUMFo8sODk

    Slide Number 1