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Vacuum I G. Franchetti CAS - Bilbao 30/5/2011 G. Franchetti 1

Vacuum I

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Vacuum I. G. Franchetti CAS - Bilbao. Index. Introduction to Vacuum. Vacuum and the Beam. Flow Regimes. Creating Vacuum. Vacuum in accelerators. All beam dynamics has the purpose of controlling a charged beam particle. - PowerPoint PPT Presentation

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Page 1: Vacuum I

G. Franchetti 1

Vacuum I

G. FranchettiCAS - Bilbao

30/5/2011

Page 2: Vacuum I

G. Franchetti 2

Index

30/5/2011

Introduction to Vacuum

Vacuum and the Beam

Creating Vacuum

Flow Regimes

Page 3: Vacuum I

G. Franchetti 3

Vacuum in accelerators

30/5/2011

All beam dynamics has the purpose of controlling a charged beam particle

Structure of magnets and RF structure have the purpose of creating a properguiding (E,B) structure

However in an accelerator are present a jungle of unwanted particles which creates a damaging background for beam operation

Page 4: Vacuum I

G. Franchetti 4

Characteristic of Vacuum

30/5/2011

Vacuum is considered as a Gas which is characterized by

Pressure

Temperature

Density

Composition

Minimize the interaction of beam with vacuum gasAim:

Macroscopic Quantities

Kinetic Theory

Microscopic Quantities

Page 5: Vacuum I

G. Franchetti 530/5/2011

Particles m-3

Atmosphere 2.5 x 1025

Vacuum Cleaner 2 x 1025

Freeze dryer 1022

Light bulb 1020

Thermos flask 1019

TV Tube 1014

Low earth orbit (300km) 1014

H2 in LHC ~1014

SRS/Diamond 1013

Surface of Moon 1011

Interstellar space 105

Typical numbers

R.J. Reid

Page 6: Vacuum I

G. Franchetti 6

Particle – Wall collision

30/5/2011

m

v1v2

Momentum is propagated to the wall

The velocity after wall collision depends on the particle-wall interaction

interaction

Page 7: Vacuum I

G. Franchetti 7

Pressure

30/5/2011

m

SI Units:

other units:

Low vacuum Atm. pressure to 1 mbar

Medium vacuum 1 to 10-3 mbar

High Vacuum (HV) 10-3 to 10-8 mbar

Ultrahigh vacuum (UHV)

10-8 to 10-12 mbar

Extreme high vacuum (XHV)

less than 10-12 mbar

Page 8: Vacuum I

G. Franchetti 8

Particle – Particle interaction

30/5/2011

mv1

m

v2

Interaction

mv1’

mv2’

In a gas large number of collisions

Most likely process P-P collision

For elastic collisions: 1) Energy conservation2) Momentum conservation

Temperature

Page 9: Vacuum I

G. Franchetti 9

Typical numbers

30/5/2011

Air at T= 20o C 20% O2 MO = 8x2 g-mole = 8x2/NA = 2.65 x 10-23 g80% N2 MN = 7x2 g-mole = 7x2/NA = 2.32 x 10-23 g

Therefore

Molecules run fast !

But the average velocity is

Page 10: Vacuum I

G. Franchetti 10

Velocity Distribution

30/5/2011

When a gas is at equilibrium the distribution of the velocity follows the Maxwell-Boltzmann distribution

max velocity

ave. velocity

Page 11: Vacuum I

G. Franchetti 11

Equation of state

30/5/2011

An ideal gas in a container of volume V satisfies the equation of state

SI units

P Pressure [Pa]V Volume in [m3]n moles [1]T absolute temperature [K]R0 = 8.314 [Nm/(mole K)] universal constant of gaskB = 1.38x10-23 [JK-1] Boltzmann constantNA = 6.022x1023 [1] Avogadro’s Number

For a gas in equilibrium

Page 12: Vacuum I

G. Franchetti 12

Mean free path

30/5/2011

Vacuum GasBeam

free path = path of a particle between two collisions

Page 13: Vacuum I

G. Franchetti 13

Mean free path

30/5/2011

Effective area covered by the rest atoms

N(l) = particle at l

# particles at l + Δl that did not collide

v

Particles that did not collide

vDensity of atomsCross-section

Transverse area

A

Page 14: Vacuum I

G. Franchetti 14

Mean free path

30/5/2011

Therefore dN particles travelled a distance l and then collided

Probability that a particle travel l and then collide is

Mean free path

In a gas

How many particles collide between and ?

Page 15: Vacuum I

G. Franchetti 15

Example

30/5/2011

Air at T = 200 C and P = 1 atm

From equation of state

atom/m3

Diameter of molecule of air

Mean free path

Page 16: Vacuum I

G. Franchetti 1630/5/2011

N2 at T = 200 C, d = 3.15 10-10 m

Page 17: Vacuum I

G. Franchetti 17

Vacuum and Beam

30/5/2011

Vacuum Gas

Beam

Page 18: Vacuum I

G. Franchetti 18

Beam lifetime

30/5/2011

Beam of particles going through a vacuum gas survives according to

As beam particle have a velocity v0, then

From the equation of state

Beam lifetime

After a beam particle collides with a gas atom, it gets ionized and lost because of the wrong charge state with respect to the machine’s optics

Beam lifetime sets the vacuum constrain

Page 19: Vacuum I

G. Franchetti 19

Example

30/5/2011

Of what is formed the vacuum ?Does it depends on the energy ?

Example LHC

H2 at 7 TeV at T = 50 K

for

It is important to know the cross-section of the interaction beam-vacuum

Nuclear scattering cross section at 7 TeV for different gases and the corresponding densities and equivalent pressures for a 100 hours beam lifetime

LHC Design Report

Page 20: Vacuum I

G. Franchetti 2030/5/2011

O. Gröbner, CAS 2007

Page 21: Vacuum I

G. Franchetti 21

Impingement rate

30/5/2011

For a Maxwell-Boltzmann distributionWall or surface

J units: [#/( s m2)]

and

Page 22: Vacuum I

G. Franchetti 22

More on collision

30/5/2011

mean free pathmean free path

Page 23: Vacuum I

G. Franchetti 23

Knudsen Number

30/5/2011

Particles collide mainly among them the fluid is continuous

Continuous Regime

particles collide mainlywith walls

Molecular Regime

SI units: [1]

Flow Regimes

Transitional RegimeThis is a regime in between continuous and molecular

Page 24: Vacuum I

G. Franchetti 24

The Throughput

30/5/2011

The quantity is proportional to the number of particles

Vessel with a gas at

Number of particles

is called throughput SI units: [Pa m3/s]

Page 25: Vacuum I

G. Franchetti 25

Conductance

30/5/2011

In absence of adsorption and desorption processes the throughput does not change

1 2

equal

Conductance SI units: [m3/s]

T = constant

Page 26: Vacuum I

G. Franchetti 26

Composition (Series)

30/5/2011

C1 C2

Pu1 Pd1=Pu2 Pd2

equal throughput

Conductance of 1+2

T = constant

Page 27: Vacuum I

G. Franchetti 27

Composition (Parallel)

30/5/2011

C1

C2

Pu Pd

Conductance of 1+2

Vessel 1 Vessel 2

T = constant

Page 28: Vacuum I

G. Franchetti 28

Molecular Flow

30/5/2011

Regime dominated by Particle – Wall interaction

m

v1v2

Classical Mechanics m

v1

v2

Molecular regime

??

?

Kn > 0.5P < 1.3 x 10-3 mbarD = 0.1 m

Page 29: Vacuum I

G. Franchetti 29

Cosine-Law

30/5/2011

1. A particle after a collision with wall will loose the memory of the initial direction2. After a collision a particle has the same velocity |v| 3. The probability that particles emerge in a certain direction follow the cosine law

surface

= solid angle

Page 30: Vacuum I

G. Franchetti 30

Consequences

30/5/2011

A gas particle can return back!

Concept of Transmission probability

In the molecular regime two fluxes in opposite direction coexist

particle flux = N1 = particle per second through 1N2 = particle per second through 2

1 2

Page 31: Vacuum I

G. Franchetti 31

Conductance of an Aperture

30/5/2011

Downstream

Upstream

Gas current Volumetric flow

Throughput Conductance

Page 32: Vacuum I

G. Franchetti 32

Conductance of a long tube

30/5/2011

long tube = no end effect

stationary stated

This result is valid for L longL 0 make α ∞ which is wrong: The dependence of 1/L is consistent with the

rule of composition of conductance

Page 33: Vacuum I

G. Franchetti 33

Continuum flow regime

30/5/2011

Roughly more than 100 collision among particles before wall collision

Local perturbation of propagate through a continuum medium

Collision among particles create the Viscosity

Collision with walls cancel the velocity

zero velocity at the walls

Max. velocity

Kn < 0.01P > 6.5 x 10-2 mbarV = 0.1 m

Page 34: Vacuum I

G. Franchetti 34

Viscous/Laminar regime

30/5/2011

Reynold Number

ρ = density of gas [Kg/m3]v = average velocity [m/s]Dh= hydraulic diameter [m]

A = cross sectional areaB = perimeter

η = fluid viscosity [Pa-s]

Turbulent Regime

Laminar Regime

M. Lesiuer, Turbulence in Fluids, 4th Edition, Ed. Springer

Page 35: Vacuum I

G. Franchetti 35

Reynold Number as function of Throughput

30/5/2011

For air (N2) at T=20C η = 1.75 x 10-5 Pa-s with

Therefore the transition to a turbulent flow takes place at the throughput of

[mbar l /s] [mm]

For a pipe of d = 25 mm

At P = 1 atm this threshold corresponds to v = 0.389 m/s

Page 36: Vacuum I

G. Franchetti 36

Laminar Regime

30/5/2011

1. Fluid is incompressible: true also for gas when Ma < 0.22. Fluid is fully developed3. Motion is laminar Re < 20004. Velocity at Walls is zero

Fully developed flow

entry length

velocity distribution at injection in the pipe

velocity distribution of a fully developed flow

Page 37: Vacuum I

G. Franchetti 37

Conductance in Laminar Regime

30/5/2011

long tube = no end effect

D Pu Pd

L

Conductance: where

The conductance now depends on the pressure!

Page 38: Vacuum I

G. Franchetti 38

Conductance in Turbulent Regime

30/5/2011

The throughput becomes a complicated relation (derived from the Darcy-Weisbach formula)

long tube = no end effect

D Pu Pd

L

Darcy friction factor, dependent from the Reynold number

Page 39: Vacuum I

G. Franchetti 39

Sources of vacuum degradation

30/5/2011

Page 40: Vacuum I

G. Franchetti 40

Evaporation/Condensation

30/5/2011

evaporation

condensation

At equilibrium

PE = saturate vapor pressure

Example: water vapor pressure

Page 41: Vacuum I

G. Franchetti 41

Outgassing

30/5/2011

The outgassing is the passage of gas from the wall of the Vessel or Pipe to the vacuum

Mean stay time

P. Chiggiato, CAS 2007

Θ = fraction of sites occupied

“Throughput” due to outgassing

Ns = A x 3x1015 A = surface in cm2

Ed [Kcal/mole] Cases τd [s]

0.1 Helium 1.18 x 10-13

1.5 H2 physisorption 1.3 x 10-12

3-4 Ar,CO,N2,CO2 physisorption 1.6 x 10-11

10-15 Weak chemisorption 2.6 x 10-6

20 H2 chemisorption 66

25 3.3 x 105 (~half week)

30 CO/Ni chemisorption 1.6 x 109 (~50 years)

40 4.3 x 1016 (~half age of earth)

150 O.W chemisorption 1.35 x 1098 (larger than the age of universe)

Page 42: Vacuum I

G. Franchetti 42

Leaks

30/5/2011

High vacuum system

QL < 10-6 mbar l /sQL < 10-5 mbar l /sQL < 10-4 mbar l /s

very tighttightleaks

Diameter hole

0.01 mm

10-10 m

10-2

10-12

mbar-l/s

mbar-l/s

Leaks rate

Small Channels

K. Zapfe, CAS 2007 317 years for leakageof 1 cm3

Page 43: Vacuum I

G. Franchetti 43

Pumps and Gas flow

30/5/2011

Ideal Pump

particles that enterin this chamber never returns back !!

Pumping speed S0 [m3/s]

but

Example

N2 at T=20C

Take D=0.1m

S0 = 0.92 m3/s

S0 is Here

Page 44: Vacuum I

G. Franchetti 44

Pumps and Conductance

30/5/2011

Pumping speed S [m3/s] Pumping speed of ideal pump S0

conductance C

As the throughput is preserved Example: if the pipe is long l=100d

m3/s

d

Page 45: Vacuum I

G. Franchetti 45

Pumping Process -- Pump-down Time -- Ultimate Pressure

30/5/2011

Pump

hole

throughput due to evaporation

throughput due to outgassing

throughput due to leaks

effective throughput

Page 46: Vacuum I

G. Franchetti 46

Pumping Process -- Pump-down Time -- Ultimate Pressure

30/5/2011

Therefore

t [s]

P/P0

Ultimate pressure equilibrium between sources of throughput and pumps throughput1

Pump down time

Page 47: Vacuum I

G. Franchetti 47

Multistage pumps

30/5/2011

t [s]

P/P0

1

First stage pump down Second stage

Page 48: Vacuum I

G. Franchetti 4830/5/2011

Creating the Vacuum: Pumps

J.Y. Tang ICA01, TUAP062

LHC 10-10 – 10-11 mbar

FAIR HEBT 10-9 mbar

SIS100 10-12 mbar

(LHC Design Report)

A. Kraemer EPAC2006, TUPCH175

Examples of vacuum in some accelerators

Page 49: Vacuum I

G. Franchetti 49

Positive Displacement Pumps

30/5/2011

Principle: A volume of gas is displaced out of the Vessel

OutVessel

volume V

Pin

Pout

A compression of the volume V is always necessary to bring the pressure from Pin to a value larger then Pout

Piston Pumps

Rotary Pumps

Liquid ring pumps

Dry vacuum pump

Page 50: Vacuum I

G. Franchetti 50

Piston Pumps

30/5/2011

Vessel

Pi Po

Po

Vmin Minimum volume

Page 51: Vacuum I

G. Franchetti 51

Piston Pumps

30/5/2011

Vessel

Pi Po

P’

Here the pressure P’is smaller than Po but larger than Pi

Page 52: Vacuum I

G. Franchetti 52

Piston Pumps

30/5/2011

Vessel

PiPo

At this point the internal pressure becomes equal to Pi

Pi

Pi Vi = P0 Vmin

Page 53: Vacuum I

G. Franchetti 53

Piston Pumps

30/5/2011

Vessel

Pi Po

The internal pressure remains Pi but the volume increase to Vmax

Effective gas volume entered into the pump equal to Vmax – Vi : this is the gas which will be expelled

Page 54: Vacuum I

G. Franchetti 54

Piston Pumps

30/5/2011

Vessel

Pi Po

At the Volume Vc the internal pressure becomes equal to Po and the valve opens.

Po

Po Vc = Pi Vmax

and from now on the gas entered into the pump goes out

Page 55: Vacuum I

G. Franchetti 55

Piston Pumps

30/5/2011

Therefore if the pumps make Nc cycles per second

Conclusion: the pumping speed depends on the ratio of outlet/inlet pressure

When the inlet pressure is too low the pump stops pumping

S

PoPlimit

S0

Page 56: Vacuum I

G. Franchetti 5630/5/2011

If the gas compression/expansion is isentropic then all transformation follow the law

hence

Clearly the dependence affects the ultimate pressure even in absence of sources of throughput

Ultimate pressure

Page 57: Vacuum I

G. Franchetti 57

General Pump

30/5/2011

Pumping speed of ideal pump S0

OutletInlet

Pump throughputBackflow

Pi P0

But in real pumps there is a backflow

Pump

Page 58: Vacuum I

G. Franchetti 58

Zero Load Compression Rate

30/5/2011

Zero Load compression rate

The backflow is foundBackflow

Closed

Inlet

Pi0

Outlet

P0

Page 59: Vacuum I

G. Franchetti 59

Rotary Pumps

30/5/2011

Gas displaced in the moving vane

S = 1-1500 m3/hPl = 5 x 10-2 mbar (1stage)Pl = 10-3 mbar (2stage)

Gas Ballast

During the compression there can be gas component (G), which partial pressure PG can be too high condensation

But the maximum pressure during compression do not exceed P0 therefore by injectionng non condensable gas during the compression rate PG is lowered blowthe condensation point

Page 60: Vacuum I

G. Franchetti 60

Liquid Ring Pumps

30/5/2011

S = 1 – 27000 m3/hP = 1000 mbar 33 mbar

The gas enter in the cavity which expand. When the pressure in the cavity reaches the sature vapor pressure Ps the water boils.

During the compression the vapor bubbles implode creating the CAVITATION

At T = 150 C Ps = 33 mbarwhich sets the Plimit=Ps

Page 61: Vacuum I

G. Franchetti 61

Dry Vacuum Pumps: Roots

30/5/2011

pumping speed:75 – 30000 m3/h

operating pressure: 10 – 10-3mbar

Page 62: Vacuum I

G. Franchetti 62

Kinetic Vacuum Pumps

30/5/2011

Molecular drag pump

Turbo molecular Pump

Diffusion Ejector pump

Principle

The pump gives a momentum to the gas particles so that they flows out from the outlet

Page 63: Vacuum I

G. Franchetti 63

Molecular Drag Pumps

30/5/2011

Based on the molecular drag effectm

U

Page 64: Vacuum I

G. Franchetti 6430/5/2011

U

h

w

Volumetric flow:

Taking into account of the backflow

K0 = zero load compression rate,

Page 65: Vacuum I

G. Franchetti 6530/5/2011

U

Pi Po

The zero load compression rate is

But for a long tube if U ~ va

Example L = 250 mm, h = 3 mm S0/C > 10 and K0 >> 1

A. Chambers, Modern Vacuum Physics, CRC, 2005

Page 66: Vacuum I

G. Franchetti 66

Example of Molecular drag pump

30/5/2011

pumping speed:7- 300 l/s

operating pressure: 10-3 – 103 Pa

ultimate pressure10-5 to 10-3 Pa

Page 67: Vacuum I

G. Franchetti 6730/5/2011

Principle

UGeneral particle velocity distribution

va

U

tilted blades

φ

Turbo-molecular pump

Page 68: Vacuum I

G. Franchetti 68

Turbo-molecular pump

30/5/2011

In the reference frame of the rotating bladesU

General particle velocity distribution

tilted blades

φ

va - U

Page 69: Vacuum I

G. Franchetti 69

Turbo-molecular pump

30/5/2011

In the reference frame of the rotating bladesU

General particle velocity distribution

va - U

Page 70: Vacuum I

G. Franchetti 70

Turbo-molecular pump

30/5/2011

Returning in the laboratory frame

The vacuum particle has received a momentum that pushes it down

U

U

but the component of velocity tangential becomes too large

Page 71: Vacuum I

G. Franchetti 71

Multistage

30/5/2011

U U

The rotational component is lost and another stage can be placed

U U

rotor

stator

rotor

stator

Page 72: Vacuum I

G. Franchetti 72

Turbo-molecular pump

30/5/2011

Probability of pumping

The maximum probability Wmax is found when Pi = Po

And we also find that

K0 = compression rate at zero load

Page 73: Vacuum I

G. Franchetti 7330/5/2011

The compression rate at zero load

Therefore therefore different species have different pumping probability

In addition the maximum pumping probability Wmax is

Therefore we find that the maximum pumping speed is independent on the gas mass

Page 74: Vacuum I

G. Franchetti 7430/5/2011(Blazers Pfeiffer)

(Blazers Pfeiffer)

Maximum compression as function of foreline pressure

Pumping speed as function of the inlet pressure

pumping speed:35- 25000 l/s

ultimate pressure10-8 to 10-7 Pa

Page 75: Vacuum I

G. Franchetti 75

End of Vacuum I

30/5/2011