Semiclassical mechanics~

Let us hypothetically assume that you are an intergalactic spaceman and have just landed on a planet with gravitational acceleration g . g. You start an experiment which requires you to take a ball of mass m , m, drop it from height H , H, and calculate a quantity H 3 m 2 g H^3m^2g which you call the squared action . After lots of trials, you come to the conclusion that the minimum value of the squared action is a × 1 0 b . a \times 10^b.

Then what is the value of a + b a+|b| to 2 decimal places?

Hint: Think about the name of the quantity and also the title!


The answer is 68.8767.

This section requires Javascript.
You are seeing this because something didn't load right. We suggest you, (a) try refreshing the page, (b) enabling javascript if it is disabled on your browser and, finally, (c) loading the non-javascript version of this page . We're sorry about the hassle.

1 solution

Ouma Shu
Mar 2, 2018

The basic outline of the solution is as follows :

  • Calculate the mean and mean of squares of positions and from that calculate the standard deviation of position.
  • Apply the same recipe for momentum to calculate the standard deviation of momentum.
  • Apply Heisenberg's Uncertainty principle.

Throughout the problem, the downward direction will be considered positive.

Step 1 : Standard deviation of position :

Let x x be the position of the body at any time t t and let T T be the total time taken for the body to fall through a height H H . Then from the equations of free fall : x = 1 2 g t 2 x=\frac12gt^2 and T = 2 H g T=\sqrt{\frac{2H}{g}} .

Then, mean of position x = 0 T 1 2 g t 2 d t T 0 d t = g 6 ( t 3 ) 0 T T = H 3 \langle x\rangle = \frac { \int _{ 0 }^{ T }{ \frac { 1 }{ 2 } gt^{ 2 }dt } }{ \int _{ T }^{ 0 } dt } =\frac {\frac{ g }{ 6 } (t^{ 3 }) \Big|_0^T}{T}=\frac H3 using the value of T T as above.

Similarly, the mean of squares of position x 2 = 0 T ( 1 2 g t 2 ) 2 d t T 0 d t = g 2 20 ( t 5 ) 0 T T = H 2 5 \langle x^2 \rangle = \frac { \int _{ 0 }^{ T }{ (\frac { 1 }{ 2 } gt^{ 2 })^2dt } }{ \int _{ T }^{ 0 } dt } =\frac {\frac{ g ^2}{ 20 } (t^{ 5 }) \Big|_0^T}{T}=\frac {H^2}5 .

Thus standard deviation of position σ x = x 2 x 2 = H 2 5 H 2 9 = 4 H 2 45 = 2 H 3 5 \sigma _x = \sqrt{\langle x^2 \rangle - \langle x\rangle ^2} = \sqrt{\frac{H^2}{5}-\frac{H^2}{9}}=\sqrt\frac{4H^2}{45}=\frac{2H}{3\sqrt 5}

Step 2 : Standard deviation of momentum :

Let v v be the velocity of the body at any time t t . Then, p = m v = m g t p=mv=mgt .

Therefore, mean of momentum p = m g t d t T 0 d t = 1 2 m g ( t 2 ) 0 T T = m g H 2 g \langle p\rangle = \frac { \int {mgt \; dt } }{ \int _{ T }^{ 0 } dt } =\frac {\frac 12 mg \; (t^{ 2 }) \Big|_0^T}{T}=mg \sqrt{\frac{H}{2g}}

Similarly, the mean of squares of momentum p 2 = m 2 g 2 t 2 d t T 0 d t = 1 3 m 2 g 2 ( t 3 ) 0 T T = 2 3 m 2 g H \langle p^2 \rangle = \frac { \int {m^2g^2t^2 \; dt } }{ \int _{ T }^{ 0 } dt } =\frac {\frac 13 m^2g^2 \; (t^{ 3 }) \Big|_0^T}{T}=\frac23m^2gH

Thus standard deviation of momentum σ p = p 2 p 2 = 2 3 m 2 g H 1 2 m 2 g H = 1 6 m 2 g H = m g H 6 \sigma _p = \sqrt{\langle p^2 \rangle - \langle p\rangle ^2} = \sqrt{\frac23m^2gH-\frac12m^2gH}=\sqrt{\frac16m^2gH}=m\sqrt{\frac{gH}{6}}

Step 3 : Heisenberg's Uncertainty Principle :

We have, from definition : σ x σ p 2 \sigma_x \sigma_p \ge \frac{\hbar}{2}

Putting everything in : 2 H 3 5 m g H 6 2 \frac { 2H }{ 3\sqrt { 5 } } \cdot m\sqrt { \frac { gH }{ 6 } } \ge \frac { \hbar }{ 2 }

Squaring both sides and doing the necessary algebra yeilds : H 3 m 2 g 135 2 8 = 1.8767 × 1 0 67 H^3m^2g\ge\frac{135\hbar^2}{8} = 1.8767\times 10^{-67} which is of the form a × 1 0 b a\times 10^b .

Thus, a + b = 1.8767 + 67 = 68.8767 a+|b|=1.8767+|-67|=\boxed{68.8767} .

0 pending reports

×

Problem Loading...

Note Loading...

Set Loading...