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XRD and XRF are highly complementary

materials analysis methods which, when used

together, greatly improve the accuracy of

phase identification and quantitative analysis.

The combination of both methods provides an

increase in the numbers of measured parameters,

which means that fewer assumptions are needed

for analysis. This in turn provides not only greater

accuracy of results, but also increases the range

of samples that can be measured to include

samples about which little or nothing is known in

advance.

XRD is the most direct and accurate analytical

method for determining the presence and

absolute amounts of mineral species in a sample.

Ambiguous results may be obtained however, if

the sample chemistry and/or origin are unknown.

In these cases phase identification can be difficult;

in particular, isostructural phases with similar

chemical composition will give similar powder

diffraction patterns.

In contrast to XRD, XRF provides highly accurate

information about the elemental composition

of a sample, but it cannot deliver direct phase

information. Mass-balance calculations may give

sufficient phase information in some cases, but

can also lead to meaningless results e.g. in the

presence of polymorphs.

It is the complimentary nature of the XRD and

XRFmethods which makes them a valuable

tool for quantitative phase analysis in numerous

applications ranging from scientific research

to industrial high-throughput quality control.

Particularily in mineralogical and geological

application areas, the combined use of XRD and

XRF is booming, offering completely new insights

into materials and processes. Typical examples

are the cement, minerals & mining, and industrial

minerals industries, where the quality of products

and / or efficiency of processes is governed by

both phase and elemental composition. The

combined use of XRD and XRF methods allows

the reliable analysis of materials, for which the

individual methods fail to deliver accurate and

reliable results.

Page 2

Quantitative phase and element analysis of

host/waste rocks and tailings is an important

application in the minerals and mining industry

with respect to both process optimization (e.g.

acid leaching) and environmental protection:

Mining and milling operations are responsible

for the production of billions of tonnes of waste

rock and finely crushed tailings worldwide. An

important application is the knowledge of the

relative amounts of the minerals with acid-

producing or neutralization potential for successful

acid-base accounting with respect to both the

leaching process as well as acid mine drainage,

with its detrimental effects on environment.

As an example, we report combined XRD-XRF

analysis of an intrusive rock with unknown

composition. Of particular interest was its

classification by mineral content as well as

the detection and accurate quantification of

potentially present minerals with significant acid-

producing or neutralization potential.

Powder diffraction data were recorded using a

D4 ENDEAVOR powder diffractometer equipped

with a LynxEye

TM

detector (Fig. 1); the total

measurement time required was about 5 minutes.

For phase identification and quantification,

the DIFFRAC

plus

software packages EVA,

SEARCH and TOPAS were used. Standardless

XRFmeasurements on the same sample were

performed with the S4 PIONEER and the

SPECTRA

plus

software (Fig. 1).

Fig. 1: D4 ENDEAVOR diffractometer (right)

and S4 PIONEER spectrometer (left) connected

with conveyer belt. The D4 is equipped with

Super Speed LynxEye

TM

detector.

Fig. 2: EVA phase identification results.

1) Phase identification

Fig. 2 and Tab. 1 show the XRD powder data and

the phase identification results. The major rock

forming minerals plagioclase, quartz, diopside

and muscovite are easily and correctly identified

in a single default run. Note, that the highly

sensitive SEARCH algorithm clearly prefers albite

(Na-plagioclase) versus anorthite (Ca-plagioclase)

as a result of the slightly different lattice

parameters of both plagioclase solid solution

end members. Best SEARCH figure-of-merits

obtained for the individual phases were 0.65 and

1.48, respectively. Neither ore minerals nor any

K-feldspars or feldspathoids could be detected.

Tab. 1: EVA phase identification results.

SS-VVV-PPPP

Compound Name

00-009-0466 (*)

Albite

00-041-1480 (I)

Albite, calcian

03-065-0466 (C)

Quartz low, syn

01-087-0700 (C)

Diopside, syn

01-089-5402 (C)

Muscovite 2M1

Page 3

Fig. 3: EVA combined XRD-XRF results -

comparison of calculated (column "SQD") versus

observed (column "XRF") element concentrations.

The difference is given in column "Delta".

2) Combined XRD-XRF analysis

To confirm the phase identification results,

and to obtain semi-quantitative phase amount

estimates consistent with the actual elemental

composition of the sample, combined XRD-XRF

analysis has been performed with EVA. EVA

enables semi-quantitative analysis based on the

reference-intensity-ratio (RIR) method using both

XRD as well as XRFdata simultaneously: On

scaling the maximum intensities of the ICDD PDF

patterns to the observed peaks in the powder

pattern, EVA calculates both phase and element

concentrations, and compares the latter with the

actually measured element concentrations.

Element concentrations as obtained by XRF and

used by EVA are provided in Tab. 2. Already at

first glance, the XRF data fully confirm the absence

of any significant acid-producing ore minerals

due to the minor concentrations found for heavy

elements and the absence of sulphur.

Tab. 2: Element concentrations [%] as obtained by XRF.

Oxygen

47.7

Silicon

30.0

Aluminum 9.75

Sodium

6.1

Calcium

3.66

Magnesium 0.456

Iron

1.35

Potassium

0.271

Phosphorus 0.114

Chlorine

0.0445

Titanium

0.252

Manganese 0.0173

Cobalt

0.0182

Nickel

0.0142

Strontium

0.0595

Zirconium

0.0143

Barium

0.0258

Wolfram

0.101

The results for combined XRD-XRF analysis with

EVA are shown in Fig. 3 and Tab. 3. The high Na

vs. Ca concentrations confirm the presence of Na-

plagioclase as found by XRD (diopside accounts

for about 60% of the total Ca, as calculated

by EVA). The present Na-plagioclase is most

successfully modelled using two albite phases

with different Ca amounts. Note the excellent

agreement found between the calculated and

observed element concentrations, which is better

than 1% for all elements, and therefore confirms

the correctness of the XRD phase identification

results for all phases.

The accuracy of the RIR method is limited by

several factors such as preferred orientation

effects and the quality of the ICDD PDF data used

(e.g. quality of relative intensities, I/Icor values,

idealized chemical formula).

Tab. 3: EVA semi-quantitative phase analysis

results based on combined XRD-XRF using

reference intensities as given in the ICDD PDF

patterns.

SS-VVV-PPPP

Compound Name

Phase

amounts

00-009-0466 (*)

Albite

58.2%

00-041-1480 (I)

Albite, calcian

15.4%

03-065-0466 (C) Quartz low, syn

14.0%

01-087-0700 (C) Diopside, syn

9.9%

01-089-5402 (C) Muscovite 2M1

2.6%

The most accurate quantitative results will be

obtained from a TOPAS Rietveld refinement. The

combined XRD-XRF results obtained are of high

value for defining the refinement model.

Page 4

BRUKER AXS, INC.

5465 EAST ChERYL pARKwAY

MADISON, wI 53711-5373

USA

TEL. (+1) (800) 234-XRAY

TEL. (+1) (608) 276-3000

FAX (+1) (608) 276-3006

email info@bruker-axs.com

www.bruker-axs.com

All configurations and specifications are subject to change without notice. Order No. L88-E00058. © 2006 BRUKER AXS GmbH. Printed in Germany.

BRUKER AXS GMBh

OESTLIChE RhEINBRUECKENSTR. 49

D-76187 KARLSRUhE

GERMANY

TEL. (+49) (0)(721)595-2888

FAX (+49) (0)(721)595-4587

EMAIL info@bruker-axs.de

www.bruker-axs.de

BRUKER AXS K.K

3-9-A, MORIYA, KANAGAwA

YOKOhAMA, KANAGAwA 221-0022

Japan

TEL. (+81) 45 453 1963

FAX (+81) 45 440 0757

www.bruker-axs.com

3) Quantitative TOPAS refinement

Quantitative Rietveld analysis has been

performed using TOPAS, the results are shown

in Fig. 4 and Tab. 4. For the final refinement

two Na-plagioclases with different compositions

have been used to model the data to take the

elemental analysis results into account: Albite (0%

Ca) and Oligoclase (25% Ca).

From the results in Tab. 4 the following

conclusions can be drawn:

1. The sample can be unambiguously classified as

a quartzdiorite according to Streckeisen, see Fig. 5.

2. Combined XRD-XRF analysis and TOPAS

Rietveld refinement can allow a distinction of even

neighboring plagioclase solid solution members

(here albite and oligoclase) if present in sufficient

amounts.

The present sample can be characterised as

a rock with insignificant acid producing or

neutralisation potential. Remarkable is the easy

and reliable determination of the plagioclase type

for estimation of the neutralisation potential. This

ability is of particular interest, as anorthite has

an about 14x higher neutralisation potential than

albite (e.g. Jambor et al., 2002).

Fig. 4: Quantitative TOPAS refinement results.

Tab. 4: Quantitative TOPAS refinement results.

Compound Name

Phase amounts

Albite

49.6%

Oligoclase

30.5%

Quartz

9.9%

Diopside

8.8%

Muscovite

1.2%

Fig. 5: Streckeisen diagram for intrusive rocks.

Q: quartz, A: alkali-feldspar, P: plagioclase.

Reference

J.L. Jambor, J.E. Dutrizac, L.A. Groat, M. Raudsepp.

Environmental Geology (2002) 43, 1-17.

Q

A

P

granite

grano-

diorite

quartz-rich

granodiorite

quartz-

syenite

quartz-

monzonite

quartz-

monzo-

diorite

quartz-

diorite

tonalite

XRD and XRF are highly complementary

materials analysis methods which, when used

together, greatly improve the accuracy of

phase identification and quantitative analysis.

The combination of both methods provides an

increase in the numbers of measured parameters,

which means that fewer assumptions are needed

for analysis. This in turn provides not only greater

accuracy of results, but also increases the range

of samples that can be measured to include

samples about which little or nothing is known in

advance.

XRD is the most direct and accurate analytical

method for determining the presence and

absolute amounts of mineral species in a sample.

Ambiguous results may be obtained however, if

the sample chemistry and/or origin are unknown.

In these cases phase identification can be difficult;

in particular, isostructural phases with similar

chemical composition will give similar powder

diffraction patterns.

In contrast to XRD, XRF provides highly accurate

information about the elemental composition

of a sample, but it cannot deliver direct phase

information. Mass-balance calculations may give

sufficient phase information in some cases, but

can also lead to meaningless results e.g. in the

presence of polymorphs.

It is the complimentary nature of the XRD and

XRFmethods which makes them a valuable

tool for quantitative phase analysis in numerous

applications ranging from scientific research

to industrial high-throughput quality control.

Particularily in mineralogical and geological

application areas, the combined use of XRD and

XRF is booming, offering completely new insights

into materials and processes. Typical examples

are the cement, minerals & mining, and industrial

minerals industries, where the quality of products

and / or efficiency of processes is governed by

both phase and elemental composition. The

combined use of XRD and XRF methods allows

the reliable analysis of materials, for which the

individual methods fail to deliver accurate and

reliable results.

Page 2

Quantitative phase and element analysis of

host/waste rocks and tailings is an important

application in the minerals and mining industry

with respect to both process optimization (e.g.

acid leaching) and environmental protection:

Mining and milling operations are responsible

for the production of billions of tonnes of waste

rock and finely crushed tailings worldwide. An

important application is the knowledge of the

relative amounts of the minerals with acid-

producing or neutralization potential for successful

acid-base accounting with respect to both the

leaching process as well as acid mine drainage,

with its detrimental effects on environment.

As an example, we report combined XRD-XRF

analysis of an intrusive rock with unknown

composition. Of particular interest was its

classification by mineral content as well as

the detection and accurate quantification of

potentially present minerals with significant acid-

producing or neutralization potential.

Powder diffraction data were recorded using a

D4 ENDEAVOR powder diffractometer equipped

with a LynxEye

TM

detector (Fig. 1); the total

measurement time required was about 5 minutes.

For phase identification and quantification,

the DIFFRAC

plus

software packages EVA,

SEARCH and TOPAS were used. Standardless

XRFmeasurements on the same sample were

performed with the S4 PIONEER and the

SPECTRA

plus

software (Fig. 1).

Fig. 1: D4 ENDEAVOR diffractometer (right)

and S4 PIONEER spectrometer (left) connected

with conveyer belt. The D4 is equipped with

Super Speed LynxEye

TM

detector.

Fig. 2: EVA phase identification results.

1) Phase identification

Fig. 2 and Tab. 1 show the XRD powder data and

the phase identification results. The major rock

forming minerals plagioclase, quartz, diopside

and muscovite are easily and correctly identified

in a single default run. Note, that the highly

sensitive SEARCH algorithm clearly prefers albite

(Na-plagioclase) versus anorthite (Ca-plagioclase)

as a result of the slightly different lattice

parameters of both plagioclase solid solution

end members. Best SEARCH figure-of-merits

obtained for the individual phases were 0.65 and

1.48, respectively. Neither ore minerals nor any

K-feldspars or feldspathoids could be detected.

Tab. 1: EVA phase identification results.

SS-VVV-PPPP

Compound Name

00-009-0466 (*)

Albite

00-041-1480 (I)

Albite, calcian

03-065-0466 (C)

Quartz low, syn

01-087-0700 (C)

Diopside, syn

01-089-5402 (C)

Muscovite 2M1

Page 3

Fig. 3: EVA combined XRD-XRF results -

comparison of calculated (column "SQD") versus

observed (column "XRF") element concentrations.

The difference is given in column "Delta".

2) Combined XRD-XRF analysis

To confirm the phase identification results,

and to obtain semi-quantitative phase amount

estimates consistent with the actual elemental

composition of the sample, combined XRD-XRF

analysis has been performed with EVA. EVA

enables semi-quantitative analysis based on the

reference-intensity-ratio (RIR) method using both

XRD as well as XRFdata simultaneously: On

scaling the maximum intensities of the ICDD PDF

patterns to the observed peaks in the powder

pattern, EVA calculates both phase and element

concentrations, and compares the latter with the

actually measured element concentrations.

Element concentrations as obtained by XRF and

used by EVA are provided in Tab. 2. Already at

first glance, the XRF data fully confirm the absence

of any significant acid-producing ore minerals

due to the minor concentrations found for heavy

elements and the absence of sulphur.

Tab. 2: Element concentrations [%] as obtained by XRF.

Oxygen

47.7

Silicon

30.0

Aluminum 9.75

Sodium

6.1

Calcium

3.66

Magnesium 0.456

Iron

1.35

Potassium

0.271

Phosphorus 0.114

Chlorine

0.0445

Titanium

0.252

Manganese 0.0173

Cobalt

0.0182

Nickel

0.0142

Strontium

0.0595

Zirconium

0.0143

Barium

0.0258

Wolfram

0.101

The results for combined XRD-XRF analysis with

EVA are shown in Fig. 3 and Tab. 3. The high Na

vs. Ca concentrations confirm the presence of Na-

plagioclase as found by XRD (diopside accounts

for about 60% of the total Ca, as calculated

by EVA). The present Na-plagioclase is most

successfully modelled using two albite phases

with different Ca amounts. Note the excellent

agreement found between the calculated and

observed element concentrations, which is better

than 1% for all elements, and therefore confirms

the correctness of the XRD phase identification

results for all phases.

The accuracy of the RIR method is limited by

several factors such as preferred orientation

effects and the quality of the ICDD PDF data used

(e.g. quality of relative intensities, I/Icor values,

idealized chemical formula).

Tab. 3: EVA semi-quantitative phase analysis

results based on combined XRD-XRF using

reference intensities as given in the ICDD PDF

patterns.

SS-VVV-PPPP

Compound Name

Phase

amounts

00-009-0466 (*)

Albite

58.2%

00-041-1480 (I)

Albite, calcian

15.4%

03-065-0466 (C) Quartz low, syn

14.0%

01-087-0700 (C) Diopside, syn

9.9%

01-089-5402 (C) Muscovite 2M1

2.6%

The most accurate quantitative results will be

obtained from a TOPAS Rietveld refinement. The

combined XRD-XRF results obtained are of high

value for defining the refinement model.

Page 4

BRUKER AXS, INC.

5465 EAST ChERYL pARKwAY

MADISON, wI 53711-5373

USA

TEL. (+1) (800) 234-XRAY

TEL. (+1) (608) 276-3000

FAX (+1) (608) 276-3006

EMAIL info@bruker-axs.com

www.bruker-axs.com

All configurations and specifications are subject to change without notice. Order No. L88-E00058. © 2006 BRUKER AXS GmbH. Printed in Germany.

BRUKER AXS GMBh

OESTLIChE RhEINBRUECKENSTR. 49

D-76187 KARLSRUhE

GERMANY

TEL. (+49) (0)(721)595-2888

FAX (+49) (0)(721)595-4587

EMAIL info@bruker-axs.de

www.bruker-axs.de

BRUKER AXS K.K

3-9-A, MORIYA, KANAGAwA

YOKOhAMA, KANAGAwA 221-0022

JApAN

TEL. (+81) 45 453 1963

FAX (+81) 45 440 0757

www.bruker-axs.com

3) Quantitative TOPAS refinement

Quantitative Rietveld analysis has been

performed using TOPAS, the results are shown

in Fig. 4 and Tab. 4. For the final refinement

two Na-plagioclases with different compositions

have been used to model the data to take the

elemental analysis results into account: Albite (0%

Ca) and Oligoclase (25% Ca).

From the results in Tab. 4 the following

conclusions can be drawn:

1. The sample can be unambiguously classified as

a quartzdiorite according to Streckeisen, see Fig. 5.

2. Combined XRD-XRF analysis and TOPAS

Rietveld refinement can allow a distinction of even

neighboring plagioclase solid solution members

(here albite and oligoclase) if present in sufficient

amounts.

The present sample can be characterised as

a rock with insignificant acid producing or

neutralisation potential. Remarkable is the easy

and reliable determination of the plagioclase type

for estimation of the neutralisation potential. This

ability is of particular interest, as anorthite has

an about 14x higher neutralisation potential than

albite (e.g. Jambor et al., 2002).

Fig. 4: Quantitative TOPAS refinement results.

Tab. 4: Quantitative TOPAS refinement results.

Compound Name

Phase amounts

Albite

49.6%

Oligoclase

30.5%

Quartz

9.9%

Diopside

8.8%

Muscovite

1.2%

Fig. 5: Streckeisen diagram for intrusive rocks.

Q: quartz, A: alkali-feldspar, P: plagioclase.

Reference

J.L. Jambor, J.E. Dutrizac, L.A. Groat, M. Raudsepp.

Environmental Geology (2002) 43, 1-17.

Q

A

P

granite

grano-

diorite

quartz-rich

granodiorite

quartz-

syenite

quartz-

monzonite

quartz-

monzo-

diorite

quartz-

diorite

tonalite

XRD and XRF are highly complementary

materials analysis methods which, when used

together, greatly improve the accuracy of

phase identification and quantitative analysis.

The combination of both methods provides an

increase in the numbers of measured parameters,

which means that fewer assumptions are needed

for analysis. This in turn provides not only greater

accuracy of results, but also increases the range

of samples that can be measured to include

samples about which little or nothing is known in

advance.

XRD is the most direct and accurate analytical

method for determining the presence and

absolute amounts of mineral species in a sample.

Ambiguous results may be obtained however, if

the sample chemistry and/or origin are unknown.

In these cases phase identification can be difficult;

in particular, isostructural phases with similar

chemical composition will give similar powder

diffraction patterns.

In contrast to XRD, XRF provides highly accurate

information about the elemental composition

of a sample, but it cannot deliver direct phase

information. Mass-balance calculations may give

sufficient phase information in some cases, but

can also lead to meaningless results e.g. in the

presence of polymorphs.

It is the complimentary nature of the XRD and

XRFmethods which makes them a valuable

tool for quantitative phase analysis in numerous

applications ranging from scientific research

to industrial high-throughput quality control.

Particularily in mineralogical and geological

application areas, the combined use of XRD and

XRF is booming, offering completely new insights

into materials and processes. Typical examples

are the cement, minerals & mining, and industrial

minerals industries, where the quality of products

and / or efficiency of processes is governed by

both phase and elemental composition. The

combined use of XRD and XRF methods allows

the reliable analysis of materials, for which the

individual methods fail to deliver accurate and

reliable results.

Page 2

Quantitative phase and element analysis of

host/waste rocks and tailings is an important

application in the minerals and mining industry

with respect to both process optimization (e.g.

acid leaching) and environmental protection:

Mining and milling operations are responsible

for the production of billions of tonnes of waste

rock and finely crushed tailings worldwide. An

important application is the knowledge of the

relative amounts of the minerals with acid-

producing or neutralization potential for successful

acid-base accounting with respect to both the

leaching process as well as acid mine drainage,

with its detrimental effects on environment.

As an example, we report combined XRD-XRF

analysis of an intrusive rock with unknown

composition. Of particular interest was its

classification by mineral content as well as

the detection and accurate quantification of

potentially present minerals with significant acid-

producing or neutralization potential.

Powder diffraction data were recorded using a

D4 ENDEAVOR powder diffractometer equipped

with a LynxEye

TM

detector (Fig. 1); the total

measurement time required was about 5 minutes.

For phase identification and quantification,

the DIFFRAC

plus

software packages EVA,

SEARCH and TOPAS were used. Standardless

XRFmeasurements on the same sample were

performed with the S4 PIONEER and the

SPECTRA

plus

software (Fig. 1).

Fig. 1: D4 ENDEAVOR diffractometer (right)

and S4 PIONEER spectrometer (left) connected

with conveyer belt. The D4 is equipped with

Super Speed LynxEye

TM

detector.

Fig. 2: EVA phase identification results.

1) Phase identification

Fig. 2 and Tab. 1 show the XRD powder data and

the phase identification results. The major rock

forming minerals plagioclase, quartz, diopside

and muscovite are easily and correctly identified

in a single default run. Note, that the highly

sensitive SEARCH algorithm clearly prefers albite

(Na-plagioclase) versus anorthite (Ca-plagioclase)

as a result of the slightly different lattice

parameters of both plagioclase solid solution

end members. Best SEARCH figure-of-merits

obtained for the individual phases were 0.65 and

1.48, respectively. Neither ore minerals nor any

K-feldspars or feldspathoids could be detected.

Tab. 1: EVA phase identification results.

SS-VVV-PPPP

Compound Name

00-009-0466 (*)

Albite

00-041-1480 (I)

Albite, calcian

03-065-0466 (C)

Quartz low, syn

01-087-0700 (C)

Diopside, syn

01-089-5402 (C)

Muscovite 2M1

Page 3

Fig. 3: EVA combined XRD-XRF results -

comparison of calculated (column "SQD") versus

observed (column "XRF") element concentrations.

The difference is given in column "Delta".

2) Combined XRD-XRF analysis

To confirm the phase identification results,

and to obtain semi-quantitative phase amount

estimates consistent with the actual elemental

composition of the sample, combined XRD-XRF

analysis has been performed with EVA. EVA

enables semi-quantitative analysis based on the

reference-intensity-ratio (RIR) method using both

XRD as well as XRFdata simultaneously: On

scaling the maximum intensities of the ICDD PDF

patterns to the observed peaks in the powder

pattern, EVA calculates both phase and element

concentrations, and compares the latter with the

actually measured element concentrations.

Element concentrations as obtained by XRF and

used by EVA are provided in Tab. 2. Already at

first glance, the XRF data fully confirm the absence

of any significant acid-producing ore minerals

due to the minor concentrations found for heavy

elements and the absence of sulphur.

Tab. 2: Element concentrations [%] as obtained by XRF.

Oxygen

47.7

Silicon

30.0

Aluminum 9.75

Sodium

6.1

Calcium

3.66

Magnesium 0.456

Iron

1.35

Potassium

0.271

Phosphorus 0.114

Chlorine

0.0445

Titanium

0.252

Manganese 0.0173

Cobalt

0.0182

Nickel

0.0142

Strontium

0.0595

Zirconium

0.0143

Barium

0.0258

Wolfram

0.101

The results for combined XRD-XRF analysis with

EVA are shown in Fig. 3 and Tab. 3. The high Na

vs. Ca concentrations confirm the presence of Na-

plagioclase as found by XRD (diopside accounts

for about 60% of the total Ca, as calculated

by EVA). The present Na-plagioclase is most

successfully modelled using two albite phases

with different Ca amounts. Note the excellent

agreement found between the calculated and

observed element concentrations, which is better

than 1% for all elements, and therefore confirms

the correctness of the XRD phase identification

results for all phases.

The accuracy of the RIR method is limited by

several factors such as preferred orientation

effects and the quality of the ICDD PDF data used

(e.g. quality of relative intensities, I/Icor values,

idealized chemical formula).

Tab. 3: EVA semi-quantitative phase analysis

results based on combined XRD-XRF using

reference intensities as given in the ICDD PDF

patterns.

SS-VVV-PPPP

Compound Name

Phase

amounts

00-009-0466 (*)

Albite

58.2%

00-041-1480 (I)

Albite, calcian

15.4%

03-065-0466 (C) Quartz low, syn

14.0%

01-087-0700 (C) Diopside, syn

9.9%

01-089-5402 (C) Muscovite 2M1

2.6%

The most accurate quantitative results will be

obtained from a TOPAS Rietveld refinement. The

combined XRD-XRF results obtained are of high

value for defining the refinement model.

Page 4

BRUKER AXS, INC.

5465 EAST ChERYL pARKwAY

MADISON, wI 53711-5373

USA

TEL. (+1) (800) 234-XRAY

TEL. (+1) (608) 276-3000

FAX (+1) (608) 276-3006

EMAIL info@bruker-axs.com

www.bruker-axs.com

All configurations and specifications are subject to change without notice. Order No. L88-E00058. © 2006 BRUKER AXS GmbH. Printed in Germany.

BRUKER AXS GMBh

OESTLIChE RhEINBRUECKENSTR. 49

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3) Quantitative TOPAS refinement

Quantitative Rietveld analysis has been

performed using TOPAS, the results are shown

in Fig. 4 and Tab. 4. For the final refinement

two Na-plagioclases with different compositions

have been used to model the data to take the

elemental analysis results into account: Albite (0%

Ca) and Oligoclase (25% Ca).

From the results in Tab. 4 the following

conclusions can be drawn:

1. The sample can be unambiguously classified as

a quartzdiorite according to Streckeisen, see Fig. 5.

2. Combined XRD-XRF analysis and TOPAS

Rietveld refinement can allow a distinction of even

neighboring plagioclase solid solution members

(here albite and oligoclase) if present in sufficient

amounts.

The present sample can be characterised as

a rock with insignificant acid producing or

neutralisation potential. Remarkable is the easy

and reliable determination of the plagioclase type

for estimation of the neutralisation potential. This

ability is of particular interest, as anorthite has

an about 14x higher neutralisation potential than

albite (e.g. Jambor et al., 2002).

Fig. 4: Quantitative TOPAS refinement results.

Tab. 4: Quantitative TOPAS refinement results.

Compound Name

Phase amounts

Albite

49.6%

Oligoclase

30.5%

Quartz

9.9%

Diopside

8.8%

Muscovite

1.2%

Fig. 5: Streckeisen diagram for intrusive rocks.

Q: quartz, A: alkali-feldspar, P: plagioclase.

Reference

J.L. Jambor, J.E. Dutrizac, L.A. Groat, M. Raudsepp.

Environmental Geology (2002) 43, 1-17.

Q

A

P

granite

grano-

diorite

quartz-rich

granodiorite

quartz-

syenite

quartz-

monzonite

quartz-

monzo-

diorite

quartz-

diorite

tonalite

XRD- provides most direct analytical methol for determining presence and absolute amounts of minerals species in sample. XRD can also identify phases

XRF- provides direct information about chemical composition but cannot deliver direct phase information. Mass-balance calculations can be deducted but may lead to useless results in the presence of a polymorph.

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14y ago
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11y ago

Here is the main difference between "working principle" of XRF and XRD :

XRF : the photons are separated by diffraction on a single crystal -called monochromator- before being detected.

XRD : the photons directly goes through the sample and than being detected.

Also the detectors are different. There are four common types of detectors used in XRF : gas flow proportional counters, sealed gas detectors, scintillation counters and semiconductor detectors. In XRD, the detectors are based on silicon semiconductors.

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Influence of grain size on following properties of meatals:- Hardness Strength Impactness Toughness Creep Fatigue Ductility Malleability Durability Brittleness INTRODUCTION Yttria-stabilized tetragonal zirconia polycrystals (Y-TZP) have proved to be important structural ceramics. High strength and fracture toughness make them attractive candidates for a number of demanding applications. It was established that these advantageous properties are strongly influenced by the ceramic microstructure [1]. The relationships between microstructure and mechanical properties in Y-TZP ceramics have been studied extensively over the past two decades. It is now generally agreed that the transformation toughening effect (stress-induced tetragonal to monoclinic phase transformation) in Y-TZP ceramics is grain size dependent [2 7]. The larger the tetragonal grains the greater propensity to undergo stress-induced transformation to an equilibrium structure, resulting in an enhanced toughness. The maximum toughness lies near the critical grain size, where the tetragonal grains undergo spontaneous tetragonal to monoclinic transformation [7]. It was found that this critical grain size depends on the yttria content [6, 7]. However, the critical grain size, cited for 3Y-TZP (3 mol% Y2O3), which is the most common zirconia ceramic material, varies significantly (from 1 to 6 µm) [3, 8-9]. This could be attributed to different processing procedures that result in different ceramic microstructures. Thus, microstructural parameters like porosity, grain size distribution, yttrium distribution in grains, purity, phase assemblage, etc. need to be taken into account for evaluating the microstructure. In contrast to the fracture toughness the strength of 3Y-TZP reaches its maximum usually at smaller grain size [5, 10]. Increasing size of failure origin coupled with microstructural coarsening was identified as the reason for strength decrease in ceramics with large grains [11]. However, the increase of strength with decreasing grain size cannot be extended to the nanocrystalline range in 3Y-TZP. Eichler et al. [10] determined the strength maximum for 3Y-TZP in the submicron range and noted a clear strength decrease in the nanocrystalline grain size range (~100 nm). In this case, the strength decrease was attributed to the grain size dependence of fracture toughness. A decrease in the fracture toughness was observed as the grain size changed from the submicrometre to the nanometre range [10, 12]. These results validate the assumption that the increase of critical defects during microstructural coarsening is connected with the formation of stress induced transformed regions at the free surface and takes place preferentially in ceramics with grains near the critical size [11]. Nevertheless, special processing of TZP ceramics has been reported, which can partially eliminate the increase of critical defects during coarsening, resulting in almost constant strength, independent of grain size [8, 9]. Original papers Ceramics − Silikáty 52 (3) 165-171 (2008) 165 EFFECT OF GRAIN SIZE ON MECHANICAL PROPERTIES OF 3Y-TZP CERAMICS MARTIN TRUNEC Department of Ceramics and Polymers, Brno University of Technology Technicka 2896/2, 616 69 Brno, Czech Republic E-mail: trunec@fme.vutbr.cz Submitted June 21, accepted September 4, 2008 Keywords: Zirconia, Nanoceramics, Transformation toughening, Microstructure, Mechanical properties The dependence of mechanical properties of 3Y-TZP ceramics on their grain sizes in the range from 0.19 µm to 2.15 µm has been investigated. Vickers indentation tests were used to determine hardness and fracture toughness. The hardness decreased with increasing grain size. The fracture toughness was almost constant for ceramics with the grain size up to 0.40 µm and then grew with increasing grain size up to 7.8 MPam0.5 for ceramics with grain size of 1.8 µm. Above this grain size a spontaneous transformation from tetragonal to monoclinic phase occurred. Ceramic samples with grain sizes of 0.30 µm and 0.78 µm yielded similar bending strength, 1020 and 1011 MPa, respectively. The microstructural coarsening required for achieving larger grain size resulted in a higher scatter of strength values, which was demonstrated by a lower Weibull modulus (13.0 vs. 7.54). The mechanical properties of nanocrystalline 3Y-zirconia ceramics coarsened to the grain size range from 0.085 to 0.70 µm were also investigated and compared. Differences in mechanical behaviour of investigated ceramics were observed and their possible causes discussed. The objective of the present investigation was to describe the dependence of mechanical properties of commercial submicrometre-grained 3Y-TZP ceramics on grain size and to compare their mechanical properties to the mechanical properties of nanocrystalline zirconia ceramics and nanocrystalline ceramics coarsened to the submicrometre range. EXPERIMENTAL Two zirconia powders stabilized by 3 mol% Y2O3 were used for the preparation of test specimens. Commercial zirconia powder TZ-3YB (Tosoh, Japan) was cold isostatically pressed at 300 MPa into disk-shaped bodies (diameter 28 mm; thickness 5 mm). For comparison, a nanocrystalline zirconia powder B261 (BUT, Czech Republic) was used. Details of the preparation of the nanopowder can be found in [13]. Nanocrystalline powder was cold isostatically pressed at 1000 MPa without additives. The pressed bodies were 18 mm in diameter and 5 mm thick. These bodies were ground to a thickness of 1.5 mm prior to sintering. Both types of bodies were densified by pressureless sintering in air at temperatures from 1100 to 1650°C and dwell times ranging from 0 to 50 hours. The density of sintered specimens was determined by the Archimedes method [14] with distilled water as the immersing medium. The relative density of all ceramic bodies was calculated using the value 6.1 g·cm-3 for the theoretical density of 3Y-TZP. The grain size of the sintered ceramics was evaluated by linear intercept method (without correction) on scanning electron microscopy (SEM) micrographs of polished and thermally etched samples, in a similar way as in [15]. At least three micrographs and total of 300 intersects were evaluated to determine the average grain size for each sintering batch. The phase composition of the sintered ceramics was determined by X-ray diffraction (XRD) analysis (X´pert, Philips, the Netherlands). The X-ray spectra of polished and fracture surface were obtained and the phase content was quantified using Rietveld analysis. For hardness and fracture toughness evaluation Vickers indentation tests (LV 700, Leco, USA) were used. Prior to indentation ceramic disks were mounted in a resin and their surfaces ground and polished (finishing with 1 µm diamond polishing fluid). Hardness tests were performed at a load of 9.8 N (1 kg) and a hold of 15 s. For determining the Vickers hardness, HV (MPa), the following expression was used: HV = 1.8544 P/d 2, (1) where P is the applied load and d is the average diagonal line length of the indentation. Ten indentations were made for each sample. Toughness was calculated directly from the crack lengths produced by Vickers indentation at higher loads. Applied loads were 49.05 N (5 kg), 98.1 N (10 kg), 196.2 N (20 kg) and 294.3 N (30 kg) always with a hold of 15 s. The crack lengths were measured immediately after indentation using a calibrated optical microscope. The fracture toughness, KIc (MPam0.5), was calculated using the equation given by Niihara et al. [16] for Palmqvist cracks: KIc = 9.052 × 10-3 H3/5 E2/5 d c-1/2 , (2) where H is the hardness, E the Young modulus (a value of 210 GPa has been assumed for all the samples), d is the average diagonal line length of the indentation and c is the length of the Palmqvist crack. Ten valid measurements were determined for each sample. The valid measurements had to satisfy the requirements of the JIS R 1607 [17] on acceptable indentation cracks. The flexural strength was determined for selected ceramic samples in four-point bending at a crosshead speed of 2 mm/min, using fully articulated fixture with a 10 mm inner and 20 mm outer span (in the "A" arrangement according to the EN 843-1 [18]). Ceramic bars with dimensions ca. 2.5 × 2 × 25 mm3 were cut from the disks, ground and polished (finally with 1-2 µm grained diamond paste). The parameters of the Weibull strength distribution were calculated numerically, in compliance with the ENV 843-5 [19]. RESULTS AND DISCUSSION Microstructure and phase analysis Various sintering schedules were applied to zirconia green bodies to obtain dense sintered ceramics with different grain sizes. Only those sintering schedules that resulted in sintered densities exceeding 99% of theoretical density (% t.d.) were employed. A temperature of 1400°C was the lowest temperature used in sintering the TZ-3YB ceramics; this was necessary to obtain a dense sintered body. Larger grains were obtained by the action of both higher sintering temperatures and longer sintering times. Sintering schedules and resulting densities and grain sizes are shown in Table 1. The density of sintered TZ-3YB bodies was constant up to the sintering temperature of 1650°C. At the sintering temperature of 1650°C the density of TZ-3YB ceramics decreased with increasing sintering time. The structure of ceramics remained dense but the theoretical density of these ceramics decreased due to spontaneous transformation of the tetragonal into the monoclinic phase (see Table 1). The average grain size of TZ-3YB ceramics ranged from 0.19 µm (sintered at 1400°C/2 h) to 2.15 µm (sintered at 1650°C/50 h). The Trunec M. 166 Ceramics − Silikáty 52 (3) 165-171 (2008) critical grain size for spontaneous transformation from tetragonal to monoclinic phase lies between 1.8 and 2.15 µm, where the content of monoclinic phase in TZ 3YB ceramics increased dramatically. The sample sintered at 1650°C for 50 hours consisted of 77 % monoclinic phase and was severely cracked due to volume changes accompanying t→m transformation. Mechanical properties could not be determined for these ceramics. Several authors [8, 9, 11] have found large cubic grains in thermally treated 3Y-TZP samples. In our case no exaggerated grain growth was observed during the microstructural coarsening. The zirconia nanopowder B261 could be sintered to dense bulk ceramics already at the temperature of 1100°C and dwell time of 4 hours. The microstructure remained nanoscaled with an average grain size of 85 nm. Microstructural coarsening occurred at higher sintering temperatures. However, the grain growth kinetics of B261 ceramics was different from that in TZ 3YB ceramics. B261 ceramics sintered at 1550°C/5 h had larger grains than TZ 3YB ceramics sintered under the same conditions (0.70 vs. 0.48 µm). Moreover, the density of B261 ceramics decreased sharply already at small grain sizes where no monoclinic phase was detected. Figure 1 shows the density as a function of grain size for both TZ-3YB and B261 ceramics. The reason for the density change in B261 ceramics is not completely clear. According to the equilibrium phase diagram given by Scott [20] the maximum amount of cubic phase occurring in 3 mol% Y2O3-ZrO2 ceramics sintered at 1550°C can be about 28 %. Matsui et al. [21] showed that in tetragonal zirconia ceramics similar to TZ-3YB the Y3+ ions segregated at grain boundaries over a width of ~10 nm. Consequently, the cubic phase started to form from grain boundaries and a triple junction, at which Y3+ ions were segregated. A mixed tetragonal- cubic structure was confirmed in TZ-3YB ceramics by XRD analysis. In B261 ceramics the nanocrystalline structure probably allowed other mechanisms of phase structure development to take place that resulted in the one-phase tetragonal structure. This fact could explain the faster grain growth found in B261 ceramics. Typical microstructures of TZ-3YB ceramics are shown in Figures 2-4 and microstructures of B261 ceramics are shown in Figures 5 and 6. The holes and voids visible in micrographs on Figures 4 and 6 are believed not to be pores but rather to result from pulling out the grains during grinding and polishing. Effect of grain size on mechanical properties of 3Y-TZP ceramics Ceramics − Silikáty 52 (3) 165-171 (2008) 167 Table 1. Sintering schedules of zirconia ceramics and resulting density, grain size and monoclinic phase content. Sintering schedule Density Relative density Grain size m - ZrO2 Powder/Sample (°C)/(h) (g/cm3) (% t.d.) (µm) (%) TZ - 3YB 1400/2 6.07 99.5 0.19 0 TZ - 3YB 1500/2 6.08 99.7 0.30 0 TZ - 3YB 1550/0 6.09 99.8 0.29 0 TZ - 3YB 1550/2 6.09 99.8 0.40 0 TZ - 3YB 1550/5 6.09 99.8 0.48 0 TZ - 3YB 1550/10 6.09 99.8 0.54 0 TZ - 3YB 1600/2 6.09 99.8 0.53 0 TZ - 3YB 1600/5 6.09 99.8 0.68 0 TZ - 3YB 1600/10 6.08 99.7 0.78 0 TZ - 3YB 1650/10 6.08 99.6 0.99 3 TZ - 3YB 1650/20 6.08 99.6 1.37 6 TZ - 3YB 1650/30 6.04 99.1 1.79 13 TZ - 3YB 1650/50 5.68 93.1 2.15 77 B 261 1100/4 6.07 99.4 0.085 0 B 261 1300/6 6.04 99.0 0.19 0 B 261 1450/2 5.93 97.3 0.33 0 B 261 1550/5 5.71 93.6 0.70 0 Figure 1. Density of TZ-3YB and B261 ceramics as a function of grain size. Grain size (µm) Density (g cm-3) 5.9 5.7 0.0 6.1 0.4 1.6 2.0 6.0 5.8 6.2 1.2 0.8 TZ-3YB B261 Mechanical properties Ten Vickers hardness tests were performed for each ceramic. Average hardness values and their standard deviation are given in Table 2. The hardness of TZ-3YB ceramics clearly decreased with increasing grain size from HV = 12620 MPa at grain size of 0.19 µm to HV = 10971 MPa at grain size of 1.79 µm. The graph in Figure 7 shows the hardness of TZ-3YB ceramics as a function of the inverse square root of grain size. The values in the graph could be reasonably fitted with a line (r2 = 0.94), which means that this dependence followed the Hall-Petch relationship. The hardness of B261 ceramics showed a higher dispersion but the linear fit seems to be also reasonable. Different parameters of the fits (lower hardness of B261 compared with TZ-3YB ceramics) could be attributed to different phase structure (mixed tetragonal-cubic vs. pure tetragonal). Trunec M. 168 Ceramics − Silikáty 52 (3) 165-171 (2008) Figure 2. SEM micrograph showing the microstructure of the TZ-3YB ceramics sintered at 1400°C for 2 h. Figure 3. SEM micrograph showing the microstructure of the TZ-3YB ceramics sintered at 1650°C for 20 h. 1 µm 5 µm Figure 4. SEM micrograph showing the microstructure of the TZ-3YB ceramics sintered at 1650°C for 50 h. Figure 5. SEM micrograph showing the microstructure of the B261 ceramics sintered at 1100°C for 4 h. 5 µm 500 nm Figure 6. SEM micrograph showing the microstructure of the B261 ceramics sintered at 1550°C for 5 h. 2 µm Different loads of Vickers indenter in the range from 49.05 N (5 kg) to 294.3 N (30 kg) were used to generate cracks in ceramic samples. It was verified that in all cases only Palmqvist cracks were produced. Fracture toughness values calculated from crack lengths using Equation (2) at different loads are shown in Table 2. The indenter load of 49.05 N (5 kg) generated unstable cracks that grew further after load release. It was not possible to measure the crack length reliably, therefore the fracture toughness calculated from this load was not included in the Table 2. The graph in Figure 8 shows the dependence of fracture toughness of TZ-3YB ceramics at different loads on grain size. The values of fracture toughness determined at different loads varied significantly. Nevertheless, the dependence of toughness on grain size showed the same trend for all loads. To obtain the most reliable value for the fracture toughness, an average of values determined at different loads was calculated (see Table 2). Figure 9 gives the dependence of the average fracture toughness on grain size for both TZ-3YB and B261 ceramics. This dependence can be divided in two areas. The toughness was almost constant (~ 5.1 MPam0.5) up to a grain size of 0.4 µm. In ceramics with larger grains, the toughness increased linearly up to the grain size of 1.8 µm, where the maximum toughness (7.8 MPam0.5) was found. Above this grain size spontaneous transformation to the monoclinic phase occurred. Figure 9 shows that both ceramics, TZ-3YB and B261, followed the same toughness dependence on grain size. It also follows from this figure that the transformation toughness effect is grain size dependent only above a particular tetragonal grain size (approx. 0.4 µm). Effect of grain size on mechanical properties of 3Y-TZP ceramics Ceramics − Silikáty 52 (3) 165-171 (2008) 169 Table 2. Hardness, HV, fracture toughness, KIc, and their standard deviations, s, of zirconia ceramics. Fracture toughness Sintering Hardness 10 kg 20 kg 30 kg Average schedule HV s KIc s KIc s KIc s KIc Sample (°C)/(h) (MPa) (MPam0.5) TZ - 3YB 1400/2 12620 186 4.94 0.07 5.29 0.06 5.49 0.05 5.24 TZ - 3YB 1500/2 12264 135 4.91 0.06 5.20 0.08 5.41 0.05 5.17 TZ - 3YB 1550/0 12137 224 4.89 0.29 5.10 0.06 5.38 0.05 5.12 TZ - 3YB 1550/2 12007 103 4.89 0.05 5.14 0.03 5.40 0.03 5.14 TZ - 3YB 1550/5 11970 113 5.06 0.07 5.23 0.05 5.45 0.06 5.25 TZ - 3YB 1550/10 11738 127 5.53 0.13 5.41 0.07 5.62 0.07 5.52 TZ - 3YB 1600/2 11858 363 5.15 0.16 5.29 0.07 5.57 0.04 5.34 TZ - 3YB 1600/5 11849 551 5.80 0.21 5.43 0.05 5.62 0.04 5.62 TZ - 3YB 1600/10 11588 176 6.39 0.09 5.53 0.03 5.72 0.03 5.88 TZ - 3YB 1650/10 11361 293 6.75 0.21 5.82 0.12 5.87 0.06 6.15 TZ - 3YB 1650/20 11145 341 7.11 0.12 6.52 0.10 6.09 0.06 6.57 TZ - 3YB 1650/30 10971 293 7.94 0.24 7.50 0.54 7.80 0.15 7.77 B 261 1100/4 12867 789 4.89 0.08 5.35 0.14 - - 5.12 B 261 1300/6 12485 218 4.79 0.07 5.15 0.12 5.38 0.08 5.11 B 261 1450/2 10587 657 4.73 0.09 5.30 0.27 - - 5.02 B 261 1550/5 10080 435 5.98 0.45 5.79 0.21 5.99 0.40 5.92 Figure 7. The dependence of the hardness of TZ-3YB and B261 ceramics on the inverse square root of grain size. d-1/2 (µm-1/2) Hardness (MPa) 11 000 10 000 0.4 12 000 0.8 2.0 2.4 11 500 10 500 12 500 1.6 1.2 13 000 2.8 3.2 3.6 TZ-3YB B261 Figure 8. Fracture toughness of TZ-3YB ceramics as a function of grain size determined at different indentation loads. Grain size (µm) Fracture toughness (MPa m0.5) 6 4 0.0 8 0.4 1.6 2.0 7 5 9 1.2 0.8 10 kg load 20 kg load 30 kg load Recently Vickers indentation fracture toughness tests (VIF) were reviewed in detail [22]. It was concluded that VIF techniques are not suitable for reliable measurement of fracture toughness, KIc, because the crack arrest process occurs in a multiple-crack environment and in highly complex residual stress conditions. To verify our fracture toughness results determined by the indentation method, two standardized methods were applied. Unfortunately, the results obtained by "Chevron V Notch" method (CVN) and "Single Edged V Notch Beam" method (SEVNB) showed extremely high scatter (5-12 MPam0.5), thus it was not possible to find any dependence on grain size. The reason for such high variance is not clear and may be connected with the toughening effect in TZP ceramics. From this point of view the indentation method utilized in the present investigation provided more consistent results compared with the CVN and SEVNB methods. The four-point bending strength of TZ-3YB bars with a grain size of 0.30 µm (sintered at 1500°C/2 h) and 0.78 µm (sintered at 1600°C/10 h) was determined and compared. Figure 10 shows the Weibull plot of both materials. Although the average strength of samples varying in grain size was similar (1020 MPa vs. 1011 MPa), it can be seen in the graph that the scatter of strength values was higher for TZ-3YB ceramics with larger grains. This observation was confirmed by calculation of Weibull moduli. The Weibull modulus was m = 13.0 for ceramics with the grain size of 0.30 µm and m = 7.54 for ceramics with the grain size of 0.78 µm. It was verified statistically that these values are significantly different. According to the linear fracture mechanics the body with higher fracture toughness should possess the higher strength. In our case TZ-3YB ceramics with a grain size of 0.78 µm had higher toughness than ceramics with a grain size of 0.30 µm (5.88 vs. 5.17 MPam0.5). Unfortunately, the effect of higher toughness was suppressed by an effect of bigger critical defects due to microstructural coarsening [10]. The competition of these two effects resulted in ceramics with strengths apparently independent of grain size. However, the size and distribution of defects during coarsening cannot be efficiently controlled, which resulted in the lower Weibull modulus for ceramics sintered at higher temperature. CONCLUSION The effect of grain size on mechanical properties of commercial submicrometre-grained 3Y-TZP ceramics (TZ-3YB) and nanocrystalline 3Y-zirconia ceramics (B261) was investigated. The following conclusions could be drawn: 1.The hardness of both TZ-3YB and B261 ceramics decreased with increasing grain size. However, the hardness was lower in coarsened nanoceramics. This could be attributed to different mechanisms of the development of phase structure in nanoceramics compared with submicrometre-grained ceramics. 2.The fracture toughness was almost constant (5.1 MPam0.5) up to the grain size of 0.4 µm. Above this grain size, the fracture toughness started to grow and reached the maximum of 7.8 MPam0.5 at the grain size of 1.8 µm. Further grain growth resulted in spontaneous transformation from tetragonal to monoclinic phase and damage of the samples due to cracking. Both ceramics followed the same grain size depen-dence of fracture toughness. 3.The four-point bending strength of TZ-3YB ceramics with grain size of 0.30 and 0.78 µm was similar, 1020 MPa and 1011 MPa, respectively. The higher Trunec M. 170 Ceramics − Silikáty 52 (3) 165-171 (2008) Figure 9. Average fracture toughness of TZ-3YB and B261 ceramics as a function of grain size. Grain size (µm) Fracture toughness (MPa m0.5) 6 4 0.0 8 0.4 1.6 2.0 7 5 9 1.2 0.8 TZ-3YB B261 Figure 10. Weibull plot of the bending strength data for TZ-3YB ceramics sintered at 1500°C for 2 h and at 1600°C for 10 h. ln (bending strength, MPa) ln{ln[1/(1-P)]} -3 -5 6.6 -1 6.7 7.0 7.1 -2 -4 0 6.9 6.8 TZ-3YB - 1500°C/2 h TZ-3YB - 1600°C/10 h 1 2 7.2 fracture toughness inherent to ceramics with larger grain size was counterbalanced with an increase of critical defects due to microstructural coarsening. Moreover, the Weibull modulus declined from m = 13 at a grain size of 0.30 µm to m = 7.54 at a grain size of 0.78 µm. Acknowledgement The author gratefully acknowledges the funding provided by the Czech Ministry of Education under grant MSM 0021630508. Dr. A. Buchal and Mrs. D. Janova are kindly acknowledged for providing XRD analyses and SEM images, respectively. The author wishes to thank Mrs. Z. Skalova for her help with the experimental work. References 1. Hannink R. H. J., Kelly P. M., Muddle B. C.: J.Am.Ceram. Soc. 83, 461 (2000). 2. Lange F. F.: J. Mater.Sci. 17, 225 (1982). 3. Lange F. F.: J.Mater.Sci. 17, 240 (1982). 4. Becher P. F., Swain M. V.: J.Am.Ceram.Soc. 75, 493 (1992). 5. Wang J, Rainforth M., Stevens R.: Br.Ceram.Trans.J. 88, 1 (1989). 6. Suresh A., Mayo M. J., Porter W. D., Rawn C. J.: J.Am. Ceram.Soc. 86, 360 (2003). 7. Bravo-Leon A., Morikawa Y., Kawahara M., Mayo M. J.: Acta Mater. 50, 4555 (2002). 8. Ruiz L., Readey M. J.: J.Am.Ceram.Soc. 79, 2331 (1996). 9. Casellas D., Feder A., Llanes L., Anglada M.: Scr.Mater. 45, 213 (2001). 10. Eichler J., Rödel J., Eisele U., Hoffman M.: J.Am.Ceram. Soc. 90, 2830 (2007). 11. Casellas D., Alcala J., Llanes L., Anglada M.: J.Mater.Sci. 36, 3011 (2001). 12. Cottom B. A., Mayo M. J.: Scr.Mater. 34, 809 (1996). 13. Trunec M., Maca K.: J.Am.Ceram.Soc. 90, 2735 (2007). 14. EN 623-2: Advanced Technical Ceramics - Monolithic Ceramics. General and Texture Properties. Part 2: Determination of Density and Porosity, CEN, Brussels 1993. 15. Maca K., Trunec M., Chmelik R.: Ceramics-Silikaty 51, 94 (2007). 16. Niihara K., Morena R., Hasselman D. P. H.: J.Mater.Sci. Lett. 1, 13 (1982). 17. JIS R 1607: Testing Methods for Fracture Toughness of High Performance Ceramics, Japanese Standards Association, Tokyo 1990. 18. EN 843-1: Advanced Technical Ceramics - Monolithic Ceramics. Mechanical Properties at Room Temperature. Part 1: Determination of Flexural Strength, CEN, Brussels 1995. 19. ENV 843-5: Advanced Technical Ceramics - Monolithic Ceramics. Mechanical Properties at Room Temperature. Part 5: Statistical Analysis, CEN, Brussels 1996. 20. Scott H. G.: J.Mater.Sci. 10, 1527 (1975). 21. Matsui K., Horikoshi H., Ohmichi N., Ohgai M.: J.Am. Ceram.Soc. 86, 1401 (2003). 22. Quinn G. D., Bradt R. C.: J.Am.Ceram.Soc. 90, 673 (2007). Effect of grain size on mechanical properties of 3Y-TZP ceramics Ceramics − Silikáty 52 (3) 165-171 (2008) 171 VLIV VELIKOSTI ZRN NA MECHANICKÉ VLASTNOSTI 3Y-TZP KERAMIKY MARTIN TRUNEC Odbor keramiky a polymerù, Vysoké uèení technické v Brnì, Technická 2896/2, 616 69 Brno Mechanické vlastnosti 3Y-TZP keramiky byly zkoumány v závislosti na velikosti zrn v rozsahu od 0,19 µm do 2,15 µm. Vickersovy indentaèní testy byly použity pro stanovení tvrdosti a lomové houževnatosti. Tvrdost klesala s rostoucí velikostí zrn. Lomová houževnatost byla témìø konstantní pro keramiky se zrny do 0,4 µm a poté rostla se zvyšující se velikosti zrn až na 7,8 MPam0,5 u keramiky se zrny o velikosti 1,8 µm. U vìtších zrn došlo ke spontánní transformaci tetragonální fáze na monoklinickou. Keramické vzorky s velikostí zrn 0,30 µm a 0,78 µm mìli podobnou pevnost v ohybu, 1020 a 1011 MPa. Mikrostrukturní zhrubnutí, které bylo nezbytné pro dosažení vìtších zrn, vedlo k vyššímu rozptylu pevností, což se projevilo snížením Weibullova modulu (13,0 vs. 7,54). Pro srovnání byly také zkoumány mechanické vlastnosti nanokrystalické 3Y-ZrO2 keramiky, jejíž zrna byla zhrublá na velikost od 0,085 do 0,70 µm. Byly zjištìny rozdíly v mechanických vlastnostech zkoumaných keramik. Možné pøíèiny tìchto rozdílù byly diskutovány.

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