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Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between trajectories is 90° - prove. But in relativistic mechanics the angle is < 90° due to increase of mass with . (squeezing in forward direction)

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Page 1: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

Lecture 11: Collisions (scattering)

Stationary particle hit by identical particle in an elastic collision

In Newtonian mechanics angle between trajectories is 90° - prove.

But in relativistic mechanics the angle is < 90° due to increase of mass with 𝑣.

(squeezing in forward direction)

Page 2: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

Collisions

Elastic: particles have same 𝐸0 = 𝑚0𝑐2 after collision.

Consider the special case, where after collision the particles travel at equal angles to direction of incident particle (viewed in lab frame)

To find 𝜃 in terms of 𝐸0, 𝐾1

Cons. of energy ⟹ 𝐸1 + 𝐸0 = 2𝐸2 (1)

Cons. of mom ⟹ 𝑝1 = 2𝑝2𝐶𝑜𝑠𝜃

2(2)

𝐸1 , 𝑝1 𝐸0 , 0

𝐸2 , 𝑝2

𝐸2 , 𝑝2

𝜃

2

𝜃

2

Page 3: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

Collisions

(1) 𝐸1 + 𝐸0 = 2𝐸2

(2) 𝑝1 = 2𝑝2𝐶𝑜𝑠𝜃

2

Also in rel. mechanics: 𝐸2 − 𝑝2𝑐2 = 𝑚02𝑐4 = 𝐸0

2

Thus 𝑝12𝑐2 = 𝐸1

2 − 𝐸02 (3)

𝑝22𝑐2 = 𝐸2

2 − 𝐸02 (3)

It is convenient to introduce 𝐾1 (K.E. of incident particle)

𝐸1 = 𝐸0 + 𝐾1 (4)

Page 4: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

Collisions

(1) 𝐸1 + 𝐸0 = 2𝐸2 (2) 𝑝1 = 2𝑝2𝐶𝑜𝑠𝜃

2

(3) 𝑝12𝑐2 = 𝐸1

2 − 𝐸02, 𝑝2

2𝑐2 = 𝐸22 − 𝐸0

2 (4) 𝐸1 = 𝐸0 + 𝐾1

(3),(4) ⇒ 𝑝12𝑐2 = 𝐸0 + 𝐾1

2 − 𝐸02 = 𝐾1(2𝐸0 + 𝐾1)

(3),(4),(1) ⇒ 𝑝22𝑐2 = 𝐸0 +

𝐾1

2

2− 𝐸0

2 = 𝐾1(𝐸0 +𝐾1

4)

Elastic collision ⇒ 𝐾𝑏𝑒𝑓𝑜𝑟𝑒 = 𝐾𝑎𝑓𝑡𝑒𝑟

∴ 2 ⇒ 4𝐶𝑜𝑠2𝜃

2=

2𝐸0 + 𝐾1

𝐸0 +𝐾14

𝐶𝑜𝑠2𝜃

2=

2𝐸0 + 𝐾1

4𝐸0 + 𝐾1

Page 5: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

Collisions

𝐶𝑜𝑠2𝜃

2=

2𝐸0 + 𝐾1

4𝐸0 + 𝐾1

We know 𝐶𝑜𝑠 𝜃 = 2𝐶𝑜𝑠2 𝜃

2− 1

∴ 𝐶𝑜𝑠 𝜃 =4𝐸0 + 2𝐾1

4𝐸0 + 𝐾1− 1

𝐶𝑜𝑠 𝜃 =𝐾1

4𝐸0 + 𝐾1

Newtonian case: 𝐾1 ≪ 𝐸0 : 𝐶𝑜𝑠 𝜃 = 0 , θ =𝜋

2

Relativistic case: 𝐾1 𝑛𝑜𝑡 ≪ 𝐸0 ∴ 𝜃 <𝜋

2

Proton rest mass energy: m0c2 = 900𝑀𝑒𝑉

Page 6: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

3-Dec-13 6

From Special Relativity by A. P. French

Page 7: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

3-Dec-13 7

From Special Relativity by A. P. French

Page 8: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

Compton Effect

Collision of photon (𝛾) with effectively free electron (𝑒)

A.H. Compton from 1919 to 1923 used x-ray photons and electrons loosely bound to atoms.

This collision is elastic in the sense that no energy is converted to other forms (rest mass).

But, energy is transferred from 𝛾 to 𝑒

ℎ𝑣 ↓ ∴ 𝜆 ↑

This is a very clear example of the particle nature of photons

Page 9: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

Compton Effect

𝜃

𝜑

𝐸2 , 𝑝2

𝐸, 𝑝

𝐸1 , 𝑝1

𝛾𝛾

𝑚0 , 𝐸0

𝑒 stationary rest mass 𝑚0

Remember p = 𝑚𝑣 =𝐸

𝑐2 𝑣 but 𝑣 = 𝑐 for photons

∴ 𝑝 =𝐸

𝑐

𝑝1 =𝐸1

𝑐 𝑛1 𝑝2 =

𝐸2

𝑐 𝑛2

𝑛1 and 𝑛2 are unit vectors

𝑒−

𝑛1

𝑛2

𝜃

Page 10: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

Compton Effect

Cons. energy ⇒ 𝐸1 + 𝑚0𝑐2 = 𝐸2 + 𝐸 (1)

Cons. Momentum ⇒𝐸1

𝑐 𝑛1 =

𝐸2

𝑐 𝑛2 + 𝑝 (2)

Also 𝐸2 − 𝑝2𝑐2 = 𝑚02𝑐4 (3)

𝐸1 − 𝐸2 + 𝑚0𝑐2 2 − 𝐸1 𝑛1 − 𝐸2 𝑛2

2 = 𝑚02𝑐4

𝐸12 − 2𝐸1𝐸2 + 𝐸2

2 + 2 𝐸1 − 𝐸2 𝑚0𝑐2 + 𝑚0

2𝑐4 − (𝐸12 − 2𝐸1𝐸2𝐶𝑜𝑠 𝜃 + 𝐸2

2) = 𝑚02𝑐4

2 𝐸1 − 𝐸2 𝑚0𝑐2 − 2𝐸1𝐸2 1 − 𝐶𝑜𝑠 𝜃 = 0

From (1) From(2)

Page 11: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

Compton Effect

2 𝐸1 − 𝐸2 𝑚0𝑐2 − 2𝐸1𝐸2 1 − 𝐶𝑜𝑠𝜃 = 0

𝑜𝑟

1

𝐸2−

1

𝐸1=

1

𝑚0𝑐2 (1 − 𝐶𝑜𝑠𝜃)

𝐵𝑢𝑡, 𝐸1 = ℎ𝑣1 =ℎ𝑐

𝜆1𝐸2 = ℎ𝑣2 =

ℎ𝑐

𝜆2

∴ 𝜆2 − 𝜆1 =ℎ

𝑚0𝑐(1 − 𝐶𝑜𝑠𝜃)

Page 12: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

Compton Effect

𝜆2 − 𝜆1 =ℎ

𝑚0𝑐(1 − 𝐶𝑜𝑠𝜃)

For 𝑒−, ℎ

𝑚0𝑐= 2.4 × 10−12𝑚 = 0.0024𝑛𝑚

Compton used 𝑥-rays with 𝜆1 = 0.07𝑛𝑚 (p.196 French)

Δ𝜆 ∝ (1 − 𝐶𝑜𝑠𝜃)

Use diffraction from crystal to measure 𝜆 of 𝑥-rays

Later, in 1950, Cross and Ramsey using 𝛾-rays of 2.6𝑀𝑒𝑉 also detected recoiling 𝑒.

• Angle between 𝑒 and scattered photon is correct

• Scattered photon and recoiling 𝑒 detected in coincidence

Page 13: Lecture 12: Collisions (scattering) · Lecture 11: Collisions (scattering) Stationary particle hit by identical particle in an elastic collision In Newtonian mechanics angle between

3-Dec-13 13

From Special Relativity by A. P. French