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Design Guide › Physics theory

Physics theory design rules

4 of the guide’s 1374 rules carry the physics-theory tag. Rules that are theoretical results rather than practice: stripping lifetimes, measurement accuracy floors, kinematic broadening, and detector efficiency models. Each rule keeps its formula where the source gives one, a verbatim quote, a page-level citation, and a stable identifier (dg-NNNN) that resolves here and on the all-in-one guide.

To combine this tag with another (rules carrying both), use the filterable view: /design-guide/?domain=physics-theory and add a second chip. Related domains, by how often they share a rule with this one: Beam measurement (2), Detectors (1), Extraction (1), Magnet (1).

Verify before use. Every rule here is a source extract in the vocabulary of the editorial methodology — faithful to its cited page, not an independently validated engineering requirement. Re-read any rule that drives a real design decision at the cited page before committing metal, money, or high voltage to it.

  1. Lorentz (magnetic) stripping of H- has rest-frame lifetime tau = (A1/E)*exp(A2/E) with A1=2.714e-6 s*V/m, A2=4.474e9 V/m, E=gamma*beta*c*B - negligible below a few MeV even at 4 T.

    tau = (A1/E)*exp(A2/E), E = gamma*beta*c*B

    extractionphysics-theorymagnet dg-600

    Source, quote & tabletop applicability
    a 4 T magnetic field for the maximum achievable energy of 8.5 MeV in the AMIT cyclotron corresponds to a beam-rest-frame electric field of E = 160 MV/m. This entails a marginal beam fraction loss per unit length of 1.42e-6 m-1

    Calvo et al., Beam Stripping Interactions in Compact Cyclotrons — PRAB 24, 090101 (2021) — p. 7-8, 14

    Tabletop: At 0.889 T and 500 keV the rest-frame field is ~9 MV/m, where the exponential makes the lifetime effectively infinite - Lorentz stripping can be ignored entirely for a next machine.

  2. Know the accuracy floor of any absorber-based energy measurement: range-energy data and straggling limit the most-probable-energy determination to a few hundred keV, the high-energy edge of the distribution is nearly as good, but the LOW-energy side of the spectrum is largely unrecoverable.

    beam-measurementphysics-theory dg-883

    Source, quote & tabletop applicability
    These factors limit the accuracy of determination of the most probable energy to a few hundred kilovolts. The high energy portion of the energy distribution can be determined with almost equivalent accuracy

    Cohen, Measurement of Beam Energy and Energy Distribution on an Internal Cyclotron Target — ORNL-1347 (1952) — p. 5

    Tabletop: Scale the absolute numbers down with energy, but keep the shape of the claim — quote the high-energy edge with confidence, treat the low-energy tail as semi-quantitative. Same asymmetry applies to a PIPS-plus-degrader spectrum on a next machine, and to interpreting any resonance-yield curve taken with a spread beam.

  3. Mounting a spectrograph with its dispersion plane horizontal costs kinematic broadening of peaks (from the in-plane angular acceptance) when scattering off light nuclei, but can buy large-angle reach - here rotation to 165 degrees, needed for back-angle cross sections and DWBA tests. Know which trade you are making.

    beam-measurementphysics-theory dg-987

    Source, quote & tabletop applicability
    In scattering from light nuclei, this introduces appreciable kinematic broadening of peaks as the entrance aperture is opened.

    Alford, Bilaniuk & Hawrylak, Broad Range Spectrograph for Use with the Rochester 27-inch Cyclotron — NYO-9683 (1961) — p. 8

    Tabletop: SCALE-HONEST - kinematic broadening scales with (m_projectile/m_target) and aperture, not beam energy, so the trade is identical for a next machine's Rutherford-scattering station. The fix they note (close the entrance aperture when it matters) is the standard resolution-vs-count-rate knob students should learn to turn.

  4. A simple single-scattering model predicts organic-scintillator neutron efficiency to satisfactory accuracy: eff = (1 - E0/En) * (1 - exp(-nH*sigma_np*l)), where the first factor (fraction of recoils above threshold) is exact and independent of the scintillator response shape so long as response is monotonic; find E0 per threshold setting from a D(d,n) check and take sigma_np from Gammel's semi-empirical formula (good to parts in 10^3 up to 42 MeV).

    eff = (1 - E0/En)(1 - exp(-n_H * sigma_np(En) * l)); assumptions - n-p single scattering only, effective length = geometric length, recoil range negligible

    detectorsphysics-theory dg-996

    Source, quote & tabletop applicability
    The first factor in (1) is exact. It does not depend on the exact shape of the response curve (pulse-height vs proton recoil energy) of the scintillator.

    Fulbright et al., A Fast Neutron Time of Flight System for Use with Cyclotrons — NYO-9360 (1962) — p. 15

    Tabletop: DIRECT for any neutron-counting next-machine experiment and a lovely teaching derivation - a two-factor closed form students can test against a calibration reaction. The identification of which factor is exact vs model-dependent is the transferable habit.