Contribution Of Scientists In Quantum Mechanics


Max Plank’s —The Blackbody Radiation

  •   In 1909 Max Plank’s introduced concept of Quantum of energy (photon) to explainBlackbody radiation.


  • He proposed that energy of radiation (light) is Quantized and dependent of frequency as 𝐸 = β„Žπ‘“

  • where h is the planck's constant of value β„Ž = 6.63×10−34𝐽 𝑠


Albert Einstein — The Photoelectric Effect

  •  In 1905 Einstein confirmed Planck's quantum concept.  

  • Einstein proposed that electromagnetic radiation (light) is quantized and exists in fixed amounts (quanta) or photons.

  • The introduction of the photon concept enabled Einstein to give explanation to the photoelectric problem, by Hertz in 1887.


Niels Bohr —The model of Hydrogen atom  

  • Bohr proposed that atoms can be found only in discrete states of energy.  

  • The emission or Absorption of radiation (or light) by atoms, takes place only in discrete amounts of 𝐸 = hf.


Arther Holly Compton — Compton’s effect 

  •  By scattering X-rays with electrons, He confirmed that the (X-ray) photons behave like particles.

  • Loss in photon energy = gain in electron energy.


de Broglie — Matter is a wave and waves are a matter too! 

  •  In 1923, de Broglie proposed that Matter waves.

  • He showed that wave nature of matter by relation πœ† = β„Ž / π‘šπ‘£ = β„Ž/ 𝑝

  • In 1927 by Davisson and Germer proved de Broglie hypothesis


Heisenberg — The Uncertainty Principle 

  •  In 1925 , Heisenberg proposed that it is impossible to determine the exact position and momentum at same time. Δ𝑝π‘₯. Ξ”π‘₯ ≥ ℏ / 2

  • There is always be the Uncertainty of ℏ.

  • He says that Quantum mechanics is a completely in-deterministic theory, no one knows the future state of particles. E.g three wings of rotating fans.

  • He formulated the Matrix Quantum Mechanics in which Eigen values are represented in matrices.


Erwin SchrΓΆdinger— The Schrodinger Wave Equation of Particle (SWE)

  •  In Quantum Mechanics Schrodinger Wave Equation play a same role like Newton’s Second Law: 𝐹 = π‘šπ‘Ž

  • In 1926, Schrodinger described the dynamics of microscopic particles with a wave equation called Schrodinger Wave Equation.

  • Schrodinger Wave Equation is 2nd order differential equation 

                   i.e 𝐻Ψ = 𝐸Ψ 

                      − ℏ2/2π‘š πœ•2Ξ¨/πœ•π‘₯2 + 𝑉(π‘Ÿ) = π‘–β„Ž πœ•Ξ¨/πœ•π‘‘ 

Where H is Hamilton Operator or Total Energy Operator, Ξ¨ is the wavefunction , E is the Energy Operator, V(r) is potential and ℏ is modified formed of Planck’s constant

 .i.e ℏ = β„Ž/2 = 1.054573 × 10−34𝐽𝑠 

  • The solution of SWE is a Wavefunction Ξ¨(π‘Ÿ,𝑑). A wavefunction completely describes the de-Broglie waves in space with respect to time. 

  • SchrΓΆdinger gave the wave formulation of Quantum Mechanics


Paul Dirac — Dirac Notations

  • An easy Notation of wave function 𝜳 and Relativistic approaches or Combined Quantum Mechanics and Special Relativity

  •  Dirac then suggested a more general formulation of quantum mechanics using two state vectors i.e Bras and Ket sVectors 

  •  The Kets notation of wavefunction Ξ¨ is |Ξ¨ > while Bra notation of Ξ¨ is < Ξ¨|.

  • Where Kets |Ξ¨ >= ∫ Ψ𝑑π‘₯ and Bras < Ξ¨| = ∫ Ψ𝑑x.







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