Hydrogen storage properties of a Mg-Ni-Fe mixture prepared via planetary ball milling in a H2 atmosphere
A sample composition has been designed based on previously reported data. An 80 wt%Mg–13.33 wt%Ni–6.67 wt%Fe (referred to as Mg–13.33Ni–6.67Fe) sample exhibited higher hydriding and dehydriding rates after activation and a larger hydrogen storage capacity compared to those of other mixtures prepared...
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Veröffentlicht in: | International journal of hydrogen energy 2010-10, Vol.35 (19), p.10366-10372 |
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container_title | International journal of hydrogen energy |
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creator | MYOUNG YOUP SONG SUNG HWAN BAEK BOBET, Jean-Louis HONG, Seong-Hyeon |
description | A sample composition has been designed based on previously reported data. An 80 wt%Mg–13.33 wt%Ni–6.67 wt%Fe (referred to as Mg–13.33Ni–6.67Fe) sample exhibited higher hydriding and dehydriding rates after activation and a larger hydrogen storage capacity compared to those of other mixtures prepared under similar conditions. After activation (at n = 3), the sample absorbed 4.60 wt%H for 5 min and 5.61 wt%H for 60 min at 593 K under 12 bar H2. The sample desorbed 1.57 wt%H for 5 min and 3.92 wt%H for 30 min at 593 K under 1.0 bar H2. Rietveld analysis of the XRD pattern using FullProf program showed that the as-milled Mg–13.33Ni–6.67Fe sample contained Mg(OH)2 and MgH2 in addition to Mg, Ni, and Fe. The Mg(OH)2 phase is believed to be formed through the reaction of Mg or MgH2 with water vapor in the air. The dehydrided Mg–13.33Ni–6.67Fe sample after hydriding-dehydriding cycling contained Mg, Mg2Ni, MgO, and Fe. |
doi_str_mv | 10.1016/j.ijhydene.2010.07.161 |
format | Article |
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An 80 wt%Mg–13.33 wt%Ni–6.67 wt%Fe (referred to as Mg–13.33Ni–6.67Fe) sample exhibited higher hydriding and dehydriding rates after activation and a larger hydrogen storage capacity compared to those of other mixtures prepared under similar conditions. After activation (at n = 3), the sample absorbed 4.60 wt%H for 5 min and 5.61 wt%H for 60 min at 593 K under 12 bar H2. The sample desorbed 1.57 wt%H for 5 min and 3.92 wt%H for 30 min at 593 K under 1.0 bar H2. Rietveld analysis of the XRD pattern using FullProf program showed that the as-milled Mg–13.33Ni–6.67Fe sample contained Mg(OH)2 and MgH2 in addition to Mg, Ni, and Fe. The Mg(OH)2 phase is believed to be formed through the reaction of Mg or MgH2 with water vapor in the air. The dehydrided Mg–13.33Ni–6.67Fe sample after hydriding-dehydriding cycling contained Mg, Mg2Ni, MgO, and Fe.</description><identifier>ISSN: 0360-3199</identifier><identifier>EISSN: 1879-3487</identifier><identifier>DOI: 10.1016/j.ijhydene.2010.07.161</identifier><identifier>CODEN: IJHEDX</identifier><language>eng</language><publisher>Kidlington: Elsevier</publisher><subject>Alternative fuels. 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An 80 wt%Mg–13.33 wt%Ni–6.67 wt%Fe (referred to as Mg–13.33Ni–6.67Fe) sample exhibited higher hydriding and dehydriding rates after activation and a larger hydrogen storage capacity compared to those of other mixtures prepared under similar conditions. After activation (at n = 3), the sample absorbed 4.60 wt%H for 5 min and 5.61 wt%H for 60 min at 593 K under 12 bar H2. The sample desorbed 1.57 wt%H for 5 min and 3.92 wt%H for 30 min at 593 K under 1.0 bar H2. Rietveld analysis of the XRD pattern using FullProf program showed that the as-milled Mg–13.33Ni–6.67Fe sample contained Mg(OH)2 and MgH2 in addition to Mg, Ni, and Fe. The Mg(OH)2 phase is believed to be formed through the reaction of Mg or MgH2 with water vapor in the air. The dehydrided Mg–13.33Ni–6.67Fe sample after hydriding-dehydriding cycling contained Mg, Mg2Ni, MgO, and Fe.</description><subject>Alternative fuels. Production and utilization</subject><subject>Applied sciences</subject><subject>Chemical Sciences</subject><subject>Energy</subject><subject>Exact sciences and technology</subject><subject>Fuels</subject><subject>Hydrogen</subject><subject>Material chemistry</subject><issn>0360-3199</issn><issn>1879-3487</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNo9kMtOwzAQRS0EEqXwC8gbFiwSxo86ybKqKEEqsIG15SST1pWbRHao6N_jqtDVSFf3jGYOIfcMUgZMPW1Tu90cGuww5RBDyFKm2AWZsDwrEiHz7JJMQChIBCuKa3ITwhaAZSCLCdmUh8b3a-xoGHtv1kgH3w_oR4uB9i019G2dvNtkiXRnf8ZvfyzgYDw2dG8NHZzpcDT-QCvjXOw4Z7s1tV0kS07NuOvDsEGPt-SqNS7g3d-ckq_l8-eiTFYfL6-L-Sqp43VjUnDezlqoZgpbBryuVIUAIAWvFauKKsuRQ9sgy5v4QdEoCXU-U5xLppBlXEzJ42nvxjg9eLuLt-neWF3OV_qYAcykFFLuWeyqU7f2fQge2zPAQB_d6q3-d6uPbjVkOrqN4MMJHEyojWu96WobzjQXQiiZ5-IXJ9x7-Q</recordid><startdate>20101001</startdate><enddate>20101001</enddate><creator>MYOUNG YOUP SONG</creator><creator>SUNG HWAN BAEK</creator><creator>BOBET, Jean-Louis</creator><creator>HONG, Seong-Hyeon</creator><general>Elsevier</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0001-7838-7004</orcidid></search><sort><creationdate>20101001</creationdate><title>Hydrogen storage properties of a Mg-Ni-Fe mixture prepared via planetary ball milling in a H2 atmosphere</title><author>MYOUNG YOUP SONG ; SUNG HWAN BAEK ; BOBET, Jean-Louis ; HONG, Seong-Hyeon</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c319t-922f5f0b56ef102cb6be000432c61b9b78e20fde18d1709d640c85622416e1723</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Alternative fuels. Production and utilization</topic><topic>Applied sciences</topic><topic>Chemical Sciences</topic><topic>Energy</topic><topic>Exact sciences and technology</topic><topic>Fuels</topic><topic>Hydrogen</topic><topic>Material chemistry</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>MYOUNG YOUP SONG</creatorcontrib><creatorcontrib>SUNG HWAN BAEK</creatorcontrib><creatorcontrib>BOBET, Jean-Louis</creatorcontrib><creatorcontrib>HONG, Seong-Hyeon</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>International journal of hydrogen energy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>MYOUNG YOUP SONG</au><au>SUNG HWAN BAEK</au><au>BOBET, Jean-Louis</au><au>HONG, Seong-Hyeon</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Hydrogen storage properties of a Mg-Ni-Fe mixture prepared via planetary ball milling in a H2 atmosphere</atitle><jtitle>International journal of hydrogen energy</jtitle><date>2010-10-01</date><risdate>2010</risdate><volume>35</volume><issue>19</issue><spage>10366</spage><epage>10372</epage><pages>10366-10372</pages><issn>0360-3199</issn><eissn>1879-3487</eissn><coden>IJHEDX</coden><abstract>A sample composition has been designed based on previously reported data. An 80 wt%Mg–13.33 wt%Ni–6.67 wt%Fe (referred to as Mg–13.33Ni–6.67Fe) sample exhibited higher hydriding and dehydriding rates after activation and a larger hydrogen storage capacity compared to those of other mixtures prepared under similar conditions. After activation (at n = 3), the sample absorbed 4.60 wt%H for 5 min and 5.61 wt%H for 60 min at 593 K under 12 bar H2. The sample desorbed 1.57 wt%H for 5 min and 3.92 wt%H for 30 min at 593 K under 1.0 bar H2. Rietveld analysis of the XRD pattern using FullProf program showed that the as-milled Mg–13.33Ni–6.67Fe sample contained Mg(OH)2 and MgH2 in addition to Mg, Ni, and Fe. The Mg(OH)2 phase is believed to be formed through the reaction of Mg or MgH2 with water vapor in the air. The dehydrided Mg–13.33Ni–6.67Fe sample after hydriding-dehydriding cycling contained Mg, Mg2Ni, MgO, and Fe.</abstract><cop>Kidlington</cop><pub>Elsevier</pub><doi>10.1016/j.ijhydene.2010.07.161</doi><tpages>7</tpages><orcidid>https://orcid.org/0000-0001-7838-7004</orcidid></addata></record> |
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subjects | Alternative fuels. Production and utilization Applied sciences Chemical Sciences Energy Exact sciences and technology Fuels Hydrogen Material chemistry |
title | Hydrogen storage properties of a Mg-Ni-Fe mixture prepared via planetary ball milling in a H2 atmosphere |
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