By Richard Talman
This primary e-book to hide in-depth the iteration of x-rays in particle accelerators makes a speciality of electron beams produced through the radical strength restoration Linac (ERL) know-how. The ensuing hugely superb x-rays are on the centre of this monograph, which keeps the place different books out there cease.
Written essentially for basic, excessive power and radiation physicists, the systematic therapy followed via the paintings makes it both appropriate as a sophisticated textbook for younger researchers.
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Extra resources for Accelerator X-Ray Sources
More explicitly this is dx/dn/n ( λ/2S) 1 dn n dx k. 6) This is known as an “adiabatic” condition. ) This approximation will permit dropping terms proportional to |dn/dx |. By matching exponents of Eq. 5) and Eq. 2) locally one can deﬁne a local wave vector kˆ such that φ(r) = n(r) kˆ (r) · r. 7) This amounts to best-approximating the wave function locally by the plane wave solution of Eq. 2). Because n and kˆ are no longer constant, Eq. 8) where inequality Eq. 6) has been used to show that the ﬁrst term is small compared to the second.
The general solution of this equation is k2 k2 z + b cos z, k k k2 k2 k2 cos z−b sin k k k F (z) = a sin F (z) = a k2 z. 42) Using the ﬁrst of Eqs. 41) to transform the dependent variable back from F to f yields f (z) = k2 k f 0 cos − f0 k2 k z+ sin k k2 k2 k sin z + cos k2 k k2 k z . 43) z For the evolution z0 → z1 this transformation is conventionally written as f1 = A10 f 0 + B10 . 44) The A, B, C, D coefﬁcients can be read off by evaluating, at z = z0 , the sines and cosines in the ratio given by Eq.
Substituting these expressions into Eq. 30) yields z y2 1 i . 35) +k − z0 2 z(1 + z20 /z2 ) z0 (1 + z2 /z20 ) √ Using the relation ln( a + ib) = ln a2 + b2 + i tan−1 (b/a) the ﬁrst term in the exponent becomes ψ = exp exp − ln − ln 1+i 1+i z z0 = 1 1 + (z/z0 exp )2 − i tan−1 z . 36) To cast Eq. 11, we deﬁne w20 = z0 , k w ( z ) = w0 1+ z2 , 2 k w40 and R( z) = z 1 + z20 . 37) Finally, by Eq. 28), the wave ﬁeld is given Ψ (y, z) = Ψ0 w0 z exp − i tan−1 w(z) z0 exp ikz + y2 2 1 ik . 38) This is rather complicated, but the magnitude of Ψ depends only on the real part of the exponent, which is −y2 /(2w2 (z)).