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Study of vacuum stability at cryogenic temperature Study of vacuum stability at cryogenic temperature

Study of vacuum stability at cryogenic temperature - PowerPoint Presentation

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Study of vacuum stability at cryogenic temperature - PPT Presentation

WP4 Activity at LNF Marco Angelucci Roberto Cimino CERN 09102017 Beam Screen Temperature CERN 100917 Marco Angelucci 1 LHC SR Power 013 Wm FCC SR Power 40 Wm Working Pressure ID: 781457

cern sey 17marco energy sey cern energy 17marco desorption argon angelucci sample clean treated electron laser electrons marco adsorption

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Slide1

Study of vacuum stability at cryogenic temperature

WP4 - Activity at LNF

Marco Angelucci

Roberto Cimino

CERN 09/10/2017

Slide2

Beam Screen Temperature

CERN 10/09/17

Marco Angelucci1LHCSR Power = 0.13 W/m

FCCSR Power = 40 W/mWorking Pressure(<10-11)BS Temperature Range

Slide3

Temperature

Find right working temperature is a fundamental point for vacuum stability.

Work near a gas desorption temperature could generate great pressure oscillations.CERN 10/09/17Marco Angelucci2

Study of adsorption/desorption behaviour near critical temperature is mandatory to understand vacuum stability

Study the behaviour of different surfaces

(treated sample)

Slide4

Vacuum Stability

CERN 10/09/17

Marco Angelucci3Interaction With PhotonsInteraction With ElectronsDesorptionSecondary Electron EmissionPhotoelectron Emission

Electron CloudHeat Load

Interaction With Ions

Slide5

LNF-Lab Now

CERN 10/09/17Marco Angelucci

4Two Different Ultra-High Vacuum Systems equipped with:

Low Energy Electron DiffractionSecondary Electron Yield SpectroscopySurface PreparationGas-Line

X-Ray/UV Photoemission

High Temperature Manipulator

Low Temperature Manipulator (

≈ 9 K)

Raman Spectroscopy

Scanning Tunneling Microscopy

New

Mass

Spectrometer

Slide6

LNF-Lab Now

CERN 10/09/17

Marco Angelucci5Two Different Ultra-High Vacuum Systems equipped with:

Low Energy Electron DiffractionSecondary Electron Yield SpectroscopySurface PreparationGas-Line

X-Ray/UV Photoemission

High Temperature Manipulator

Low Temperature Manipulator (

≈ 9 K)

Raman Spectroscopy

Scanning Tunneling Microscopy

New

Mass

Spectrometer

Synchrotron beamlines (30-1000 eV)

Slide7

Important

Results

CERN 10/09/17Marco Angelucci6

Follow Adsorption process checking the High-Energy SEY (HE-SEY)Distinguish Single Layer (SL) from Thick Film (TF) formation by Low-Energy SEY (LE-SEY) Quantify the number of adsorbed layers on surfaceMeasure the desorption temperature of TF and SL with SEY and TPDMeasure Work Function (WF) variation

Slide8

Important Tasks

CERN 10/09/17

Marco Angelucci7

Distinguish electron-induced from thermal desorption Study the contribution of reflected e- to Low-Energy SEYStudy the influence of the adsorbed gas in the Low-Energy SEY

Slide9

Important Tasks

Study the adsorption and desorption processes on Laser treated samples

(preliminary results)TPD measurements with new mass spectrometer (done)Measure desorption with SEY and TPD at the same time (data acquisition system improved)CERN 10/09/17Marco Angelucci8

Slide10

LNF-Lab Activities

SEY of Clean metals

SEY of clean Cu with low contaminantsAdsorption and Desorption processes from different surfaces (clean Cu, Laser Treated sample)Interaction between electron and ArgonContribution of reflected Electrons to the Low-Energy SEY (Graphite, Cu, Cu with Argon)CERN 10/09/17Marco Angelucci9

Slide11

LNF-Lab Activities

SEY of Clean metals

SEY of clean Cu with low contaminantsAdsorption and Desorption processes from different surfaces (clean Cu, Laser Treated sample)Interaction between electron and ArgonContribution of reflected Electrons to the Low-Energy SEY (Graphite, Cu, Cu with Argon)CERN 10/09/17Marco Angelucci10

Slide12

Clean Metals

CERN 10/09/17Marco Angelucci

11Differences between “As Received” and Atomically Clean MetalsHigh-Energy SEY dependenceContaminants (as received)Materials (clean)General High SEY

Lower SEYCharacteristic CurvesL. A. Gonzalez et al: "The secondary electron yield of noble metal surfaces.” In print to AIP Advances

Slide13

Clean Metals

CERN 10/09/17Marco Angelucci

12Differences between “As Received” and Atomically Clean Metalsin the Low-Energy rangeEvaluation of Work FunctionGeneral Behaviour in all clean metals

L. A. Gonzalez et al: "The secondary electron yield of noble metal surfaces.” In print to AIP Advances

Slide14

LNF-Lab Activities

SEY of Clean metals

SEY of clean Cu with low contaminantsAdsorption and Desorption processes from different surfaces (clean Cu, Laser Treated sample)Interaction between electron and ArgonContribution of reflected Electrons to the Low-Energy SEY (Graphite, Cu, Cu with Argon)CERN 10/09/17Marco Angelucci13

Slide15

Surface Modification

CERN 10/09/17Marco Angelucci

14Sub-Monolayer ContaminationsStrong Variations(SEY @10eV from 0.05 to 0.25)New characteristic structuresLow-Energy RangeLow Variations

(SEY Max from 1.4 to 1.3)Variation Dependence on Gas contaminant (?)High-Energy RangeInduced SEY variation by external contaminants L. A. Gonzalez et al: "The secondary electron yield of noble metal surfaces.” In print to AIP Advances

Slide16

Surface Modification

CERN 10/09/17Marco Angelucci

15Induced SEY variation by external contaminants Sub-Monolayer ContaminationsHigh-Energy RangeStrong Variations

(SEY @10eV from 0.05 to 0.25)New characteristic structuresLow-Energy RangeLow Variations (SEY Max from 1.4 to 1.3)Variation Dependence on Gas contaminant (?)L. A. Gonzalez et al: "The secondary electron yield of noble metal surfaces.” In print to AIP Advances

Slide17

LNF-Lab Activities

SEY of Clean metals

SEY of clean Cu with low contaminantsAdsorption and Desorption processes from different surfaces (clean Cu, Laser Treated sample) with ArgonInteraction between electron and ArgonContribution of reflected Electrons to the Low-Energy SEY (Graphite, Cu, Cu with Argon)CERN 10/09/17Marco Angelucci16

Slide18

Argon Adsorption (SEY)

CERN 10/09/17Marco Angelucci

17Two different regionswith characteristic trends Low Energy(<50 eV)Thick Film (TF)

High Energy(>50 eV)Single Layer (SL)Adsorption process of Argon on Cu sample at 10 KGeneral behaviourMax dose160 LCu

Cu

Max dose

160 L

Δ

= 4.1

From 1.4 (10 K) to 5.5 (160 L)

(@900 eV)

Slide19

Argon Desorption (SEY)

CERN 10/09/17Marco Angelucci

18AdsorptionDesorptionTFSL

Slide20

Argon Desorption (TPD)

CERN 10/09/17Marco Angelucci

19Temperature Programmed Desorption (TPD) Characteristic desorption behaviourFirst desorption process around 20 K (P1)Second desorption process @ 30 K (P2)Other desorption after 50 KP1P2

Slide21

Argon Desorption (TPD)

CERN 10/09/17Marco Angelucci

20Temperature Programmed Desorption (TPD) P1P2P1Correlation between P1 and SEY signals

Slide22

Argon Results (Cu)

Berlin 30/05/17

Marco Angelucci21System returns to the original state with slight differences Possibility to follow formation of SL from TFPossibility to measure desorption temperature with SEY and TPDDesorption Process (Heating)

Formation of a Thick Film (TF) at high coverage (increasing of SEY)

Formation of a Single Layer (SL) on Cu at LT (characteristic peaks)

Adsorption Process (LT)

Slide23

LNF-Lab Activities

SEY of Clean metals

SEY of clean Cu with low contaminantsAdsorption and Desorption processes from different surfaces (clean Cu, Laser Treated sample) with ArgonInteraction between electron and ArgonContribution of reflected Electrons to the Low-Energy SEY (Graphite, Cu, Cu with Argon)CERN 10/09/17Marco Angelucci22

Slide24

Laser Treated Sample

CERN 10/09/17

Marco Angelucci23

Laser treated sample at 10 K

Strong Variation of SEY due to

the contamination

Slide25

Laser Treated Sample

CERN 10/09/17

Marco Angelucci24

Laser treated sample Heated up to 300 K

Desorption

of contaminants

SEY returns to the initial value

Slide26

Laser Treated Sample

CERN 10/09/17Marco Angelucci

25

Adsorption of contaminantsCooling Process

Modification of SEY

Additional contribution to Thermal Desorption

Slide27

Laser Treated Sample

CERN 10/09/17

Marco Angelucci26Adsorption process of Argon (500 L) on Laser Treated sample at 10 KNo “significant” variation of SEYΔ = 0.05From 0.55 (10 K) to 0.6 (500 L)

(@900 eV)

Slide28

Laser Treated Sample

CERN 10/09/17

Marco Angelucci27Desorption process from Laser Treated Sample with Argon (500 L)General behaviour between 30 and 100 KNo visible peak at 20 K (P1)Huge peak at 30 K (P2)

Temperature Programmed Desorption (TPD)

P1

P2

Slide29

Laser Treated Sample

CERN 10/09/17

Marco Angelucci28Adsorption process of Argon (2000 L) on Laser Treated sample at 10 KNo “significant” variation of SEY

minor differences in the starting pointΔ = 0.1From 0.4 (10 K) to 0.5 (2000 L) (@900 eV)

Slide30

Laser Treated Sample

CERN 10/09/17

Marco Angelucci29Desorption process from Laser Treated Sample with Argon (2000 L)General behaviour between 30 and 100 KVisible peak at 20 K (P1)Huge peak at 30 K (P2)

Temperature Programmed Desorption (TPD)

P1

P2

Slide31

Laser Treated Sample

CERN 10/09/17Marco Angelucci

30

Temperature Programmed Desorption (TPD) P1P2P1P2

Slide32

Laser Treated Sample

CERN 10/09/17Marco Angelucci

31CuLaserLaser500 L2000 L160 L

Temperature Programmed Desorption (TPD)

Slide33

Laser Treated Sample

CERN 10/09/17Marco Angelucci

32P1 (@ 20 K) (10-7 mbar)P2 (@ 30 K) (10-7 mbar)Cu (160 L)0.10.45Laser Treated (500 L)0.0132Laser Treated (2000 L)0.18

7

Maximum pressure during desorption process

Slide34

Argon Results (Laser Treated)

Berlin 30/05/17

Marco Angelucci33System returns to the original state with slight differences Differences with Cu in the range around 20 KDesorption Process (Heating)

Strong Variation during cooling process (contaminants)

No significant SEY variation during Argon Adsorption (up to 2000 L)

Adsorption Process (LT)

Slide35

Important Tasks

Study the adsorption and desorption processes on “As Received” samples

Adsorption/Desorption processes with different gasesCERN 10/09/17Marco Angelucci34

Slide36

LNF-Lab Activities

SEY of Clean metals

SEY of clean Cu with low contaminantsAdsorption and Desorption processes from different surfaces (clean Cu, Laser Treated sample) with Carbon-MonoxideInteraction between electron and ArgonContribution of reflected Electrons to the Low-Energy SEY (Graphite, Cu, Cu with Argon)CERN 10/09/17Marco Angelucci35

Slide37

CO Adsorption (SEY)

CERN 10/09/17Marco Angelucci

36Two different regions High Energy(>50 eV)Low Energy(<50 eV)SEY @ 1000 eV decreases during deposition from 1.4 to 1.1

Formation of CO Thick Film (TF)Characteristic peak of TF at 65 eVAdsorption process of Carbon Monoxide on Cu sample at 10KGeneral behaviour

Slide38

CO Adsorption (SEY)

CERN 10/09/17Marco Angelucci

37Two different regions High Energy(>50 eV)Low Energy(<50 eV)Characteristic peaks at different low energiesFormation of Argon Single Layer (SL)

Adsorption process of Argon on Cu sample at 10KLow Energy behaviour

Slide39

CO Results (SEY)

CERN 10/09/17

Marco Angelucci38Formation of a TF with Low SEYAdsorption Process (10 K)

Characteristic peaks for SL in the Low Energy Region

Slide40

LNF-Lab Activities

SEY of Clean metals

SEY of clean Cu with low contaminantsAdsorption and Desorption processes from different surfaces (clean Cu, Laser Treated sample)Interaction between electron and ArgonContribution of reflected Electrons to the Low-Energy SEY (Graphite, Cu, Cu with Argon)CERN 10/09/17Marco Angelucci39

Slide41

Argon Adsorption II (SEY)

CERN 10/09/17Marco Angelucci

4010We can summarize the results observed forAr adsorption on Cu sample at 10 K

Slide42

e--

Argon Interaction (SEY)CERN 10/09/17

Marco Angelucci4110Subsequent SEY scans on the Ar-dosed Cu sample

Slide43

e

--Argon (SEY)

CERN 10/09/17Marco Angelucci42GAS ON: AdsorptionGAS OFF: e- DesorptionContinuous SEY scansSEY at 930 decreases as a function of time

SEY at 10 eV remains constante- bombardment induced different behaviour

Slide44

e--Argon (SEY)

CERN 10/09/17

Marco Angelucci43SEY measured in different pointsNew Point presents different SEY spectra with the same features of SEY with large amount of Ar

Slide45

e--Argon (SEY) II

CERN 10/09/17

Marco Angelucci44900 eV400 eVElectron Stimulated Desorption at different EnergiesStrong Interaction (desorption) with HE electrons

Slide46

e--Argon (SEY) II

CERN 10/09/17

Marco Angelucci4510 eVElectron Stimulated Desorption at different EnergiesLow interaction (no desorption) with LE electrons

Slide47

e--Argon (SEY)

CERN 10/09/17

Marco Angelucci46Continuous SEY scans (mass spec. signal)complete SEY scan

Study Electron Stimulated Desorption with Mass spectrometer

Slide48

e

Argon results (SEY)CERN 10/09/17Marco Angelucci47Argon Thick film interacts with primary electrons and desorbsBeam-Layer Interaction

Slide49

Beam Interaction

CERN 10/09/17Marco Angelucci

48Thermal DesorptionElectron beam dependence (size, energy …)

Non-Thermal Desorption

Slide50

Important Tasks

Study the adsorption and desorption processes on “As Received” samples

Adsorption/Desorption processes with different gasesStudy the Electron Stimulated Desorption with different parametersCERN 10/09/17Marco Angelucci49

Slide51

LNF-Lab Activities

SEY of Clean metals

SEY of clean Cu with low contaminantsAdsorption and Desorption processes from different surfaces (clean Cu, Laser Treated sample)Interaction between electron and ArgonContribution of reflected Electrons to the Low-Energy SEY (Graphite, Cu, Cu with Argon)CERN 10/09/17Marco Angelucci50

Slide52

Low-Energy SEY

CERN 10/09/17Marco Angelucci

51CO

Ar10Different LE-SEY structuresdepending from adsorbed gasesStudy of reflected e- contribution

Slide53

Low Energy SEY

CERN 10/09/17Marco Angelucci

52”Probabilistic model for the simulation of secondary electron emission” M. A. Furman and M. T. F. Pivi Phys. Rev. ST Accel. Beams 5, 124404 (2002)SEY: Total number of electrons emitted (TEE , TEY,...)True secondaries: number of electrons emitted between 0-50 eV. (if EP > 50 eV.)Backscattered electrons (Reflected): number of electrons emitted at E

P (+ D)Rediffused electrons: number of electrons emitted between 50 eV and EP – D (if EP > 50 eV.)

Slide54

Low Energy SEY

CERN 10/09/17Marco Angelucci

53abdd

SERSERSERSER

d

c

b

a

Evaluation of Reflected

(R)

and True Secondary (SE) electrons parts

Cimino

et al., PRL 93 (2004)

Slide55

CERN 10/09/17

Marco Angelucci

54WfWf

WfEp= 2 eVEp= 6.5 eVEp= 20 eVEp= 130 eVEp= 310 eVPlotting all the data normalizing to UNITY the intensity of the EDC @ Ep< WfOrIntegrating the curves: (when Ep <50 eV)

0 to E

P

D (

True Secondary)

E

P

D

to

E

P

+

D (

Elastically Back.)

(

when Ep

> 50

eV

)

0 to

50 eV

(

True Secondary

)

50 eV to

E

P

D

(

Rediffused

)

E

P

D

to

E

P

+

D (

Elastically Back.)

D

Low Energy SEY

Slide56

Low Energy SEY

CERN 10/09/17Marco Angelucci

55Clean Poly-Cu SEYEDCsReflected electrons in CopperPlotting all the data normalizing to UNITY the intensity of the EDC @ Ep< WfStructures in SEY are oscillations in the elastically backscattered components

Slide57

Low Energy SEY

CERN 10/09/17Marco Angelucci

56Reflected electrons in CopperDifferent ContributionsSEYSecond.Redif.

Reflec

.

SEY

Second.

Redif

.

Reflec

.

Slide58

Low Energy SEY

CERN 10/09/17Marco Angelucci

57Reflected electrons in CopperDifferent Contributions

SEYSecond.Redif.Reflec.

Slide59

Low Energy SEY

CERN 10/09/17Marco Angelucci

58Reflected electrons in GraphiteSEYEDCsPlotting all the data normalizing to UNITY the intensity of the EDC @ Ep< WfStructures in SEY are oscillations in the elastically backscattered components

Slide60

Low Energy SEY

CERN 10/09/17Marco Angelucci

59Reflected electrons in GraphiteDifferent ContributionsSEYSecond.Reflec.Redif.SEY

Second.Reflec.Redif.

Slide61

Low Energy SEY

CERN 10/09/17Marco Angelucci

60Ar monolayerAr multilayerSEYEDCsSEYEDCs

Reflected electrons in Argon

Slide62

Low Energy SEY

CERN 10/09/17Marco Angelucci

61... and: Bauer: “Surface microscopy with low

energy electrons” Springher 2014

Slide63

Important Results I

CERN 10/09/17

Marco Angelucci62

Follow Adsorption process checking the High-Energy SEY (HE-SEY)Distinguish Single Layer (SL) from Thick Film (TF) formation by Low-Energy SEY (LE-SEY) Quantify the number of adsorbed layers on surfaceMeasure Work Function (WF) variation

Slide64

Important

Results II

CERN 10/09/17Marco Angelucci63

Measure the desorption temperature of TF and SL with SEY and TPDStudy the Electron Stimulated Desorption with mass spectrometer (quantify desorption)Study the contribution of reflected e- to Low-Energy SEYStudy the influence of the adsorbed gas in the Low-Energy SEY

Slide65

Maintenance /Upgrades I

CERN 10/09/17

Marco Angelucci64

Non Standard chamber maintenance (open system)Implementations for Induced Desorption Studies

Standard chamber maintenance (

transfer)

Preparation chamber

Implemented data acquisition software

Slide66

Future Activities

CERN 10/09/17Marco Angelucci

65Synchrotron BeamlinesXUV2: High Energy 60-1000 eV. XUV1: High Energy 30-150 eV.

Slide67

Maintenance /Upgrades II

CERN 10/09/17

Marco Angelucci66

Connection (2/3 month)System optimization for experiment with electrons and photons

Alignment of Sychrotron beamlines

Preparation for connection with Experimental Chamber

Slide68

Future Activities

CERN 10/09/17Marco Angelucci

67

Different Gases adsorption (CO, CO2, CH4 ...) (pure and mixture) Electron Stimulated Desorption Measurements on treated samples (continue)Study of reflected electron on different systems

Different studies with Synchrotron light

Slide69

e—cloud conference

CERN 10/09/17

Marco Angelucci68... Which will reconvene in Elba in June 2018

Slide70

Argon Adsorption (SEY)

CERN 10/09/17Marco Angelucci

69Adsorption process of Argon on Cu sample at 10 KGeneral behaviourTwo different regionswith characteristic trends Low Energy(<50 eV)Thick Film (TF)

High Energy(>50 eV)Single Layer (SL)

Slide71

Argon Adsorption (SEY)

CERN 10/09/17Marco Angelucci

70Two different regionswith characteristic trends Low Energy(<50 eV)Thick Film (TF)

High Energy(>50 eV)Single Layer (SL)

Slide72

e--Argon (SEY) II

CERN 10/09/17

Marco Angelucci71

Slide73

Laser Treated Sample

CERN 10/09/17Marco Angelucci

72

Slide74

LNF-Lab Activities II

CERN 10/09/17Marco Angelucci

73Working Parameters:Basic Pressure ≤ 1x10-10 mbarElectron Beam Current < 1x10-7 Ampere (A) (Max Current @ max electron energy)Electron Beam Energy from 75 to 1000 eVSample Bias 75 VSingle Spectra Acquisition Time ≈ 120 secBeam Radius < 1.0 mm1 Langmuir (L) = 1 sec @ 1x10-6 mbar1 L = 1 Mono-Layer (ML) (with sticking coefficient = 1)Temperature range: form 10 to 300 K

Slide75

LNF-lab Activities II

Why start with Atomically Sputtered clean Copper?

CERN 10/09/17Marco Angelucci74Electron Beams have not effect on a clean surface so any modification to the SEY can be attributed to atoms and molecules on surface.easy to single out contamination (sample pumping) from experimental.easy to eliminate spurious and otherwise occurring scrubbing effects from real non-clean surfaces.

Slide76

LNF-lab Activities II

CERN 10/09/17Marco Angelucci

75Experimental Test with Atomically Sputtered CopperFirst observable changes (blu) after 0.02C/mm2  more than 6 h SEY measurementsMore significant changes (green) needs more than 60 h continuous measuringOur standard SEY lasts 120s!

Thanks to: Luis Gonzalezat P = 2x10-10 mbar

Slide77

LNF-lab Activities II

Why Argon and Carbon-Monoxide?

CERN 10/09/17Marco Angelucci76Argon is a inert gas and it’s the best starting point to study SEY al Low TemperatureCarbon-Monoxide is a gas of great interest for accelerator physics

Slide78

LNF-lab Activities II

CERN 10/09/17Marco Angelucci

77Reference Literature spectra of Argon and Carbon-Monoxide SEYJ. Cazaux et al.: Phys. Rev. B 71 (2005) 035419Argon

A. Kuzucan et al.: J. of Vacuum Sci. & Tech. A 30 (2012) 051401Carbon-Monoxide