- We energize charged particles with electric fields: \( \Delta E_{\text{kin}} = q \int \mathbf{E}\cdot\mathrm{d}\mathbf{s} \).
- DC gaps are limited by breakdown; RF lets us reuse the same voltage many times — but only if the gap is short enough (transit time).
- Higher RF frequency ⇒ shorter drift tubes (\( \propto \lambda/2 \)) ⇒ more compact linacs — ultimately motivating optical/laser fields.
- Energetic ions matter far beyond therapy: volumetric heating, warm dense matter, planetary interiors, fusion, and particle physics.
1. How do we energize a charged particle?
In mechanics we speak of acceleration, but in accelerator physics the central quantity is the kinetic energy gain. For a charge \( q \) in an electric field, the work done along a path gives \( \Delta E_{\text{kin}} = q U \) across a potential difference \( U \) (also in the relativistic regime, where \( E_{\text{kin}} = mc^2(\gamma-1) \)).
Derivation: Newton's law, work, and the electron volt
Newton's second law for a charge in a field: \( \mathrm{d}\mathbf{v}/\mathrm{d}t = (q/m)\mathbf{E} \). The kinetic energy gain is \[ W = \Delta E_{\text{kin}} = \int_A^B \mathbf{F}\cdot\mathrm{d}\mathbf{s} = q \int_A^B \mathbf{E}\cdot\mathrm{d}\mathbf{s}. \] In a parallel-plate capacitor with gap \( d_{\text{gap}} \) and voltage \( U_0 \), a particle crossing the full gap gains \( \Delta E_{\text{kin}} = q U_0 \). One electron volt (1 eV) is the energy gained by an electron across 1 V.
2. Electrostatic acceleration — and its limits
A single large DC gap is the simplest accelerator: apply a high voltage, let the particle fall through the potential. Van de Graaff and tandem electrostatic machines still use this principle (up to ~10 MV in evacuated tanks). The hard limit is electrical breakdown: above a material-dependent field strength, sparks quench the gap.
Historical note: Van de Graaff and breakdown physics
Robert J. Van de Graaff developed the belt-charged electrostatic generator around 1930; machines reached MV-scale voltages within a few years and remain in use as precision low-energy ion sources.
Breakdown in gases involves avalanche ionization (Paschen-type behaviour); at surfaces, microscopic field emitters and defects initiate arcs. RF structures can often sustain higher gradients than DC gaps, with a weak scaling with of breakdown field strength with frequency.
3. RF in a single gap: transit time
AC voltages are easier to generate at high amplitude (transformers). But in a sinusoidal gap the field reverses every half period. For net acceleration the particle must leave the gap before the field flips: \( d_{\text{gap}} \lesssim v/(2 f_0) \). If the gap is too long at a given frequency, the particle merely oscillates — no sustained energy gain.
Transit-time estimate and Figure 1.2
Transit time \( t_{\text{cross}} \approx d_{\text{gap}}/v \). The RF reverses after \( T_0/2 = 1/(2 f_0) \). Requiring \( t_{\text{cross}} \lesssim T_0/2 \) gives \( d_{\text{gap}} \lesssim v/(2 f_0) \).
Even with RF, a single gap cannot reach arbitrary energy: breakdown and power handling still cap \( U_0 \). The way forward is to reuse the same RF source in many gaps in series.
4. Widerøe linac: many gaps and lengthening drift tubes
Rolf Widerøe (1928) placed drift tubes between gaps so particles travel in field-free regions while the RF phase prepares the next accelerating kick. Odd and even tubes alternate in polarity; each gap adds energy. As velocity grows, drift tubes must become longer (\( d_{\text{drift}} \approx v/(2 f_0) \), or odd multiples thereof).
Drift-tube phasing, Figure 1.3, and compactness
Inside a drift tube \( t_{\text{drift}} \approx d_{\text{drift}}/v \). For the next gap to be accelerating, \( t_{\text{drift}} \approx (2n+1)/(2 f_0) \), hence \( d_{\text{drift}} \approx (2n+1)\, v/(2 f_0) \). The shortest choice is \( d_{\text{drift}} \approx v/(2 f_0) \).
For ultra-relativistic particles \( d_{\text{drift}}^{\min} \approx c/(2 f_0) = \lambda/2 \). Compact linacs require higher frequency — shorter wavelength.
Cyclotron (related idea, not the main path here)
Ernest Lawrence's cyclotron (1932) reuses an RF gap on every half turn in a magnetic field instead of stacking drift tubes in a line. The same transit-time and synchronism ideas apply: the RF frequency must match the particle's revolution period (until relativistic dephasing sets in).
Explore the interactive cyclotron module in lecture02_cyclotron_simulator.html (also discussed in Lecture 2). For a pencil-and-paper version, see Exercise 1.
5. Why higher frequency — and why light?
Accelerator technology tracked the highest-power EM sources of each era. Each step shrinks \( \lambda/2 \) and enables higher gradients:
- Radio (1920s): kHz–MHz broadcasting; wavelengths metres to kilometres.
- Early accelerators (1930s): MV-scale DC (Van de Graaff, Cockcroft–Walton) and MHz RF (Widerøe, cyclotron).
- Microwaves (1940s–50s): klystrons and radar → GHz cavities for linacs and synchrotrons.
- Lasers (from 1960): optical cycles at µm scale; CPA systems (Nobel 2018) reach extreme peak powers — e.g. the ATLAS 3000 PW laser at CALA, LMU Munich.
This course asks: can petawatt laser fields replace or complement conventional structures for compact ion acceleration?
6. Why energetic ions? The Bragg curve and applications
Building compact accelerators is not an end in itself. MeV–GeV ions deposit energy in matter with a characteristic depth dose profile: a slow rise followed by a sharp Bragg peak near the end of range (Bethe–Bloch stopping). That localized deposition makes ions uniquely useful wherever energy must be delivered inside a target.
- Cancer therapy: proton and carbon-ion therapy exploit the Bragg peak to spare tissue beyond the tumour — the clinical spread-out Bragg curve (SOBP) is built from many peaks (Lecture 11).
- Volumetric heating: ion beams heat matter in depth, not just at the surface — relevant for warm dense matter (WDM) samples in the laboratory.
- Planetary and stellar interiors: WDM physics connects to equations of state in giant-planet cores and brown dwarfs.
- Nuclear physics: ion beams drive fission and fusion reactions, produce exotic nuclei, and explore nonlinear nuclear physics at high energy density — from reactor materials testing to rare-isotope production.
- Inertial fusion: fast ignition and related schemes use intense particle beams to heat compressed fuel regions; ion stopping sets where energy is deposited.
- Particle physics: ion beams probe structure functions, produce secondary beams, and stress-test detectors — the same stopping physics appears in calorimetry and beam dumps.
Laser-driven ion sources (TNSA, RPA, …) aim to deliver such beams from compact, high-repetition platforms — but first we need the language of fields, plasmas, and diagnostics developed in the following lectures.
Bethe–Bloch stopping (qualitative)
The mean excitation energy, material density, and charge state control
how \( \mathrm{d}E/\mathrm{d}x \) varies with ion energy. Near the
Bragg peak, straggling and nuclear scattering modify the detailed curve;
Exercise 7 (e07) provides background calculations used
later for spread-out Bragg curves (Exercise 10).