nc 200 test data

Upload: divyanshu-bhatnagar

Post on 04-Apr-2018

214 views

Category:

Documents


0 download

TRANSCRIPT

  • 7/30/2019 Nc 200 Test Data

    1/9

    1. Deposition rate measurements

    A quartz crystal monitor (at a distance of 100mm from the source aperture) was usedto measure the deposition rate of the clusters (note for Cu, 1Hz = 0.11).

    The deposition rate was measured as a function of the magnetron power for variousAr flow rates and a set aggregation length of 205 mm.

    0 50 100 150 200 250

    0

    50

    100

    150

    200

    Depositionrate(Hz/min)

    Power (W)

    Ar 25 sccm

    Ar 20 sccm

    Ar 15 sccm

    Ar 10 sccm

    Figure 2: Deposition rate as a function of magnetron power for various flows

    The deposition rate was measured as a function of the Ar gas flow rate for variousaggregation lengths and a fixed power of 25Watts.

    0 5 10 15 20 25 30

    0

    20

    40

    60

    80

    100

    120

    140

    160

    Depositionrate(Hz/min)

    Ar flow (sccm)

    Distance 205 mm

    Distance 195 mm

    Distance 155 mm

    Distance 85 mm

    Figure 3: Deposition rate as a function of Ar gas flow rate for various aggregation lengths

  • 7/30/2019 Nc 200 Test Data

    2/9

    Note that the deposition rate drops at higher Ar flow and magnetron power. This isdue to the increased number of collisions between particles and thus a reduction in themean free path of the clusters.

    2. Cluster mass measurements

    Cluster mass with Ar flow rateThe Ar flow rate was varied for a fixed power and aggregation length. The resultingmass spectra (taken using the QMF200) are shown below of negatively charged Cuclusters.Power: 38W, Agg length: minimum, He: 0 sccm, Apertures 5mm inner, 4mm outer.

    01x10

    5

    2x10

    5

    3x10

    5

    4x10

    5

    5x10

    5

    6x10

    5

    0

    1

    2

    3

    4

    5

    6

    7

    8

    9Cu Mass Spectra with Ar Flow Rate

    ClusterIonCurrent(x1010A)

    Mass (a.m.u.)

    10sccm

    30sccm

    50sccm

    70sccm90sccm

    Figure 4.

    From these spectra the mean cluster mass can be plotted as a function of the Ar flow.This is shown below in figure 2.

  • 7/30/2019 Nc 200 Test Data

    3/9

    0 20 40 60 80 100

    4.0x104

    6.0x104

    8.0x104

    1.0x105

    1.2x105

    1.4x105

    1.6x105

    1.8x105

    2.0x105

    2.2x105

    2.4x105

    Relationship between mean cluster mass

    and Ar gas flow for Cu clusters

    ClusterMass(amu)

    Ar Flow (sccm)

    Figure 5

    Cluster mass with He flow rateThe He flow rate was varied for a fixed power, aggregation length and Ar flow rate.The resulting mass spectra (taken using the QMF200) are shown below of negativelycharged Cu clusters.Power: 37W, Agg length: minimum, Ar: 20 sccm, Apertures 5mm inner, 4mm outer.

    0 1x105

    2x105

    3x105

    4x105

    5x105

    6x105

    7x105

    0

    2

    4

    6

    8

    10

    ClusterIonCurrent(x1010A)

    Cu mass spectra with He flow rate

    Mass (a.m.u.)

    0sccm

    10sccm

    30sccm

    50sccm

    70sccm

    90sccm

    Figure 6

    From these spectra the mean cluster mass can be plotted as a function of the He flow.This is shown below in figure 4.

  • 7/30/2019 Nc 200 Test Data

    4/9

    0 20 40 60 80 100

    6.0x104

    8.0x104

    1.0x105

    1.2x105

    1.4x105

    1.6x105

    Relationship between mean cluster mass

    and He flow for Cu clusters

    ClusterMass(a.m.u.

    )

    He Flow (sccm)

    Figure 7

    Cluster mass with magnetron powerThe magnetron power was varied for a fixed aggregation length, Ar and He flowrates. The resulting mass spectra (taken using the QMF200) are shown below ofnegatively charged Cu clusters.Agg length: minimum, Ar: 40 sccm, He: 60sccm, Apertures 5mm inner, 4mm outer.

    0.0 5.0x104

    1.0x105

    1.5x105

    2.0x105

    2.5x105

    3.0x105

    3.5x105

    0

    1

    2

    3

    4

    5

    6

    7

    ClusterIonCurrent(x1010A)

    Cu mass spectra with power

    Mass (a.m.u.)

    35W

    30W

    25W

    20W

    15W

    Figure 8

    From these spectra the mean cluster mass can be plotted as a function of the power.This is shown below in figure 6.

  • 7/30/2019 Nc 200 Test Data

    5/9

    15 20 25 30 35 402x10

    4

    3x104

    4x104

    5x104

    6x104

    7x104

    8x104

    9x104

    Relationship between mean cluster mass

    and power for Cu clusters

    Mass(a.m.u.)

    Power (Watts)

    Figure 9

    Cluster mass with aggregation lengthThe aggregation length was varied for a fixed power, Ar and He flow rates. Theresulting mass spectra (taken using the QMF200) are shown below of negatively

    charged Cu clusters.Power: 35W, Ar: 15 sccm, He: 0sccm, Apertures 5mm inner, 4mm outer.

    0 1x105

    2x105

    3x105

    4x105

    5x105

    6x105

    0.0

    0.5

    1.0

    1.5

    2.0

    2.5

    3.0

    3.5

    4.0

    4.5

    5.0

    5.5

    6.0

    6.5

    7.0

    7.5

    8.0

    ClusterIonCurrent(x1010A)

    Cu mass spectra with aggregation length

    Cluster mass (a.m.u.)

    65mm

    95mm

    125mm

    155mm

    Figure 10

  • 7/30/2019 Nc 200 Test Data

    6/9

    Large clusters

    Large clusters can be acquired with the NC200U using high powers and relativelyhigh Ar gas flows. The graph below shows such a spectrum which goes beyond therange of the QMF200. These clusters are positively charged.Power : 95W, Ar flow: 65sccm, He:0, Aggregation length: maximum.

    0.0 5.0x105

    1.0x106

    1.5x106

    2.0x106

    2.5x106

    3.0x106

    0.0

    0.5

    1.0

    1.5

    2.0

    2.5

    3.0Large Cu clusters from the NC200U source

    IonCurre

    nt(nA)

    Mass (a.m.u.)

    Figure 11

  • 7/30/2019 Nc 200 Test Data

    7/9

    Small clusters

    Small clusters can be acquired with the NC200U using low powers and high He gasflows. The graph below shows spectra of negatively charged clusters for two differentHe flows. Individual cluster peaks can just be resolved.Power : 10W, Ar flow: 35sccm, He flow:110sccm, 90sccm Aggregation length:minimumQMF: f=100kHz, U/V =0.15, Sit=0, External Keitherly nanometer input.

    0 200 400 600 800 1000 1200 1400 1600 1800

    0.2

    0.4

    0.6

    0.8

    1.0

    1.2

    1.4

    1.6

    ClusterIonCurrent(x1

    010A)

    BA

    Mass (a.m.u.)

    110sccm He

    90sccm He

    Figure 12

  • 7/30/2019 Nc 200 Test Data

    8/9

    From the above graph the value of k (the correction factor) can be calculated. Thevalue k is used in the calculation of the mass:

    M=7x107(kV/f2d2)

    Where M is the mass, V is the AC voltage, f is the frequency and d is the diameter ofthe quadrupole poles.

    On the graph the peaks A and B lie at 500amu and 793amu. There are five distinctpeaks between these peaks giving an average separation of 48.8amu. For Cu clustersthis value should be 63.5 (the atomic weight of Cu). The correction factor is therefore:

    k= 63.5/48.8 = 1.30

    This value is comparable with the result calculated by Baker et al1. (1.25) whodetermined the constant by using ionised Ar. The corrected mass spectrum is shown

    in figure 10. The number of atoms per cluster has been added.

    0 200 400 600 800 1000 1200 1400 1600 1800 2000

    0.5

    1.0

    1.5

    ClusterIonCurrent(x1010A)

    Mass (a.m.u.)

    1716

    15

    14131211

    10

    9

    8

    7

    6

    110sccm He

    90sccm He

    Figure 13

    1 S.H.Baker et al. Rev.Sci.Instrum. 68(4) p 1853, 1997.

  • 7/30/2019 Nc 200 Test Data

    9/9

    3. Other measurements

    Beam size from cluster sourceThe beam diameter was measured for different aperture plate arrangements at adistance of 100mm.

    -40 -30 -20 -10 0 10 20 30 40

    0.0

    0.2

    0.4

    0.6

    0.8

    1.0Red - 4mm inner, 5mm skimmer

    Black - 4mm inner, 10mm skimmer

    Blue - 8mm inner, 10mm skimmer

    NC200U Beam profiles with different aperture

    arrangements at a distance of 100mm

    Depositionrate(normalised)

    Distance (mm) Figure 14