26.08.2013 Views

Sinterizazio-atmosferaren eragina M graduko (ASP 30 ... - Euskara

Sinterizazio-atmosferaren eragina M graduko (ASP 30 ... - Euskara

Sinterizazio-atmosferaren eragina M graduko (ASP 30 ... - Euskara

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

Referring now to oversintering, it is observed in figure 4 that even for <strong>30</strong>°C oversintering in<br />

the gas atmosphere, for steels T42 and Px<strong>30</strong>, the total amount of primary particles remains<br />

constant. Taking into account also that the size of MX particles is nearly the same and that only a<br />

small increase in size for M6C is produced, a similar or slightly larger grain size is predicted, which<br />

is in agreement with experimental observation for gas sintering . For T42, an oversintering of 60°C<br />

produces a significant dissolution and growth of M6C carbides, but the MX carbonitrides remain<br />

and 3 .8% of 1µm MX carbonitrides predicts a limiting grain size of 35µm, in close agreement with<br />

the 40µm found experimentally . For oversintering in vacuum, for T42, as shown in figure 4 , 10 °C<br />

oversintering decreases the amount of primary carbides to around 6-8% which with a mean value of<br />

1 .5µm for the mean particle size, predicts values of limiting grain size of 26-33 µm, in close<br />

agreement with the 34 gm found experimentally . For <strong>30</strong>°C oversintering in vacuum for the same<br />

steel, volume fraction 2-6% of primary (non eutectic) carbides are found, predicting values of 33-<br />

100 µm, the observed values being 50-60 µm . For oversintered Px<strong>30</strong>, the Zener equation predicts<br />

smaller values than those observed experimentally . This could be due to the fact that, althought less<br />

M6C carbides are dissolved for the same amount of oversintering, as shown in figure 4 , the<br />

carbides observed are more clustered, which explains why they are less effective in preventing<br />

grain growth .<br />

CONCLUSIONS<br />

1 . Oversintering of several high speed steels in a gas atmosphere composed of N2-H2-CH4<br />

results in only small increases in grain sizes in contrast with the significant increases observed for<br />

vacuum sintering .<br />

2 . This difference in behaviour can be explained in terms of the Zener drag exerted by fine<br />

and stable carbonitirides present after gas sintering, which do not dissolve even at high<br />

temperatures .<br />

3. Significant levels of oversintering are therefore allowable, without impairing the<br />

mechanical properties of the sintered components produced in the gas atmosphere, this effect<br />

having important industrial relevance .<br />

REFERENCES<br />

1 . I . Urrutibeaskoa, R . Palma, V . Martínez, J . J . Urcola . Powder Metall, 1990, vol . 33, 4, <strong>30</strong>5-312 .<br />

2 . H . Fredriksson, M . Hillert, M . Nica . Scand . J . Metall, 1979, 8, 115-122 .<br />

3 . V . Martínez . Ph . D . Thesis, ESTI, San Sebastián, Basque Country, Spain, 1990 .<br />

4 . R. Palma . Ph . D . Thesis, ESII, San Sebastián, Basque Country, Spain, 1990 .<br />

5 . Swedish Standars Institution . Powder Metallurgy MNC Handbook 6E, 1978 .<br />

6 . R . L . Miller. Trans. ASM . 1964, pp 892 .

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!