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Vacuum Science for Optics — Abridged Guide

Quick-reference equations, tables, and rules of thumb for vacuum technology in photonics. For full derivations, worked examples, and diagrams, see the Comprehensive Guide.

1.Introduction

Vacuum quality is classified into ranges based on pressure — from low/rough vacuum (10⁵–10² Pa) used for initial pumping, to ultra-high vacuum (10⁻⁵–10⁻¹⁰ Pa) required for surface science and cold-atom experiments. The relevant physical transition is the mean free path exceeding the system dimensions, shifting gas behavior from fluid-like to independent molecular trajectories.
For a quick mental model: at high vacuum, molecules fly wall-to-wall without colliding with each other. At atmospheric pressure, they collide after ~68 nm.
RangePressure (Pa)Mean Free PathKey Optics Application
Low (rough)10⁵ – 10²nm – μmInitial pumpdown
Medium10² – 10⁻¹μm – mmSputtering
High (HV)10⁻¹ – 10⁻⁵mm – kmOptical coating, laser systems
Ultra-high (UHV)10⁻⁵ – 10⁻¹⁰km – 10⁷ kmCold atoms, surface science

Vacuum prevents contamination of optical surfaces, enables beam propagation at UV/EUV wavelengths, provides the environment for thin film deposition, and eliminates convection and acoustic coupling in precision experiments.

2.Pressure Units & Measurement

Conversion fundamentals
1 atm=760 Torr=1013 mbar=101,325 Pa1 \text{ atm} = 760 \text{ Torr} = 1013 \text{ mbar} = 101{,}325 \text{ Pa}
The SI unit is the pascal (Pa); Torr dominates North American practice; mbar is common in European practice. Remember: 1 Torr ≈ 4/3 mbar.
No single gauge spans the full vacuum range. Capacitance diaphragm gauges (gas-independent) are best for process control; Bayard-Alpert ionization gauges are the HV/UHV workhorse but require gas correction factors.
GaugeRange (Pa)Gas Independent?Best For
Capacitance diaphragm10⁻² – 10⁵YesProcess control
Pirani10⁵ – 10⁻¹NoRoughing
Bayard-Alpert10⁻¹ – 10⁻⁹NoHV/UHV
RGA< 10⁻²Species-resolvedDiagnostics

3.Kinetic Gas Theory

Mean free path (air, room temperature)
λair6.6×103p(m, p in Pa)\lambda_{\text{air}} \approx \frac{6.6 \times 10^{-3}}{p} \quad \text{(m, } p \text{ in Pa)}
Monolayer formation time (air, room temperature)
τML3.5×104p(s, p in Pa)\tau_{ML} \approx \frac{3.5 \times 10^{-4}}{p} \quad \text{(s, } p \text{ in Pa)}
The mean free path determines the flow regime and thus the entire approach to vacuum system design. The monolayer time tells you how long a clean surface stays clean — at 10⁻⁴ Pa it is ~3.5 seconds; at 10⁻⁸ Pa it is ~10 hours.
For quick estimates: at 10⁻⁴ Pa, the mean free path is ~66 m (well into molecular flow in any lab-sized system). At 1 Pa, the mean free path is ~6.6 mm — comparable to tubing dimensions, so you are in the transitional regime.

4.Gas Flow Regimes

Knudsen number
Kn=λD\text{Kn} = \frac{\lambda}{D}
Kn > 0.5 = molecular flow; Kn < 0.01 = viscous flow
Molecular flow tube conductance (air, 20°C)
Ctube12.1D3L(L/s, D,L in cm)C_{\text{tube}} \approx 12.1 \frac{D^3}{L} \quad \text{(L/s, } D,L \text{ in cm)}
In molecular flow, conductance depends on D³/L — doubling the pipe diameter gives 8× the conductance. This is the most important design rule in vacuum plumbing.
Series conductances add reciprocally (like parallel resistors). The lowest-conductance element dominates. Always check that your plumbing conductance is not the bottleneck before buying a bigger pump.

5.Vacuum Pumps

No single pump covers the full vacuum range. Rough pumping (atmosphere to ~1 Pa) uses positive displacement pumps; high vacuum uses turbomolecular or diffusion pumps; UHV uses ion pumps and getters. A typical optical system uses a scroll pump backing a turbo pump.
PumpRange (Pa)Oil-Free?Best For
Scroll10⁵ – 1YesClean backing
Turbo10⁻¹ – 10⁻⁸YesGeneral HV/UHV
Cryopump10⁻¹ – 10⁻⁸YesWater pumping, coatings
Ion pump10⁻⁴ – 10⁻⁹YesVibration-free UHV
Diffusion10⁻¹ – 10⁻⁷NoLarge industrial systems
For precision optics, avoid oil-sealed pumps entirely. A dry scroll pump + turbomolecular pump combination gives clean vacuum to 10⁻⁶ Pa without hydrocarbon contamination.

6.Outgassing & Gas Loads

In a leak-free system, the ultimate pressure is determined by outgassing — the release of adsorbed water (initially dominant) and dissolved hydrogen (long-term limit) from chamber walls. Baking at 150°C for 24 hours reduces water outgassing by 100–1000×.
ASTM E595 qualification (TML < 1.0%, CVCM < 0.10%) is the gold standard for selecting materials that will not contaminate your vacuum system. Check NASA's outgassing database before using any adhesive, paint, or polymer in vacuum.
MaterialUnbaked q (Pa·m/s)Baked q (Pa·m/s)Limit Species
304/316L SS~10⁻⁶~10⁻⁸H₂O → H₂
Aluminum 6061~10⁻⁶~10⁻⁸H₂O → H₂
Viton O-ring~10⁻⁵~10⁻⁶H₂O, organics
OFHC copper~10⁻⁷~10⁻⁹H₂

7.Vacuum System Design

Effective pumping speed
1Seff=1Sp+1C\frac{1}{S_{\text{eff}}} = \frac{1}{S_p} + \frac{1}{C}
Ultimate base pressure
pbase=qASeffp_{\text{base}} = \frac{q \cdot A}{S_{\text{eff}}}
The effective pumping speed at the chamber is always less than the pump rating because connecting tubes reduce gas flow. Always calculate S_eff before selecting a pump.
CF flanges with copper gaskets are the universal choice for UHV (bakeable to 450°C, leak rate <10⁻¹² Pa·m³/s). KF flanges with Viton O-rings are fine for HV (limited to ~10⁻⁵ Pa).

8.Vacuum-Compatible Optics

Standard optomechanics fail in vacuum due to trapped volumes, outgassing materials, and lack of thermal management. Use only vacuum-rated components with vented screw holes, no zinc/cadmium plating, no standard grease, and no anodized surfaces (UHV).
Fused silica is the default viewport material for UV/Vis/NIR. For VUV (< 200 nm), use MgF₂ or CaF₂. All viewports should have AR coatings rated for the bakeout temperature.
Wavelength RangeWindow MaterialNotes
VUV (< 200 nm)MgF₂, CaF₂Crystalline; seal with indium
UV–NIR (200 nm – 2.5 μm)Fused silicaStandard; brazed CF viewports
Mid-IR (2–12 μm)ZnSe, CaF₂, BaF₂ZnSe for CO₂ lasers
Far-IR/THzDiamond, Si, GeSpecialty applications

9.Optical Applications

Vacuum is required for PVD coating (mean free path > source-to-substrate distance), VUV/EUV beam propagation (atmospheric absorption), high-power laser damage prevention (hydrocarbon elimination), and quantum optics experiments (minimizing background gas collisions for trap lifetime).
For optical coatings, base pressure before deposition is more important than process pressure. A base pressure 100× lower than the process pressure ensures negligible contamination incorporation into the film.

10.System Selection Workflow

System design starts with the target pressure — it determines everything downstream: pump type, materials, seals, and cost. Calculate S_eff = Q_total / p_target to size the pump, then verify that plumbing conductance does not dominate.
The three most common design errors are: (1) trapped volumes (virtual leaks from unvented screw holes), (2) conductance-limited plumbing (undersized tubes negate a large pump), and (3) skipping bakeout after air exposure.
Continue Learning

The Comprehensive Guide includes worked examples, SVG diagrams, and 8 references.

All information, equations, and calculations have been compiled and verified to the best of our ability. For mission-critical applications, we recommend independent verification of all values. If you find an error, please let us know.