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Ti-5.8Al-4.8Sn-2Zr-1Mo-0.35Si-0.70Nd合金中富釹稀土相研究
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Nd-rich Rare Earth Phases in Ti-5.8Al-4.8Sn-2Zr-1Mo-0.35Si-0.70Nd Alloy
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    摘要:

    針對Ti-5.8 Al-4.8 Sn-2 Zr-1 Mo-0.35 Si-0.70 Nd粉末冶金高溫鈦合金中富釹稀土相的形成、尺寸、分布、形態(tài)、長大及結(jié)構(gòu)特征進行了系統(tǒng)研究。結(jié)果表明:快速凝固態(tài)高溫鈦合金粉末中稀土相為液態(tài)析出相,其尺寸大部分在50~250 nm之間,彌散分布在基體中;晶內(nèi)稀土相多為球狀,晶界稀土相多為橢球狀,其長軸平行于晶界;TEM觀察到的稀土相的尺寸和分布與理論計算相符合;快速凝固高溫鈦合金粉末經(jīng)過700~1000 ℃/110 MPa/0.5 h熱等靜壓成形后,快速凝固過程中已析出的稀土相尺寸變化不大;同時細小的稀土相從過飽和的基體中大量固相析出;經(jīng)過1200 ℃/140 MPa/3 h 熱等靜壓成形后,稀土相顆粒尺寸大部分在150~500 nm之間,有明顯長大;稀土相的高分辨圖像及同心衍射環(huán)花樣表明,快速凝固高溫鈦合金粉末中的稀土相由5~10 nm的納米晶組成,經(jīng)過1200 ℃熱等靜壓成形處理后的稀土相仍由納米晶組成,而且納米晶的尺寸沒有明顯變化;但是稀土相的“基體”上明顯出現(xiàn)富Sn元素的“第二相”顆粒,結(jié)構(gòu)變得復(fù)雜。

    Abstract:

    The formation, morphology, size, distribution, growth and structure of Nd-rich rare earth (RE) phases in powder metallurgy (PM) high temperature titanium alloy were investigated. The results show that the RE-rich phases in as-rapidly-solidified high temperature titanium alloy powder precipitate in the process of powder droplet solidification, and the particle size is 50~250 nm in diameter. The majority of the particles are uniformly distributed in the alloy matrix. The particles are nearly spherical within the grains and ellipsoidal along the grain boundary. The major axes of the ellipsoidal particles are lying nearly parallel to the grain boundary. The calculated size and distribution of the second phase particles are in agreement with the TEM experimental results. The diameters of RE-rich phases are largely smaller than 50 nm precipitated from the supersaturated matrix after hot isostatic pressing (HIP) between 700 and 1000 oC in a short time. The size variation of the original RE-rich phases is minimal. However, the particle size including the original and the precipitated is 150~500 nm in diameter after HIP at 1200 oC for 3 h. The HRTEM image and SAED pattern of the RE-rich phases indicate that they are composed of many nanocrystallines while they are still composed of nanocrystallines whose size grows up minutely after HIP at high temperature. Maybe the later nanocrystalline is different from the former one because the tin-rich phases appear on the RE-rich phases “matrix”, resulting in the complex microstructure of the RE-rich phases.

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王曉軒. Ti-5.8Al-4.8Sn-2Zr-1Mo-0.35Si-0.70Nd合金中富釹稀土相研究[J].稀有金屬材料與工程,2015,44(1):243~246.[Wang Xiaoxuan. Nd-rich Rare Earth Phases in Ti-5.8Al-4.8Sn-2Zr-1Mo-0.35Si-0.70Nd Alloy[J]. Rare Metal Materials and Engineering,2015,44(1):243~246.]
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  • 收稿日期:2014-01-27
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  • 在線發(fā)布日期: 2015-05-22
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