v = 20m/s,m = 0.5kg,h = 6.626 × 10-34 m2 kg / sΔp =p×1×10−6As we know that,
P = m×v = 0.5×20 = 10kgm/s
Δp = 10×1×10−6Δp = 10-5Heisenberg Uncertainty principle formula is given as,∆x∆p ∆x ∆x ∆x =0.527 x 10-29 mQ6) Prove non-existence of electrons in the nucleus?A 6)One of the applications is to prove that electron cannot exist inside the nucleus. But to prove it, let us assume that electrons exist in the nucleus. As the radius of the nucleus in approximately 10-14m. If electron is to exist inside the nucleus, then uncertainty in the position of the electron is given byAccording to uncertainty principle∆x ∆p =h/2πThus ∆p=h/2π∆xOr ∆p=6.62 x10-34/2 x 3.14 x 10-14Or ∆p=1.05 x 10-20 kg m/ secIf this is p the uncertainty in the momentum of electron, then the momentum of electron should be at least of this order that is p=1.05*10-20 kg m/sec.An electron having this much high momentum must have a velocity comparable to the velocity of light. Thus, its energy should be calculated by the following relativistic formulaE =
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From equation En is the energy value (Eigen Value) of the particle in a well. It is clear that the energy values of the particle in well are discrete not continuous.
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=-iω (x, t) and =- (π2/a2) (x, t) the Schrödinger equation yields Hence V(x,t) is time independent and given by (b) The probability of finding the particle in the interval a/4 x 3a/4.can be obtained from
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Substituting these values in the time dependendent Schrödinger equation, we have
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= ( - )2 = + -2pp’cosθ = ( + -2νν’cosθ) ………..(2) Energy Conservation The energies of the electron before and after the collision are given, respectively, by E0 =mec2 ………..(3)
Since the energies of the incident and scattered photons are given by E = hν and E0 = hν’, respectively, conservation of energy dictates that E + E0 = E’ + Ee ………..(4) ………..(5)
Which leads to ………..(6) Squaring both sides of (5) and simplifying, we get Hence wavelength shift is given by Where λC = h/mec = 2.426 x 10-12 m is called the Compton wavelength of the electron.
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(a) In the case where the photons backscatter i.e. θ = π The wavelength shift becomes = - = 2c sin2θ = 2c sin2 π = 2c = 2 x 2.426 x 10-12 m =4.86 x 10-12 m
(b) Since the energy of the scattered photons E’ is related to the wavelength by E =hc / Where E = hc/ is the energy of the incident photons. If E = mec2 we can approximate
(c) If E = 150 MeV, the kinetic energy of the recoiling electrons can be obtained from conservation of energy Ke = E – E’ 150 – 0.25 =14.75 MeV
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(4) that can be rearranged to give (5) It is convenient to define two new variables (both positive), one for regions 0 and 2, and one for region 1—they are wavenumbers: (6) (7) and Schrödinger’s equation becomes In regions 0 and 2 the general solution is a linear combination of exponentials with the same form, but with different constants, namely In region 1 we have the same general solution that we had for the infinite square well, Equations (10) to (12) have 7 unknowns—A,B,C,D,F,G and the energy E that is im-plicitly contained in the variables κ0,k1. Therefore we need to get 7 equations to be ableto solve for the unknowns. We will first use the requirement that the wavefunction remain finite everywhere. Consider ψ2 as x→∞. For this to remain finite we must require G= 0. Similarly, as x→−∞, we require A= 0. Our solutions become The next step is to require that the wavefunction and its first derivative be continuous everywhere, and in our case we look at the boundaries, x= 0 and x=L. Hence ψ0=D exp(+κ0x).Take derivatives of the wave functions,
There remain 3 unknowns, D,F, and E. Finding them is a bit messier! Consider the boundary conditions at x=L, We are not going much farther, but if we divided Equation (22) by Equation (23), we can see that the constants D and F cancel leaving us with one rather difficult equation to solve for energy E (remember this is implicitly included in the values of k1and κ0.) There is one remaining condition, normalization, that for this problem is Even without solving the entire problem we can make some conclusions about the wave-function and the allowed energy levels. Recall that for an infinite square well potential of width L the allowed energies are quantized and Here is Equation(22)/Equation(23) Now put in the values ofκ0andk1from Equations (6) and (7) and do some algebra to get This equation is a single equation in a single unknown, E < U0. Once we have the details of our particle (its mass) and the potential energy (depth U0 and width L), we can solve it. There is no analytic solution, only a numerical one. From equation (25) With n being any positive integer. Outside the well the wavefunction is 0. We are certain that the particle is somewhere inside the box, so ∆x ∞ =L. With the finite well, the wavefunction is not zero outside the well, Figure 9: Wave function in Finite well So ∆x finite> L, hence from the uncertainty principle, ∆pfinite x<∆p∞x. This suggests that the average value of momentum is less for the finite well, and therefore that the kinetic energy inside the well is less for the finite well than for the infinite well. Indeed this is borne out with detailed analysis. In addition, the number of allowed energy levels is finite, and there is a possibility that a well may be sufficiently narrow or sufficiently shallow that no energy levels are allowed. Also note that the non-zero wave functions in regions 0 and 2 mean that there is a non-zero probability of finding the particle in a region that is classically forbidden, a region where the total energy is less than the potential energy so that the kinetic energy is negative.
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