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The ψ2,1,0state –2p the state in which mI=0has most of its probability density along the z-axis, and so it is often referred to as a 2pzstate. To allow its probability density to stick out in other ways and thus facilitate various kinds of molecular bonding with other atoms, an atomic electron may assume a wave function that is an algebraic combination of multiple wave functions open to it. One such “hybrid state” is the sum ψ2,1,0=ψ2,1,-1(Note: Because the Schrodinger equation is a linear differential equation, a sum of solutions with the same energy is a solution with that energy. Also, normalization constants may be ignored in the following questions.)

(a) Write this wave function and its probability density in terms of r, θ, and ϕ, (Use the Euler formula to simplify your result.)

(b) In which of the following ways does this state differ from its parts (i.e., ψ2,1,+1and ψ2,1,-1) and from the 2pz state: Energy? Radial dependence of its probability density? Angular dependence of its probability density?

(c) This state is offer is often referred to as the 2pz. Why?

(d) How might we produce a 2pystate?

Short Answer

Expert verified

(a) Wave Function is 14a05/2πre-r/2asinθcosϕ.

Probability density is 116a05πre-r/a0sin2θcos2ϕ.

(b) They do not differ in energy, they have the same radial probability dependence but their angular probabilities differ.

(c) While , the angular factor in the 2pzis large along z, the angular factor here, sinθcosϕ, is large along .

(d) The required function will bere-r/2a0sinθ2isinϕ.

Step by step solution

01

A concept:

As you know that the probability density can be found by the square of the absolute value of the wave function. The wave function gives us the likelihood of finding an electron at a given point in space.

02

(a) Wave function and probability density:

Wave function is define by,

ψ2,1+1+ψ2,1,-1=1a05/224re-r/2a038πsinθe+iϕ1a05/224re-r/2a038πsinθe-iϕ=14a05/2πre-r/2a0sinθcosϕ

Probability Density is define by,

ψ2,1,+1+ψ2,1,-1*ψ2,1,+1+ψ2,1,-1=116a05πre-r/a0sin2θcos2ϕ

03

(b) Difference and dependence:

Energy of all n=2 states is same; hence, it does not differ in energy.

All 2p states will have the same R(r), and thus the same radial probability dependence. The wave function ψ2,1,0depends on cosθ,ψ2,1,+1depends on sinθe+iϕ,ψ2,1-1depends on sinθe-and the wave function depends on sinθcosϕ. Since these all differ, hence, their angular probabilities will also differ.

04

(c) Reason to be referred as 2pz:

Whilecosθ, the angular factor in the 2pzis large along z, the angular factor here, sinθcosϕ, is large along x.

05

(d) Production of 2py state:

You have,

ψ2,1,+1-ψ2,1,-1αre-r/2asinθe+-re-r/2a0sinθe-=re-r/2a0sinθ2isinϕ

This is large along the y-axis.

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Most popular questions from this chapter

A particle is subject to a potential energy that has an essentially infinitely high wall at the origin, like the infinite well, but for positive values of x is of the form U(x)= -b/ x, where b is a constant

(a) Sketch this potential energy.

(b) How much energy could a classical particle have and still be bound by such a potential energy?

(c) Add to your sketch a plot of E for a bound particle and indicate the outer classical tuning point (the inner being the origin).

(d) Assuming that a quantum-mechanical description is in order, sketch a plausible ground-state wave function, making sure that your function's second derivative is of the proper sign when U(x)is less than E and when it is greater.

Determine the Fourier transform A(k)of the oscillatory functionf(x) ) and interpret the result. (The identity cos(k0x)=12(e+ik0+eik0)may be useful.)

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(a) In which of the factors considered in nuclear binding (represented by terms in the semi empirical binding energy formula) do these two isobars differ?

(b) Which of the isobars should be more tightly bound?

(c) k your conclusion in part (b) supported by the decay mode information of Appendix 1? Explain.

(d) Calculate the binding energies of oxygen-15 and nitrogen-15. By how much do they differ?

(e) Repeat part (d) but use the semi empirical binding energy formula rather than the known atomic masses.

A particle of mass m and energy E moving in a region where there is initially no potential energy encounters a potential dip of width L and depth U=-Uo.

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