Loading…

First principles molecular dynamics simulations of diopside (CaMgSi 2O 6) liquid to high pressure

We use first principles molecular dynamics simulations based on density functional theory in the local density approximation to investigate CaMgSi 2O 6 liquid over the entire mantle pressure regime. We find that the liquid structure becomes much more densely packed with increasing pressure, with the...

Full description

Saved in:
Bibliographic Details
Published in:Geochimica et cosmochimica acta 2011-07, Vol.75 (13), p.3792-3802
Main Authors: Sun, Ni, Stixrude, Lars, Koker, Nico de, Karki, Bijaya B.
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c354t-759aa3b5cdf08ba6bf6f72678f32b1483a9f5fe6c9b34f4bef29456948e6a3003
cites cdi_FETCH-LOGICAL-c354t-759aa3b5cdf08ba6bf6f72678f32b1483a9f5fe6c9b34f4bef29456948e6a3003
container_end_page 3802
container_issue 13
container_start_page 3792
container_title Geochimica et cosmochimica acta
container_volume 75
creator Sun, Ni
Stixrude, Lars
Koker, Nico de
Karki, Bijaya B.
description We use first principles molecular dynamics simulations based on density functional theory in the local density approximation to investigate CaMgSi 2O 6 liquid over the entire mantle pressure regime. We find that the liquid structure becomes much more densely packed with increasing pressure, with the mean Si–O coordination number increasing nearly linearly with volume from fourfold near ambient pressure to sixfold at the base of the mantle. Fivefold Si–O coordination environments are most abundant at intermediate compression. The properties of Mg and Si coordination environments are nearly identical to those in MgSiO 3 liquid, whereas Ca is more highly coordinated with larger mean Ca–O bond length as compared with Mg. The density increases smoothly with increasing pressure over the entire range studied. The Grüneisen parameter increases by a factor of three on twofold compression. The density contrast between diopside composition liquid and the isochemical crystalline assemblage is less than 2% at the core mantle boundary, less than that in the case of MgSiO 3. Thermodynamic properties are described in terms of a liquid-state fundamental thermodynamic relation.
doi_str_mv 10.1016/j.gca.2011.04.004
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1678534370</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S0016703711002146</els_id><sourcerecordid>1678534370</sourcerecordid><originalsourceid>FETCH-LOGICAL-c354t-759aa3b5cdf08ba6bf6f72678f32b1483a9f5fe6c9b34f4bef29456948e6a3003</originalsourceid><addsrcrecordid>eNp9kE1r3DAURUVJoZO0P6Crapku7EqW5A-6KkOmCaRkkWYtZPlp8gbbmujZhfz7apiss3rwOPfCPYx9laKUQtY_DuXeu7ISUpZCl0LoD2wj26YqOqPUBduIDBWNUM0ndkl0EEI0xogNcztMtPBjwtnjcQTiUxzBr6NLfHid3YSeOOGUHwvGmXgMfMB4JByAX2_dn_0j8uqB19_5iC8rDnyJ_Bn3z7kSiNYEn9nH4EaCL2_3ij3tbv5ub4v7h99321_3hVdGL0VjOudUb_wQRNu7ug91aKq6aYOqeqlb5bpgAtS-65UOuodQddrUnW6hdkoIdcWuz73HFF9WoMVOSB7G0c0QV7IydxmlVXNC5Rn1KRIlCDbvn1x6tVLYk057sFmnPem0QtusM2e-nTPBRev2Cck-PWbAZLNSma7LxM8zAXnlP4RkySPMHgZM4Bc7RHyn_z9l0YZ2</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1678534370</pqid></control><display><type>article</type><title>First principles molecular dynamics simulations of diopside (CaMgSi 2O 6) liquid to high pressure</title><source>ScienceDirect Freedom Collection 2022-2024</source><creator>Sun, Ni ; Stixrude, Lars ; Koker, Nico de ; Karki, Bijaya B.</creator><creatorcontrib>Sun, Ni ; Stixrude, Lars ; Koker, Nico de ; Karki, Bijaya B.</creatorcontrib><description>We use first principles molecular dynamics simulations based on density functional theory in the local density approximation to investigate CaMgSi 2O 6 liquid over the entire mantle pressure regime. We find that the liquid structure becomes much more densely packed with increasing pressure, with the mean Si–O coordination number increasing nearly linearly with volume from fourfold near ambient pressure to sixfold at the base of the mantle. Fivefold Si–O coordination environments are most abundant at intermediate compression. The properties of Mg and Si coordination environments are nearly identical to those in MgSiO 3 liquid, whereas Ca is more highly coordinated with larger mean Ca–O bond length as compared with Mg. The density increases smoothly with increasing pressure over the entire range studied. The Grüneisen parameter increases by a factor of three on twofold compression. The density contrast between diopside composition liquid and the isochemical crystalline assemblage is less than 2% at the core mantle boundary, less than that in the case of MgSiO 3. Thermodynamic properties are described in terms of a liquid-state fundamental thermodynamic relation.</description><identifier>ISSN: 0016-7037</identifier><identifier>EISSN: 1872-9533</identifier><identifier>DOI: 10.1016/j.gca.2011.04.004</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><subject>calcium ; magnesium ; molecular dynamics ; silicon ; thermodynamics</subject><ispartof>Geochimica et cosmochimica acta, 2011-07, Vol.75 (13), p.3792-3802</ispartof><rights>2011 Elsevier Ltd</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c354t-759aa3b5cdf08ba6bf6f72678f32b1483a9f5fe6c9b34f4bef29456948e6a3003</citedby><cites>FETCH-LOGICAL-c354t-759aa3b5cdf08ba6bf6f72678f32b1483a9f5fe6c9b34f4bef29456948e6a3003</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Sun, Ni</creatorcontrib><creatorcontrib>Stixrude, Lars</creatorcontrib><creatorcontrib>Koker, Nico de</creatorcontrib><creatorcontrib>Karki, Bijaya B.</creatorcontrib><title>First principles molecular dynamics simulations of diopside (CaMgSi 2O 6) liquid to high pressure</title><title>Geochimica et cosmochimica acta</title><description>We use first principles molecular dynamics simulations based on density functional theory in the local density approximation to investigate CaMgSi 2O 6 liquid over the entire mantle pressure regime. We find that the liquid structure becomes much more densely packed with increasing pressure, with the mean Si–O coordination number increasing nearly linearly with volume from fourfold near ambient pressure to sixfold at the base of the mantle. Fivefold Si–O coordination environments are most abundant at intermediate compression. The properties of Mg and Si coordination environments are nearly identical to those in MgSiO 3 liquid, whereas Ca is more highly coordinated with larger mean Ca–O bond length as compared with Mg. The density increases smoothly with increasing pressure over the entire range studied. The Grüneisen parameter increases by a factor of three on twofold compression. The density contrast between diopside composition liquid and the isochemical crystalline assemblage is less than 2% at the core mantle boundary, less than that in the case of MgSiO 3. Thermodynamic properties are described in terms of a liquid-state fundamental thermodynamic relation.</description><subject>calcium</subject><subject>magnesium</subject><subject>molecular dynamics</subject><subject>silicon</subject><subject>thermodynamics</subject><issn>0016-7037</issn><issn>1872-9533</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNp9kE1r3DAURUVJoZO0P6Crapku7EqW5A-6KkOmCaRkkWYtZPlp8gbbmujZhfz7apiss3rwOPfCPYx9laKUQtY_DuXeu7ISUpZCl0LoD2wj26YqOqPUBduIDBWNUM0ndkl0EEI0xogNcztMtPBjwtnjcQTiUxzBr6NLfHid3YSeOOGUHwvGmXgMfMB4JByAX2_dn_0j8uqB19_5iC8rDnyJ_Bn3z7kSiNYEn9nH4EaCL2_3ij3tbv5ub4v7h99321_3hVdGL0VjOudUb_wQRNu7ug91aKq6aYOqeqlb5bpgAtS-65UOuodQddrUnW6hdkoIdcWuz73HFF9WoMVOSB7G0c0QV7IydxmlVXNC5Rn1KRIlCDbvn1x6tVLYk057sFmnPem0QtusM2e-nTPBRev2Cck-PWbAZLNSma7LxM8zAXnlP4RkySPMHgZM4Bc7RHyn_z9l0YZ2</recordid><startdate>20110701</startdate><enddate>20110701</enddate><creator>Sun, Ni</creator><creator>Stixrude, Lars</creator><creator>Koker, Nico de</creator><creator>Karki, Bijaya B.</creator><general>Elsevier Ltd</general><scope>FBQ</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7S9</scope><scope>L.6</scope></search><sort><creationdate>20110701</creationdate><title>First principles molecular dynamics simulations of diopside (CaMgSi 2O 6) liquid to high pressure</title><author>Sun, Ni ; Stixrude, Lars ; Koker, Nico de ; Karki, Bijaya B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c354t-759aa3b5cdf08ba6bf6f72678f32b1483a9f5fe6c9b34f4bef29456948e6a3003</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>calcium</topic><topic>magnesium</topic><topic>molecular dynamics</topic><topic>silicon</topic><topic>thermodynamics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sun, Ni</creatorcontrib><creatorcontrib>Stixrude, Lars</creatorcontrib><creatorcontrib>Koker, Nico de</creatorcontrib><creatorcontrib>Karki, Bijaya B.</creatorcontrib><collection>AGRIS</collection><collection>CrossRef</collection><collection>AGRICOLA</collection><collection>AGRICOLA - Academic</collection><jtitle>Geochimica et cosmochimica acta</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sun, Ni</au><au>Stixrude, Lars</au><au>Koker, Nico de</au><au>Karki, Bijaya B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>First principles molecular dynamics simulations of diopside (CaMgSi 2O 6) liquid to high pressure</atitle><jtitle>Geochimica et cosmochimica acta</jtitle><date>2011-07-01</date><risdate>2011</risdate><volume>75</volume><issue>13</issue><spage>3792</spage><epage>3802</epage><pages>3792-3802</pages><issn>0016-7037</issn><eissn>1872-9533</eissn><abstract>We use first principles molecular dynamics simulations based on density functional theory in the local density approximation to investigate CaMgSi 2O 6 liquid over the entire mantle pressure regime. We find that the liquid structure becomes much more densely packed with increasing pressure, with the mean Si–O coordination number increasing nearly linearly with volume from fourfold near ambient pressure to sixfold at the base of the mantle. Fivefold Si–O coordination environments are most abundant at intermediate compression. The properties of Mg and Si coordination environments are nearly identical to those in MgSiO 3 liquid, whereas Ca is more highly coordinated with larger mean Ca–O bond length as compared with Mg. The density increases smoothly with increasing pressure over the entire range studied. The Grüneisen parameter increases by a factor of three on twofold compression. The density contrast between diopside composition liquid and the isochemical crystalline assemblage is less than 2% at the core mantle boundary, less than that in the case of MgSiO 3. Thermodynamic properties are described in terms of a liquid-state fundamental thermodynamic relation.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/j.gca.2011.04.004</doi><tpages>11</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0016-7037
ispartof Geochimica et cosmochimica acta, 2011-07, Vol.75 (13), p.3792-3802
issn 0016-7037
1872-9533
language eng
recordid cdi_proquest_miscellaneous_1678534370
source ScienceDirect Freedom Collection 2022-2024
subjects calcium
magnesium
molecular dynamics
silicon
thermodynamics
title First principles molecular dynamics simulations of diopside (CaMgSi 2O 6) liquid to high pressure
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-08T01%3A07%3A33IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=First%20principles%20molecular%20dynamics%20simulations%20of%20diopside%20(CaMgSi%202O%206)%20liquid%20to%20high%20pressure&rft.jtitle=Geochimica%20et%20cosmochimica%20acta&rft.au=Sun,%20Ni&rft.date=2011-07-01&rft.volume=75&rft.issue=13&rft.spage=3792&rft.epage=3802&rft.pages=3792-3802&rft.issn=0016-7037&rft.eissn=1872-9533&rft_id=info:doi/10.1016/j.gca.2011.04.004&rft_dat=%3Cproquest_cross%3E1678534370%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c354t-759aa3b5cdf08ba6bf6f72678f32b1483a9f5fe6c9b34f4bef29456948e6a3003%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1678534370&rft_id=info:pmid/&rfr_iscdi=true