Severity: Warning
Message: file_get_contents(https://...@gmail.com&api_key=61f08fa0b96a73de8c900d749fcb997acc09): Failed to open stream: HTTP request failed! HTTP/1.1 429 Too Many Requests
Filename: helpers/my_audit_helper.php
Line Number: 143
Backtrace:
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 143
Function: file_get_contents
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 209
Function: simplexml_load_file_from_url
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 3098
Function: getPubMedXML
File: /var/www/html/application/controllers/Detail.php
Line: 574
Function: pubMedSearch_Global
File: /var/www/html/application/controllers/Detail.php
Line: 488
Function: pubMedGetRelatedKeyword
File: /var/www/html/index.php
Line: 316
Function: require_once
Severity: Warning
Message: Attempt to read property "Count" on bool
Filename: helpers/my_audit_helper.php
Line Number: 3100
Backtrace:
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 3100
Function: _error_handler
File: /var/www/html/application/controllers/Detail.php
Line: 574
Function: pubMedSearch_Global
File: /var/www/html/application/controllers/Detail.php
Line: 488
Function: pubMedGetRelatedKeyword
File: /var/www/html/index.php
Line: 316
Function: require_once
The structures of the 6H perovskites Ba(3)B(2+)Sb(5+)(2)O(9), B = Ca and Sr, have been solved and refined using synchrotron X-ray and neutron powder diffraction data. Ba(3)CaSb(2)O(9) and Ba(3)SrSb(2)O(9) have monoclinic C2/c and triclinic P\bar 1 space-group symmetries, respectively, while Ba(3)MgSb(2)O(9) has ideal hexagonal P6(3)/mmc space-group symmetry. The symmetry-lowering distortions are a consequence of internal ;chemical pressure' owing to the increasing effective ionic radius of the alkaline-earth cation in the perovskite B site from Mg(2+) (0.72 A) to Ca(2+) (1.00 A) to Sr(2+) (1.18 A). Increasing the effective ionic radius further to Ba(2+) (1.35 A) leads to decomposition at room temperature. The driving force behind the transition from P6(3)/mmc to C2/c is the need to alleviate underbonding of Ba(2+) cations in the perovskite A site via octahedral rotations, while the transition from C2/c to P\bar 1 is driven by the need to regularize the shape of the Sb(2)O(9) face-sharing octahedral dimers. Ab initio geometry-optimization calculations were used to find a triclinic starting model for Ba(3)SrSb(2)O(9).
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Source |
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http://dx.doi.org/10.1107/S0108768108005041 | DOI Listing |
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