Question: How do I duplicate a complex plot that was done in Wolfram math sofware?

Hi,

I have been trying to duplicate a solution to Schrodinger Eq from a utube video...the presenter use Wolfram software to graph and 

animate the plot...I have working on this all day..I a new user (several months)..any help would be appreciated.

I am attaching a screenshot

Thanks 

Frank

 

I am attaching my Maple worksheet for reference 
 

NULL

BELOW IS ADRESSING PARTICLE MOTION AND HOW ELECTRONS MOVE AROUND AND HOW MAGNETIC FIELDS AFFECTION THE MOTION OF ELECTRONS

 

PARTICLE MOTION "IGNORING SPIN" WILL COME BACK TO THAT

restart

with(Physics); interface(imaginaryunit = i)

Setup(hermitianoperators = {H, O__H, O__S}, realobjects = {`ℏ`, m, t, x_}, combinepowersofsamebase = true, mathematicalnotation = true)

[combinepowersofsamebase = true, hermitianoperators = {H, O__H, O__S}, mathematicalnotation = true, realobjects = {`ℏ`, m, t, x_}]

(1)

with(Physics[Vectors])

WAVE FUNCTION OF PARITCLE. t =time , x= some position vector

x_ = `<,>`(x, y, z)

x_ = Vector[column](%id = 36893489722226370188)

(2)

psi(t, x_)

psi(t, x_)

(3)

psi(t, x, y, z)

psi(t, x, y, z)

(4)

p_

p_

(5)

ψ is xome complex number with a real and imaginary number, the absolute value of abs(psi(t, x_))^2
`and`((is*the*probabilty*density*of*finding*the)*particle*at*postion*vector*x, at*time*t), ASSUME*SOME*POSITION*VECTOR*x, with*an*infintesmial*cube*around*it, infintesimal*volume*dV, PROBABILY*DENSITY*IS*abs(psi(t, x_))^2*dV, int(abs(psi(t, x_))^2, V) = 1

abs(psi(t, x_))^2

 

is*the^2*probabilty*density*of*finding*particle*at*postion*vector*x and at*time*t, ASSUME*SOME*POSITION*VECTOR*x, with*an*infintesmial*cube*around*it, infintesimal*volume*dV, PROBABILY*DENSITY*IS*abs(psi(t, x_))^2*dV, abs(psi(t, x_))^2*V = 1

(6)

THE ABOVE EQUATION IS TRUE IF THE WAVE FUNCTION IS "PROPERLY NORMALIZED"

THE WAVE FUNCTION EVOLVES IN TIME ACCORDING TO SCHRODINGER EQ

"`i&hbar;`(&PartialD;Psi)/(&PartialD;t)= -(`&hbar;`^(2))/(2 m)(((&PartialD;)^2)/((&PartialD;)^( )x^2)(psi)+((&PartialD;)^2)/((&PartialD;)^( )y^2)(psi)+((&PartialD;)^2)/((&PartialD;)^( )z^2)(psi))",
diff(psi, x, x)+diff(psi, y, y)+((diff(psi, z, z))*IS*THE*KENETIC*ENERGY*OF*THE)*PARTICLE

restart

psi(t, x, y, z)

psi(t, x, y, z)

(7)

Loading PDEtools

I*`&hbar;`*(diff(Ket(psi, t), t))

I*`&hbar;`*(diff(Ket(psi, t), t))

(8)

SElns := I*`&hbar;`*(diff(Ket(psi, t), t)); 'SElns'

SElns

(9)

SErhs1 := `&hbar;`^2*(diff(psi, t, x, x)+diff(psi, t, y, y)+diff(psi, t, z, z))/(2*m)

0

(10)

``

 

``

Classical physics example

KE = p^2/(2*m)

KE = (1/2)*p^2/m

(11)

KE = (p[x]^2+p[y]^2+p[z]^2)/(2*m)

KE = (1/2)*(p[x]^2+p[y]^2+p[z]^2)/m

(12)

QUANTUM MECHANICS

``

p[x] = `&hbar;`*(Diff(p[x], x))/(I)

p[x] = -I*`&hbar;`*(Diff(p[x], x))

(13)

 

p[x]^2 = Diff(rhs(p[x] = -I*`&hbar;`*(Diff(p[x], x))))

p[x]^2 = Diff(-I*`&hbar;`*(Diff(p[x], x)))

(14)

substituting each value of p[x], p[y],p[z]  IN EQ 11 is the KE

ONE VERY IMPORTANT SOLUTUION TO SE IS LISTED BELOW

psi(t, `#mover(mi("x"),mo("&rarr;"))`)= "Pi^(-3/(4)) sigma^(-3/(2))C(t)^(-3/(2))Exp((-1/(2))(((x)^(2))/(sigma^(2 )C(t)))+ ((i p *x-(i( p)^(2)(t/(`&hbar;`^())))/(2 m))/(C(t)))"

C(t) = 1 +  "(`i&hbar;` t))/((m sigma^(2))), sigma= initial position uncertainty of the particle,m,mass of particle"

```#mover(mi("p"),mo("&rarr;"))`=<p[x],p[y],p[z]>...just 3 Real no...this is NOT THE SAME AS EQ 14

There are 3 parmeters in the above eq σ (NOT PAULI), m ,`#mover(mi("p"),mo("&rarr;"))`

abs(psi(t, `#mover(mi("x"),mo("&rarr;"))`))^2 = 1/Pi^(3/2)Exp(-(`#mover(mi("x"),mo("&rarr;"))`-i*`#mover(mi("p"),mo("&rarr;"))`(t/m))^2/(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2))/(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2)^(3/2)

int(abs(psi(t, `#mover(mi("x",fontweight = "bold"),mo("&rarr;",fontweight = "bold"))`))^2, V) = 1

THE ABOVE FUNCTION WILL BE A MAXIMUM WHEN `#mover(mi("x"),mo("&rarr;"))` = `#mover(mi("p"),mo("&rarr;"))`*t/m

distribution,

n. 1. (Statistics) the set of possible values of a random variable, or points in a sample space , considered in terms of their theoretical or observed frequency . 2. also called generalized function. a generalization of the concept of a function, defined as continuous linear functionals  over spaces of infinitely differentiable functions, introduced so that all continuous functions possess partial distributional derivatives (also called Schwartzian derivatives) that are again distributions. This leads to so-called weak solutions of differential equations and is of importance in the theory of partial differential equations ...

THE EQ YIEDS A GAUSSIAN "BELL SHAPE IN 2 D ONLY, CANNOT BE DRAWN 3D, 
abs(psi)^2*y*axis, `#mover(mi("x"),mo("&rarr;"))` = `#mover(mi("p"),mo("&rarr;"))`*t*x*axis/m, width = sqrt(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2)*so*at*t and sqrt(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2)*so*at*t = ((0*this)*will*equal*sigma*initial*uncertainity*of*the*position*of)*the*particle

t→∞ width = `#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m)

``

restart

with(Student[VectorCalculus])

with(VectorCalculus)

with(plots)

 

ln(1) := ts

ts

(15)

ts := 2

2

(16)

sigma := 4

4

(17)

h := 1

1

(18)

M := 1

1

(19)

P := 1

1

(20)

x

x

(21)

psi(x, t)

psi(x, t)

(22)

I = sqrt(-1)

I = I

(23)

about(I)

I:
  All numeric values are properties as well as objects.
  Their location in the property lattice is obvious,
  in this case complex(extended_numeric).
 

 

h, I, ts, M

1, I, 2, 1

(24)

sigma^2

16

(25)

I*h*ts/M

2*I

(26)

 

about(I)

I:
  All numeric values are properties as well as objects.
  Their location in the property lattice is obvious,
  in this case complex(extended_numeric).
 

 

2+2*I

2+2*I

(27)

(-1/2)*(x^2)

-(1/2)*x^2

(28)

"((-1/2)((x^2)/((sigma^2+(I*h*(t/M))))"

NULL

-(1/2)*x^2/(2+2*I)

(-1/8+(1/8)*I)*x^2

(29)

``

``

"Exp(((-1/2)((x^2)/((sigma^2+(I*h*(t/M)))))+(((I *P* (x/h))- (I* ((P^2)/(2*M))*(t/h))/((1+(((I*h*t))/((M+sigma^2))))"

NULL

I*P*x/h

I*x

(30)

 

I*P^2*t/((2*M)*h)

((1/2)*I)*t

(31)

I*x-((1/2)*I)*t

I*x-((1/2)*I)*t

(32)

"((I *P* (x/h))- (I* ((P^2)/(2*M))*(t/h))/((1+(((I*h*t))/((M+sigma^2))))"

``

NULL

I*h*t

I*t

(33)

sigma^2+M

17

(34)

1+I*t*(1/17)

1+((1/17)*I)*t

(35)

(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t)

(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t)

(36)

NULL

exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

(37)

psi(x, t) = exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

psi(x, t) = exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

(38)

simplify(psi(x, t) = exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t)))

psi(x, t) = exp(-I*(-2*x+t)*(I*t+34)/((2*I)*t+34))

 

Explore(psi(x, t) = exp(VectorCalculus:-`-`(VectorCalculus:-`*`(VectorCalculus:-`*`(VectorCalculus:-`*`(I, `-`(2*x)+t), VectorCalculus:-`+`(VectorCalculus:-`*`(I, t), 34)), 1/VectorCalculus:-`+`(VectorCalculus:-`*`(VectorCalculus:-`*`(2, I), t), 34)))), parameters = [[t = 0 .. 40, controller = slider], [x = -20 .. 80, controller = slider]], loop = never, size = NoUserValue, numeric = false, echoexpression = true)

(39)

with(plots)

implicitplot(abs(psi(x, ts*t)), Re(psi(x, ts*t)), Im(psi(x, ts*t)), x = -20 .. 80, scaling = constrained)

Error, (in plots/implicitplot) invalid input: lhs received Im(psi(x, 2*t)), which is not valid for its 1st argument, expr

 

NULL


 

Download Lec7QuantumWaveSE.mw
 

NULL

BELOW IS ADRESSING PARTICLE MOTION AND HOW ELECTRONS MOVE AROUND AND HOW MAGNETIC FIELDS AFFECTION THE MOTION OF ELECTRONS

 

PARTICLE MOTION "IGNORING SPIN" WILL COME BACK TO THAT

restart

with(Physics); interface(imaginaryunit = i)

Setup(hermitianoperators = {H, O__H, O__S}, realobjects = {`&hbar;`, m, t, x_}, combinepowersofsamebase = true, mathematicalnotation = true)

[combinepowersofsamebase = true, hermitianoperators = {H, O__H, O__S}, mathematicalnotation = true, realobjects = {`&hbar;`, m, t, x_}]

(1)

with(Physics[Vectors])

WAVE FUNCTION OF PARITCLE. t =time , x= some position vector

x_ = `<,>`(x, y, z)

x_ = Vector[column](%id = 36893489722226370188)

(2)

psi(t, x_)

psi(t, x_)

(3)

psi(t, x, y, z)

psi(t, x, y, z)

(4)

p_

p_

(5)

ψ is xome complex number with a real and imaginary number, the absolute value of abs(psi(t, x_))^2
`and`((is*the*probabilty*density*of*finding*the)*particle*at*postion*vector*x, at*time*t), ASSUME*SOME*POSITION*VECTOR*x, with*an*infintesmial*cube*around*it, infintesimal*volume*dV, PROBABILY*DENSITY*IS*abs(psi(t, x_))^2*dV, int(abs(psi(t, x_))^2, V) = 1

abs(psi(t, x_))^2

 

is*the^2*probabilty*density*of*finding*particle*at*postion*vector*x and at*time*t, ASSUME*SOME*POSITION*VECTOR*x, with*an*infintesmial*cube*around*it, infintesimal*volume*dV, PROBABILY*DENSITY*IS*abs(psi(t, x_))^2*dV, abs(psi(t, x_))^2*V = 1

(6)

THE ABOVE EQUATION IS TRUE IF THE WAVE FUNCTION IS "PROPERLY NORMALIZED"

THE WAVE FUNCTION EVOLVES IN TIME ACCORDING TO SCHRODINGER EQ

"`i&hbar;`(&PartialD;Psi)/(&PartialD;t)= -(`&hbar;`^(2))/(2 m)(((&PartialD;)^2)/((&PartialD;)^( )x^2)(psi)+((&PartialD;)^2)/((&PartialD;)^( )y^2)(psi)+((&PartialD;)^2)/((&PartialD;)^( )z^2)(psi))",
diff(psi, x, x)+diff(psi, y, y)+((diff(psi, z, z))*IS*THE*KENETIC*ENERGY*OF*THE)*PARTICLE

restart

psi(t, x, y, z)

psi(t, x, y, z)

(7)

Loading PDEtools

I*`&hbar;`*(diff(Ket(psi, t), t))

I*`&hbar;`*(diff(Ket(psi, t), t))

(8)

SElns := I*`&hbar;`*(diff(Ket(psi, t), t)); 'SElns'

SElns

(9)

SErhs1 := `&hbar;`^2*(diff(psi, t, x, x)+diff(psi, t, y, y)+diff(psi, t, z, z))/(2*m)

0

(10)

``

 

``

Classical physics example

KE = p^2/(2*m)

KE = (1/2)*p^2/m

(11)

KE = (p[x]^2+p[y]^2+p[z]^2)/(2*m)

KE = (1/2)*(p[x]^2+p[y]^2+p[z]^2)/m

(12)

QUANTUM MECHANICS

``

p[x] = `&hbar;`*(Diff(p[x], x))/(I)

p[x] = -I*`&hbar;`*(Diff(p[x], x))

(13)

 

p[x]^2 = Diff(rhs(p[x] = -I*`&hbar;`*(Diff(p[x], x))))

p[x]^2 = Diff(-I*`&hbar;`*(Diff(p[x], x)))

(14)

substituting each value of p[x], p[y],p[z]  IN EQ 11 is the KE

ONE VERY IMPORTANT SOLUTUION TO SE IS LISTED BELOW

psi(t, `#mover(mi("x"),mo("&rarr;"))`)= "Pi^(-3/(4)) sigma^(-3/(2))C(t)^(-3/(2))Exp((-1/(2))(((x)^(2))/(sigma^(2 )C(t)))+ ((i p *x-(i( p)^(2)(t/(`&hbar;`^())))/(2 m))/(C(t)))"

C(t) = 1 +  "(`i&hbar;` t))/((m sigma^(2))), sigma= initial position uncertainty of the particle,m,mass of particle"

```#mover(mi("p"),mo("&rarr;"))`=<p[x],p[y],p[z]>...just 3 Real no...this is NOT THE SAME AS EQ 14

There are 3 parmeters in the above eq σ (NOT PAULI), m ,`#mover(mi("p"),mo("&rarr;"))`

abs(psi(t, `#mover(mi("x"),mo("&rarr;"))`))^2 = 1/Pi^(3/2)Exp(-(`#mover(mi("x"),mo("&rarr;"))`-i*`#mover(mi("p"),mo("&rarr;"))`(t/m))^2/(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2))/(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2)^(3/2)

int(abs(psi(t, `#mover(mi("x",fontweight = "bold"),mo("&rarr;",fontweight = "bold"))`))^2, V) = 1

THE ABOVE FUNCTION WILL BE A MAXIMUM WHEN `#mover(mi("x"),mo("&rarr;"))` = `#mover(mi("p"),mo("&rarr;"))`*t/m

distribution,

n. 1. (Statistics) the set of possible values of a random variable, or points in a sample space , considered in terms of their theoretical or observed frequency . 2. also called generalized function. a generalization of the concept of a function, defined as continuous linear functionals  over spaces of infinitely differentiable functions, introduced so that all continuous functions possess partial distributional derivatives (also called Schwartzian derivatives) that are again distributions. This leads to so-called weak solutions of differential equations and is of importance in the theory of partial differential equations ...

THE EQ YIEDS A GAUSSIAN "BELL SHAPE IN 2 D ONLY, CANNOT BE DRAWN 3D, 
abs(psi)^2*y*axis, `#mover(mi("x"),mo("&rarr;"))` = `#mover(mi("p"),mo("&rarr;"))`*t*x*axis/m, width = sqrt(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2)*so*at*t and sqrt(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2)*so*at*t = ((0*this)*will*equal*sigma*initial*uncertainity*of*the*position*of)*the*particle

t→∞ width = `#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m)

``

restart

with(Student[VectorCalculus])

with(VectorCalculus)

with(plots)

 

ln(1) := ts

ts

(15)

ts := 2

2

(16)

sigma := 4

4

(17)

h := 1

1

(18)

M := 1

1

(19)

P := 1

1

(20)

x

x

(21)

psi(x, t)

psi(x, t)

(22)

I = sqrt(-1)

I = I

(23)

about(I)

I:
  All numeric values are properties as well as objects.
  Their location in the property lattice is obvious,
  in this case complex(extended_numeric).
 

 

h, I, ts, M

1, I, 2, 1

(24)

sigma^2

16

(25)

I*h*ts/M

2*I

(26)

 

about(I)

I:
  All numeric values are properties as well as objects.
  Their location in the property lattice is obvious,
  in this case complex(extended_numeric).
 

 

2+2*I

2+2*I

(27)

(-1/2)*(x^2)

-(1/2)*x^2

(28)

"((-1/2)((x^2)/((sigma^2+(I*h*(t/M))))"

NULL

-(1/2)*x^2/(2+2*I)

(-1/8+(1/8)*I)*x^2

(29)

``

``

"Exp(((-1/2)((x^2)/((sigma^2+(I*h*(t/M)))))+(((I *P* (x/h))- (I* ((P^2)/(2*M))*(t/h))/((1+(((I*h*t))/((M+sigma^2))))"

NULL

I*P*x/h

I*x

(30)

 

I*P^2*t/((2*M)*h)

((1/2)*I)*t

(31)

I*x-((1/2)*I)*t

I*x-((1/2)*I)*t

(32)

"((I *P* (x/h))- (I* ((P^2)/(2*M))*(t/h))/((1+(((I*h*t))/((M+sigma^2))))"

``

NULL

I*h*t

I*t

(33)

sigma^2+M

17

(34)

1+I*t*(1/17)

1+((1/17)*I)*t

(35)

(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t)

(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t)

(36)

NULL

exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

(37)

psi(x, t) = exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

psi(x, t) = exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

(38)

simplify(psi(x, t) = exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t)))

psi(x, t) = exp(-I*(-2*x+t)*(I*t+34)/((2*I)*t+34))

 

Explore(psi(x, t) = exp(VectorCalculus:-`-`(VectorCalculus:-`*`(VectorCalculus:-`*`(VectorCalculus:-`*`(I, `-`(2*x)+t), VectorCalculus:-`+`(VectorCalculus:-`*`(I, t), 34)), 1/VectorCalculus:-`+`(VectorCalculus:-`*`(VectorCalculus:-`*`(2, I), t), 34)))), parameters = [[t = 0 .. 40, controller = slider], [x = -20 .. 80, controller = slider]], loop = never, size = NoUserValue, numeric = false, echoexpression = true)

(39)

with(plots)

implicitplot(abs(psi(x, ts*t)), Re(psi(x, ts*t)), Im(psi(x, ts*t)), x = -20 .. 80, scaling = constrained)

Error, (in plots/implicitplot) invalid input: lhs received Im(psi(x, 2*t)), which is not valid for its 1st argument, expr

 

NULL


 

Download Lec7QuantumWaveSE.mw
 

NULL

BELOW IS ADRESSING PARTICLE MOTION AND HOW ELECTRONS MOVE AROUND AND HOW MAGNETIC FIELDS AFFECTION THE MOTION OF ELECTRONS

 

PARTICLE MOTION "IGNORING SPIN" WILL COME BACK TO THAT

restart

with(Physics); interface(imaginaryunit = i)

Setup(hermitianoperators = {H, O__H, O__S}, realobjects = {`&hbar;`, m, t, x_}, combinepowersofsamebase = true, mathematicalnotation = true)

[combinepowersofsamebase = true, hermitianoperators = {H, O__H, O__S}, mathematicalnotation = true, realobjects = {`&hbar;`, m, t, x_}]

(1)

with(Physics[Vectors])

WAVE FUNCTION OF PARITCLE. t =time , x= some position vector

x_ = `<,>`(x, y, z)

x_ = Vector[column](%id = 36893489722226370188)

(2)

psi(t, x_)

psi(t, x_)

(3)

psi(t, x, y, z)

psi(t, x, y, z)

(4)

p_

p_

(5)

ψ is xome complex number with a real and imaginary number, the absolute value of abs(psi(t, x_))^2
`and`((is*the*probabilty*density*of*finding*the)*particle*at*postion*vector*x, at*time*t), ASSUME*SOME*POSITION*VECTOR*x, with*an*infintesmial*cube*around*it, infintesimal*volume*dV, PROBABILY*DENSITY*IS*abs(psi(t, x_))^2*dV, int(abs(psi(t, x_))^2, V) = 1

abs(psi(t, x_))^2

 

is*the^2*probabilty*density*of*finding*particle*at*postion*vector*x and at*time*t, ASSUME*SOME*POSITION*VECTOR*x, with*an*infintesmial*cube*around*it, infintesimal*volume*dV, PROBABILY*DENSITY*IS*abs(psi(t, x_))^2*dV, abs(psi(t, x_))^2*V = 1

(6)

THE ABOVE EQUATION IS TRUE IF THE WAVE FUNCTION IS "PROPERLY NORMALIZED"

THE WAVE FUNCTION EVOLVES IN TIME ACCORDING TO SCHRODINGER EQ

"`i&hbar;`(&PartialD;Psi)/(&PartialD;t)= -(`&hbar;`^(2))/(2 m)(((&PartialD;)^2)/((&PartialD;)^( )x^2)(psi)+((&PartialD;)^2)/((&PartialD;)^( )y^2)(psi)+((&PartialD;)^2)/((&PartialD;)^( )z^2)(psi))",
diff(psi, x, x)+diff(psi, y, y)+((diff(psi, z, z))*IS*THE*KENETIC*ENERGY*OF*THE)*PARTICLE

restart

psi(t, x, y, z)

psi(t, x, y, z)

(7)

Loading PDEtools

I*`&hbar;`*(diff(Ket(psi, t), t))

I*`&hbar;`*(diff(Ket(psi, t), t))

(8)

SElns := I*`&hbar;`*(diff(Ket(psi, t), t)); 'SElns'

SElns

(9)

SErhs1 := `&hbar;`^2*(diff(psi, t, x, x)+diff(psi, t, y, y)+diff(psi, t, z, z))/(2*m)

0

(10)

``

 

``

Classical physics example

KE = p^2/(2*m)

KE = (1/2)*p^2/m

(11)

KE = (p[x]^2+p[y]^2+p[z]^2)/(2*m)

KE = (1/2)*(p[x]^2+p[y]^2+p[z]^2)/m

(12)

QUANTUM MECHANICS

``

p[x] = `&hbar;`*(Diff(p[x], x))/(I)

p[x] = -I*`&hbar;`*(Diff(p[x], x))

(13)

 

p[x]^2 = Diff(rhs(p[x] = -I*`&hbar;`*(Diff(p[x], x))))

p[x]^2 = Diff(-I*`&hbar;`*(Diff(p[x], x)))

(14)

substituting each value of p[x], p[y],p[z]  IN EQ 11 is the KE

ONE VERY IMPORTANT SOLUTUION TO SE IS LISTED BELOW

psi(t, `#mover(mi("x"),mo("&rarr;"))`)= "Pi^(-3/(4)) sigma^(-3/(2))C(t)^(-3/(2))Exp((-1/(2))(((x)^(2))/(sigma^(2 )C(t)))+ ((i p *x-(i( p)^(2)(t/(`&hbar;`^())))/(2 m))/(C(t)))"

C(t) = 1 +  "(`i&hbar;` t))/((m sigma^(2))), sigma= initial position uncertainty of the particle,m,mass of particle"

```#mover(mi("p"),mo("&rarr;"))`=<p[x],p[y],p[z]>...just 3 Real no...this is NOT THE SAME AS EQ 14

There are 3 parmeters in the above eq σ (NOT PAULI), m ,`#mover(mi("p"),mo("&rarr;"))`

abs(psi(t, `#mover(mi("x"),mo("&rarr;"))`))^2 = 1/Pi^(3/2)Exp(-(`#mover(mi("x"),mo("&rarr;"))`-i*`#mover(mi("p"),mo("&rarr;"))`(t/m))^2/(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2))/(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2)^(3/2)

int(abs(psi(t, `#mover(mi("x",fontweight = "bold"),mo("&rarr;",fontweight = "bold"))`))^2, V) = 1

THE ABOVE FUNCTION WILL BE A MAXIMUM WHEN `#mover(mi("x"),mo("&rarr;"))` = `#mover(mi("p"),mo("&rarr;"))`*t/m

distribution,

n. 1. (Statistics) the set of possible values of a random variable, or points in a sample space , considered in terms of their theoretical or observed frequency . 2. also called generalized function. a generalization of the concept of a function, defined as continuous linear functionals  over spaces of infinitely differentiable functions, introduced so that all continuous functions possess partial distributional derivatives (also called Schwartzian derivatives) that are again distributions. This leads to so-called weak solutions of differential equations and is of importance in the theory of partial differential equations ...

THE EQ YIEDS A GAUSSIAN "BELL SHAPE IN 2 D ONLY, CANNOT BE DRAWN 3D, 
abs(psi)^2*y*axis, `#mover(mi("x"),mo("&rarr;"))` = `#mover(mi("p"),mo("&rarr;"))`*t*x*axis/m, width = sqrt(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2)*so*at*t and sqrt(sigma^2+(`#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m))^2)*so*at*t = ((0*this)*will*equal*sigma*initial*uncertainity*of*the*position*of)*the*particle

t→∞ width = `#msup(mi("&hbar;"),mo("&InvisibleTimes;"))`*t/(sigma*m)

``

restart

with(Student[VectorCalculus])

with(VectorCalculus)

with(plots)

 

ln(1) := ts

ts

(15)

ts := 2

2

(16)

sigma := 4

4

(17)

h := 1

1

(18)

M := 1

1

(19)

P := 1

1

(20)

x

x

(21)

psi(x, t)

psi(x, t)

(22)

I = sqrt(-1)

I = I

(23)

about(I)

I:
  All numeric values are properties as well as objects.
  Their location in the property lattice is obvious,
  in this case complex(extended_numeric).
 

 

h, I, ts, M

1, I, 2, 1

(24)

sigma^2

16

(25)

I*h*ts/M

2*I

(26)

 

about(I)

I:
  All numeric values are properties as well as objects.
  Their location in the property lattice is obvious,
  in this case complex(extended_numeric).
 

 

2+2*I

2+2*I

(27)

(-1/2)*(x^2)

-(1/2)*x^2

(28)

"((-1/2)((x^2)/((sigma^2+(I*h*(t/M))))"

NULL

-(1/2)*x^2/(2+2*I)

(-1/8+(1/8)*I)*x^2

(29)

``

``

"Exp(((-1/2)((x^2)/((sigma^2+(I*h*(t/M)))))+(((I *P* (x/h))- (I* ((P^2)/(2*M))*(t/h))/((1+(((I*h*t))/((M+sigma^2))))"

NULL

I*P*x/h

I*x

(30)

 

I*P^2*t/((2*M)*h)

((1/2)*I)*t

(31)

I*x-((1/2)*I)*t

I*x-((1/2)*I)*t

(32)

"((I *P* (x/h))- (I* ((P^2)/(2*M))*(t/h))/((1+(((I*h*t))/((M+sigma^2))))"

``

NULL

I*h*t

I*t

(33)

sigma^2+M

17

(34)

1+I*t*(1/17)

1+((1/17)*I)*t

(35)

(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t)

(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t)

(36)

NULL

exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

(37)

psi(x, t) = exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

psi(x, t) = exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t))

(38)

simplify(psi(x, t) = exp(I*x-((1/2)*I)*t+(I*x-((1/2)*I)*t)/(1+((1/17)*I)*t)))

psi(x, t) = exp(-I*(-2*x+t)*(I*t+34)/((2*I)*t+34))

 

Explore(psi(x, t) = exp(VectorCalculus:-`-`(VectorCalculus:-`*`(VectorCalculus:-`*`(VectorCalculus:-`*`(I, `-`(2*x)+t), VectorCalculus:-`+`(VectorCalculus:-`*`(I, t), 34)), 1/VectorCalculus:-`+`(VectorCalculus:-`*`(VectorCalculus:-`*`(2, I), t), 34)))), parameters = [[t = 0 .. 40, controller = slider], [x = -20 .. 80, controller = slider]], loop = never, size = NoUserValue, numeric = false, echoexpression = true)

(39)

with(plots)

implicitplot(abs(psi(x, ts*t)), Re(psi(x, ts*t)), Im(psi(x, ts*t)), x = -20 .. 80, scaling = constrained)

Error, (in plots/implicitplot) invalid input: lhs received Im(psi(x, 2*t)), which is not valid for its 1st argument, expr

 

NULL


 

Download Lec7QuantumWaveSE.mw

 

 

Please Wait...