ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY
Author
HONG LI1 ; XIA, Jun-Qing2 ; ZHAO, Gong-Bo3 ; FAN, Zu-Hui1 ; XINMII ZHANG2
[1]
Department of Astronomy, School of Physics, Peking University, Beijing 100871, China
[2]
Institute of High Energy Physics, Chinese Academy of Science, P.O. Box 918-4, Beijing 100049, China
[3]
Department of Physics, Simon Fraser University, Burnaby, BC V5A 1S6, Canada
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
"O:13:\"PanistOpenUrl\":36:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000idc\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:0:\"\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:105:\"ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"2008\";s:9:\"\u0000*\u0000volume\";s:3:\"683\";s:8:\"\u0000*\u0000issue\";s:1:\"1\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:5:\"L1-L4\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:7:\"HONG LI\";s:10:\"\u0000*\u0000aufirst\";s:0:\"\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:4:{i:0;s:13:\"XIA, Jun-Qing\";i:1;s:13:\"ZHAO, Gong-Bo\";i:2;s:11:\"FAN, Zu-Hui\";i:3;s:12:\"XINMII ZHANG\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"2\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:105:\"ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
"O:12:\"IstexOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:0:\"\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:105:\"ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"2008\";s:9:\"\u0000*\u0000volume\";s:3:\"683\";s:8:\"\u0000*\u0000issue\";s:1:\"1\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:5:\"L1-L4\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:7:\"HONG LI\";s:10:\"\u0000*\u0000aufirst\";s:0:\"\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:4:{i:0;s:13:\"XIA, Jun-Qing\";i:1;s:13:\"ZHAO, Gong-Bo\";i:2;s:11:\"FAN, Zu-Hui\";i:3;s:12:\"XINMII ZHANG\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"2\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:105:\"ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
"O:16:\"EuropePMCOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:0:\"\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:105:\"ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"2008\";s:9:\"\u0000*\u0000volume\";s:3:\"683\";s:8:\"\u0000*\u0000issue\";s:1:\"1\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:5:\"L1-L4\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:7:\"HONG LI\";s:10:\"\u0000*\u0000aufirst\";s:0:\"\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:4:{i:0;s:13:\"XIA, Jun-Qing\";i:1;s:13:\"ZHAO, Gong-Bo\";i:2;s:11:\"FAN, Zu-Hui\";i:3;s:12:\"XINMII ZHANG\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"2\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:105:\"ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
"O:11:\"BaseOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:0:\"\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:105:\"ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"2008\";s:9:\"\u0000*\u0000volume\";s:3:\"683\";s:8:\"\u0000*\u0000issue\";s:1:\"1\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:5:\"L1-L4\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:7:\"HONG LI\";s:10:\"\u0000*\u0000aufirst\";s:0:\"\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:4:{i:0;s:13:\"XIA, Jun-Qing\";i:1;s:13:\"ZHAO, Gong-Bo\";i:2;s:11:\"FAN, Zu-Hui\";i:3;s:12:\"XINMII ZHANG\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"2\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:105:\"ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
"O:12:\"ArXivOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:0:\"\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:105:\"ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"2008\";s:9:\"\u0000*\u0000volume\";s:3:\"683\";s:8:\"\u0000*\u0000issue\";s:1:\"1\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:5:\"L1-L4\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:7:\"HONG LI\";s:10:\"\u0000*\u0000aufirst\";s:0:\"\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:4:{i:0;s:13:\"XIA, Jun-Qing\";i:1;s:13:\"ZHAO, Gong-Bo\";i:2;s:11:\"FAN, Zu-Hui\";i:3;s:12:\"XINMII ZHANG\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"2\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:105:\"ON USING THE WMAP DISTANCE INFORMATION IN CONSTRAINING THE TIME-EVOLVING EQUATION OF STATE OF DARK ENERGY\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"