Lecture 1: Introduction Quantum mechanics (QM) is one of two theories - - PowerPoint PPT Presentation

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Lecture 1: Introduction Quantum mechanics (QM) is one of two theories - - PowerPoint PPT Presentation

EE201/MSE207 Applied Quantum Mechanics Lecture 1: Introduction Quantum mechanics (QM) is one of two theories of 20 th century physics, which considerably changes our understand of nature. - Relativity changed our understanding of space and time.


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SLIDE 1

EE201/MSE207 Applied Quantum Mechanics Lecture 1: Introduction

Quantum mechanics (QM) is one of two theories of 20th century physics, which considerably changes our understand of nature.

  • Relativity changed our understanding of space and time.
  • QM changed the logic of thinking about microscopic objects.

Main philosophical ideas: wave-particle duality and indeterminism 𝐹 = β„πœ• (Planck-Einstein) for particles πœ‡ =

2πœŒβ„ π‘ž (de Broglie) for particles

ℏ = 1.05 Γ— 10βˆ’34 Jοƒ—s Estimates: Electron: πœ‡ =

2πœŒβ„ 2𝑛𝑓𝐹 = 1 nm 1.504 eV 𝐹

=

1.226 nm 𝐹[eV]

Photon: πœ‡ =

2πœŒπ‘‘ πœ• = 2πœŒβ„π‘‘ 𝐹

=

1.240 𝜈m 𝐹[eV]

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SLIDE 2

Prehistory of Quantum Mechanics

1) 1900 Max Planck: suggested discrete absorption and emission of light to explain experimental formula for black-body radiation (Nobel Prize 1918) 𝐹 = β„Žπœ‰ = β„πœ• β„Ž = 6.63 Γ— 10βˆ’34 Jοƒ—s ℏ = 1.05 Γ— 10βˆ’34 Jοƒ—s 2) 1905 Albert Einstein: theory of photoelectric effect (Nobel Prize 1921) β„Žπœ‰ = Ξ¦ +

𝑛𝑀2 2

Ξ¦ is work function (ionization energy) 3) 1913 Niels Bohr: model of atom (Nobel Prize 1922) Discrete atomic spectra and Rutherford’s experiments (1910-1911, N.P. 1908) 𝑛𝑀𝑠 = π‘œβ„ 4) 1923 Arthur Compton: scattering of X-rays on electrons (Nobel Prize 1927) 5) 1923 Louis de Broglie: matter waves (theory only, in 1927 confirmed for electrons, Nobel Prize 1929)

πœ‡ = 2πœŒβ„ π‘ž

β€œBirth” of Quantum mechanics: 1927 (5th Solvay conference, Brussels)

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SLIDE 3

Classical mechanics vs. Quantum Mechanics

(one particle in one dimension)

Position 𝑦(𝑒), velocity 𝑀 𝑒 =

𝑒𝑦 𝑒𝑒 , acceleration 𝑏 𝑒 = 𝑒2𝑦 𝑒𝑒2

𝐺 = βˆ’

π‘’π‘Š(𝑦) 𝑒𝑦

for a conservative system, π‘Š(𝑦) is potential energy Classical mechanics: Main evolution equation: 𝑏 =

𝐺 𝑛

𝑒2𝑦 𝑒𝑒2 = βˆ’ 1 𝑛 π‘’π‘Š 𝑒𝑦

initial conditions: 𝑦 0 , 𝑦(0)

οƒž

𝑦(𝑒) Quantum mechanics:

𝑗ℏ πœ–Ξ¨ πœ–π‘’ = βˆ’ ℏ2 2𝑛 πœ–2Ξ¨ πœ–π‘¦2 + π‘ŠΞ¨

Main evolution equation: SchrΓΆdinger equation Ξ¨(𝑦, 𝑒) is a complex function, characterizing the particle state (wave function) Ξ¨ 𝑦, 𝑒

2𝑒𝑦 is the probability to find the particle between 𝑦 and 𝑦 + 𝑒𝑦

at time 𝑒 (if observed!) Indeterminacy: particle does not have position (still debates about philosophy)