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PENELOPE 2003 - OECD Nuclear Energy Agency

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210 Appendix A. Collision kinematics<br />

is the total energy in units of the rest energy. From the relation (A.5), it follows that<br />

√<br />

E = (cp) 2 + m 2 c 4 − mc 2<br />

(A.9)<br />

and<br />

dp<br />

dE = 1 v = 1<br />

cβ .<br />

(A.10)<br />

For a photon (and any other particle with m = 0), the energy and momentum are<br />

related by<br />

E = cp.<br />

(A.11)<br />

A.1 Two-body reactions<br />

Consider a reaction in which a projectile “1” collides with a target “2” initially at rest in<br />

the laboratory frame of reference. We limit our study to the important case of two-body<br />

reactions in which the final products are two particles, “3” and “4”. The kinematics of<br />

such reactions is governed by energy and momentum conservation.<br />

We take the direction of movement of the projectile to be the z-axis, and set the<br />

x-axis in such a way that the reaction plane (i.e. the plane determined by the momenta<br />

of particles “1”, “3” and “4”) is the x-z plane. The energy-momentum 4-vectors of the<br />

projectile, the target and the reaction products are then (see fig. A.1)<br />

˜P 1 = (W 1 c −1 , 0, 0, p 1 )<br />

˜P 2 = (m 2 c, 0, 0, 0)<br />

˜P 3 = (W 3 c −1 , p 3 sin θ 3 , 0, p 3 cos θ 3 )<br />

˜P 4 = (W 4 c −1 , −p 4 sin θ 4 , 0, p 4 cos θ 4 )<br />

(A.12a)<br />

(A.12b)<br />

(A.12c)<br />

(A.12d)<br />

<strong>Energy</strong> and momentum conservation is expressed by the 4-vector equation<br />

˜P 1 + ˜P 2 = ˜P 3 + ˜P 4 .<br />

(A.13)<br />

From this equation, the angles of emergence of the final particles, θ 3 and θ 4 , are uniquely<br />

determined by their energies, W 3 and W 4 . Thus,<br />

m 2 4c 2 = ( ˜P ˜P 4 4 ) = ( ˜P 1 + ˜P 2 − ˜P 3 )( ˜P 1 + ˜P 2 − ˜P 3 )<br />

= ( ˜P ˜P 1 1 ) + ( ˜P ˜P 2 2 ) + ( ˜P ˜P 3 3 ) + 2( ˜P ˜P 1 2 ) − 2( ˜P ˜P 1 3 ) − 2( ˜P ˜P 2 3 )<br />

= m 2 1c 2 + m 2 2c 2 + m 2 3c 2 + 2W 1 W 2 c −2<br />

− 2 ( )<br />

W 1 W 3 c −2 − p 1 p 3 cos θ 3 − 2W2 W 3 c −2 ,<br />

(A.14)<br />

and it follows that<br />

cos θ 3 = m2 4 c4 − m 2 1 c4 − m 2 2 c4 − m 2 3 c4 + 2W 1 (W 3 − W 2 ) + 2W 2 W 3<br />

2 (W 2 1 − m 2 1c 4 ) 1/2 (W 2 3 − m 2 3c 4 ) 1/2 . (A.15)

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