1Recap. 2 Quantum description of a particle in an infinite well  Imagine that we put particle (e.g. an electron) into an “infinite well” with width L.

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Presentation transcript:

1Recap

2 Quantum description of a particle in an infinite well  Imagine that we put particle (e.g. an electron) into an “infinite well” with width L (e.g. a potential trap with sufficiently high barrier)  In other words, the particle is confined within 0 < x < L

3 Particle forms standing wave within the infinite well  How would the wave function of the particle behave inside the well?  They form standing waves which are confined within 0 ≤ x ≤ L

4 Standing wave in general  Description of standing waves which ends are fixed at x = 0 and x = L. (for standing wave, the speed is constant), v = = constant) L = 1 /2 (n = 1) L =  (n = 2) L = 3 3 /2 (n = 3) L

5 mathematical description of standing waves  In general, the equation that describes a standing wave (with a constant width L) is simply: L = n n /2 n = 1, 2, 3, … (positive, discrete integer)  n characterises the “mode” of the standing wave  n = 1 mode is called the ‘fundamental’ or the first harminic  n = 2 is called the second harmonics, etc.  n are the wavelengths associated with the n-th mode standing waves  The lengths of n is “quantised” as it can take only discrete values according to n = 2L/n n = 2L/n

6 Energy of the particle in the box  Recall that  For such a free particle that forms standing waves in the box, it has no potential energy  It has all of its mechanical energy in the form of kinetic energy only  Hence, for the region 0 < x < L, we write the total energy of the particle as E = K + V = p 2 /2m + 0 = p 2 /2m

7 Energies of the particle are quantised  Due to the quantisation of the standing wave (which comes in the form of n = 2L/n ), n = 2L/n ),  the momentum of the particle must also be quantised due to de Broglie’s postulate: It follows that the total energy of the particle is also quantised:

8 The n = 1 state is a characteristic state called the ground state = the state with lowest possible energy (also called zero-point energy ) Ground state is usually used as the reference state when we refer to ``excited states’’ (n = 2, 3 or higher) The total energy of the n-th state can be expressed in term of the ground state energy as (n = 1,2,3,4…) (n = 1,2,3,4…) The higher n the larger is the energy level

9  Some terminology  n = 1 corresponds to the ground state  n = 2 corresponds to the first excited state, etc  Note that lowest possible energy for a particle in the box is not zero but E 0 (= E 1 ), the zero-point energy  This a result consistent with the Heisenberg uncertainty principle n =1 n =2 n =3 n = 1 is the ground state (fundamental mode): 2 nodes, 1 antinode n = 2 is the first excited state, 3 nodes, 2 antinodes n = 3 is the second excited state, 4 nodes, 3 antinodes

10 Simple analogy Cars moving in the right lane on the highway are in ‘excited states’ as they must travel faster (at least according to the traffic rules). Cars travelling in the left lane are in the ``ground state’’ as they can move with a relaxingly lower speed. Cars in the excited states must finally resume to the ground state (i.e. back to the left lane) when they slow down Ground stateexcited states

11 Example on energy levels  Consider an electron confined by electrical force to an infinitely deep potential well whose length L is 100 pm, which is roughly one atomic diameter. What are the energies of its three lowest allowed states and of the state with n = 15?  SOLUTION  For n = 1, the ground state, we have

12  The energy of the remaining states (n=2,3,15) are  When electron make a transition from the n = 3 excited state back to the ground state, does the energy of the system increase or decrease?

13  Solution: the energy of the system decreases as energy drops from 339 eV to 150 eV  The lost amount |  E| = E 3 - E 1 = 339 eV – 150 eV is radiated away in the form of electromagnetic wave with wavelength obeying  E = hc/  The lost amount |  E| = E 3 - E 1 = 339 eV – 150 eV is radiated away in the form of electromagnetic wave with wavelength obeying  E = hc/

14 Example radiation emitted during de-excitation  Calculate the wavelength of the electromagnetic radiation emitted when the excited system at n = 3 in the previous example de-excites to its ground state  Solution   =  hc/|  E| = 1240 nm. eV / (|E 3 - E 1 |) = 1240 nm. eV / (|E 3 - E 1 |)  = 1240 nm. eV / (299 eV – 150 eV) = = 8.3 nm = 8.3 nm n = 1 n = 3 Photon with = 8.3 nm

15 Example macroscopic particle’s quantum state  Consider a 1 microgram speck of dust moving back and forth between two rigid walls separated by 0.1 mm. It moves so slowly that it takes 100 s for the particle to cross this gap. What quantum number describes this motion?

16 Solution  The energy of the particle is  Solving for n in  Yields  This is a very large number. It is experimentally impossible to distinguish between the n = 3 x and n = 3 x states, so that the quantized nature of this motion would never reveal itself

17  The quantum states of a macroscopic particle cannot be experimentally discerned (as seen in previous example)  Effectively its quantum states appear as a continuum E(n=10 14 ) = 5x J allowed energies in classical system – appear continuous (such as energy carried by a wave; total mechanical energy of an orbiting planet, etc.) descret energies in quantised system – discrete (such as energy levels in an atom, energies carried by a photon)  E ≈ 5x /10 14 =1.67x = eV is too tiny to the discerned