Magnetic Behavior of Twin Roller Melt Spun Cu Co Alloys
Magnetoresistive Cu 90 Co 10 alloys have been produced by twin roller melt spinning at tangential wheel speeds between 10 m/s and 30 m/s to obtain different solute and Co-rich precipitate distributions. X-ray diffraction indicates that the ribbons are polycrystalline with a fcc Cu(Co) (200) textured...
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Veröffentlicht in: | IEEE transactions on magnetics 2013-08, Vol.49 (8), p.4518-4521 |
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creator | Nunez Coavas, Henry Pozo Lopez, Gabriela Fabietti, Luis M. Condo, Adriana M. Urreta, Silvia E. |
description | Magnetoresistive Cu 90 Co 10 alloys have been produced by twin roller melt spinning at tangential wheel speeds between 10 m/s and 30 m/s to obtain different solute and Co-rich precipitate distributions. X-ray diffraction indicates that the ribbons are polycrystalline with a fcc Cu(Co) (200) textured matrix; no evidence of a spinodal-like composition modulation could be detected with this technique. Transmission electron microscopy observations performed in samples quenched at 10 m/s indicate the existence of small, coherent, Co-rich precipitates of mean size of about 11 nm and bigger (~40 nm) Co-oxide particles. The small coherent precipitates form colonies inside the grains, mediated by precipitate free zones. Samples quenched at 30 m/s are single magnetic phase (superparamagnetic), but the hysteresis loops of the other as cast ribbons are well fitted by a superparamagnetic contribution and a ferromagnetic one, the latter arising from the Co-rich precipitates. Room temperature coercivities, of about 30-50 mT, are lower than those predicted for a mechanism of coherent rotation in the ensemble of non-interacting, Co-rich precipitates. |
doi_str_mv | 10.1109/TMAG.2013.2259618 |
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X-ray diffraction indicates that the ribbons are polycrystalline with a fcc Cu(Co) (200) textured matrix; no evidence of a spinodal-like composition modulation could be detected with this technique. Transmission electron microscopy observations performed in samples quenched at 10 m/s indicate the existence of small, coherent, Co-rich precipitates of mean size of about 11 nm and bigger (~40 nm) Co-oxide particles. The small coherent precipitates form colonies inside the grains, mediated by precipitate free zones. Samples quenched at 30 m/s are single magnetic phase (superparamagnetic), but the hysteresis loops of the other as cast ribbons are well fitted by a superparamagnetic contribution and a ferromagnetic one, the latter arising from the Co-rich precipitates. Room temperature coercivities, of about 30-50 mT, are lower than those predicted for a mechanism of coherent rotation in the ensemble of non-interacting, Co-rich precipitates.</description><identifier>ISSN: 0018-9464</identifier><identifier>EISSN: 1941-0069</identifier><identifier>DOI: 10.1109/TMAG.2013.2259618</identifier><identifier>CODEN: IEMGAQ</identifier><language>eng</language><publisher>New York: IEEE</publisher><subject>Magnetic hysteresis ; Magnetic properties ; Magnetism ; Materials science ; melt spinning ; Metals ; Microstructure ; precipitation ; Spinning ; spinodal decomposition ; Temperature distribution ; Temperature measurement ; X-ray scattering</subject><ispartof>IEEE transactions on magnetics, 2013-08, Vol.49 (8), p.4518-4521</ispartof><rights>Copyright The Institute of Electrical and Electronics Engineers, Inc. (IEEE) Aug 2013</rights><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c903-82023a80df7ad2611c0d279e9be76be5c9674ad99d57dfe47331e7366a09803</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://ieeexplore.ieee.org/document/6566106$$EHTML$$P50$$Gieee$$H</linktohtml><link.rule.ids>314,780,784,796,27924,27925,54758</link.rule.ids><linktorsrc>$$Uhttps://ieeexplore.ieee.org/document/6566106$$EView_record_in_IEEE$$FView_record_in_$$GIEEE</linktorsrc></links><search><creatorcontrib>Nunez Coavas, Henry</creatorcontrib><creatorcontrib>Pozo Lopez, Gabriela</creatorcontrib><creatorcontrib>Fabietti, Luis M.</creatorcontrib><creatorcontrib>Condo, Adriana M.</creatorcontrib><creatorcontrib>Urreta, Silvia E.</creatorcontrib><title>Magnetic Behavior of Twin Roller Melt Spun Cu Co Alloys</title><title>IEEE transactions on magnetics</title><addtitle>TMAG</addtitle><description>Magnetoresistive Cu 90 Co 10 alloys have been produced by twin roller melt spinning at tangential wheel speeds between 10 m/s and 30 m/s to obtain different solute and Co-rich precipitate distributions. X-ray diffraction indicates that the ribbons are polycrystalline with a fcc Cu(Co) (200) textured matrix; no evidence of a spinodal-like composition modulation could be detected with this technique. Transmission electron microscopy observations performed in samples quenched at 10 m/s indicate the existence of small, coherent, Co-rich precipitates of mean size of about 11 nm and bigger (~40 nm) Co-oxide particles. The small coherent precipitates form colonies inside the grains, mediated by precipitate free zones. Samples quenched at 30 m/s are single magnetic phase (superparamagnetic), but the hysteresis loops of the other as cast ribbons are well fitted by a superparamagnetic contribution and a ferromagnetic one, the latter arising from the Co-rich precipitates. Room temperature coercivities, of about 30-50 mT, are lower than those predicted for a mechanism of coherent rotation in the ensemble of non-interacting, Co-rich precipitates.</description><subject>Magnetic hysteresis</subject><subject>Magnetic properties</subject><subject>Magnetism</subject><subject>Materials science</subject><subject>melt spinning</subject><subject>Metals</subject><subject>Microstructure</subject><subject>precipitation</subject><subject>Spinning</subject><subject>spinodal decomposition</subject><subject>Temperature distribution</subject><subject>Temperature measurement</subject><subject>X-ray scattering</subject><issn>0018-9464</issn><issn>1941-0069</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><sourceid>RIE</sourceid><recordid>eNo9kFFLwzAUhYMoOKc_QHwJ-Nx5b5ImzeMsOoUNYe49ZO2tdtRmpquyf2_Hhk-XA985Fz7GbhEmiGAfVovpbCIA5USI1GrMztgIrcIEQNtzNgLALLFKq0t21XWbIaoUYcTMwn-0tKsL_kif_qcOkYeKr37rli9D01DkC2p2_H3btzzveR74tGnCvrtmF5VvOro53TFbPj-t8pdk_jZ7zafzpLAgk0yAkD6DsjK-FBqxgFIYS3ZNRq8pLaw2ypfWlqkpK1JGSiQjtfZgM5Bjdn8c3cbw3VO3c5vQx3b451ChVKCFlAOFR6qIoesiVW4b6y8f9w7BHeS4gxx3kONOcobO3bFTE9E_r1OtEbT8A6hPXWc</recordid><startdate>201308</startdate><enddate>201308</enddate><creator>Nunez Coavas, Henry</creator><creator>Pozo Lopez, Gabriela</creator><creator>Fabietti, Luis M.</creator><creator>Condo, Adriana M.</creator><creator>Urreta, Silvia E.</creator><general>IEEE</general><general>The Institute of Electrical and Electronics Engineers, Inc. (IEEE)</general><scope>97E</scope><scope>RIA</scope><scope>RIE</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7SP</scope><scope>7U5</scope><scope>8BQ</scope><scope>8FD</scope><scope>JG9</scope><scope>L7M</scope></search><sort><creationdate>201308</creationdate><title>Magnetic Behavior of Twin Roller Melt Spun Cu Co Alloys</title><author>Nunez Coavas, Henry ; Pozo Lopez, Gabriela ; Fabietti, Luis M. ; Condo, Adriana M. ; Urreta, Silvia E.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c903-82023a80df7ad2611c0d279e9be76be5c9674ad99d57dfe47331e7366a09803</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Magnetic hysteresis</topic><topic>Magnetic properties</topic><topic>Magnetism</topic><topic>Materials science</topic><topic>melt spinning</topic><topic>Metals</topic><topic>Microstructure</topic><topic>precipitation</topic><topic>Spinning</topic><topic>spinodal decomposition</topic><topic>Temperature distribution</topic><topic>Temperature measurement</topic><topic>X-ray scattering</topic><toplevel>online_resources</toplevel><creatorcontrib>Nunez Coavas, Henry</creatorcontrib><creatorcontrib>Pozo Lopez, Gabriela</creatorcontrib><creatorcontrib>Fabietti, Luis M.</creatorcontrib><creatorcontrib>Condo, Adriana M.</creatorcontrib><creatorcontrib>Urreta, Silvia E.</creatorcontrib><collection>IEEE All-Society Periodicals Package (ASPP) 2005-present</collection><collection>IEEE All-Society Periodicals Package (ASPP) 1998-Present</collection><collection>IEEE Electronic Library (IEL)</collection><collection>CrossRef</collection><collection>Electronics & Communications Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>METADEX</collection><collection>Technology Research Database</collection><collection>Materials Research Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>IEEE transactions on magnetics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Nunez Coavas, Henry</au><au>Pozo Lopez, Gabriela</au><au>Fabietti, Luis M.</au><au>Condo, Adriana M.</au><au>Urreta, Silvia E.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Magnetic Behavior of Twin Roller Melt Spun Cu Co Alloys</atitle><jtitle>IEEE transactions on magnetics</jtitle><stitle>TMAG</stitle><date>2013-08</date><risdate>2013</risdate><volume>49</volume><issue>8</issue><spage>4518</spage><epage>4521</epage><pages>4518-4521</pages><issn>0018-9464</issn><eissn>1941-0069</eissn><coden>IEMGAQ</coden><abstract>Magnetoresistive Cu 90 Co 10 alloys have been produced by twin roller melt spinning at tangential wheel speeds between 10 m/s and 30 m/s to obtain different solute and Co-rich precipitate distributions. X-ray diffraction indicates that the ribbons are polycrystalline with a fcc Cu(Co) (200) textured matrix; no evidence of a spinodal-like composition modulation could be detected with this technique. Transmission electron microscopy observations performed in samples quenched at 10 m/s indicate the existence of small, coherent, Co-rich precipitates of mean size of about 11 nm and bigger (~40 nm) Co-oxide particles. The small coherent precipitates form colonies inside the grains, mediated by precipitate free zones. Samples quenched at 30 m/s are single magnetic phase (superparamagnetic), but the hysteresis loops of the other as cast ribbons are well fitted by a superparamagnetic contribution and a ferromagnetic one, the latter arising from the Co-rich precipitates. Room temperature coercivities, of about 30-50 mT, are lower than those predicted for a mechanism of coherent rotation in the ensemble of non-interacting, Co-rich precipitates.</abstract><cop>New York</cop><pub>IEEE</pub><doi>10.1109/TMAG.2013.2259618</doi><tpages>4</tpages></addata></record> |
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subjects | Magnetic hysteresis Magnetic properties Magnetism Materials science melt spinning Metals Microstructure precipitation Spinning spinodal decomposition Temperature distribution Temperature measurement X-ray scattering |
title | Magnetic Behavior of Twin Roller Melt Spun Cu Co Alloys |
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