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Dark Energy Cosmology with Spinor Field
Recent observations have shown that our universe is currently undergoing a period of accelerating expansion. In view of the astrophysical data we find that the equation of state of the dark energy lies in a narrow range around w = −1. In this paper we discuss the possibility of treating a spinor fie...
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Published in: | International journal of theoretical physics 2023-10, Vol.62 (Suppl 1), Article S1 |
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container_title | International journal of theoretical physics |
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creator | Sun, Zu-Yao Shen, You-Gen |
description | Recent observations have shown that our universe is currently undergoing a period of accelerating expansion. In view of the astrophysical data we find that the equation of state of the dark energy lies in a narrow range around
w
= −1. In this paper we discuss the possibility of treating a spinor field as dark energy to realize the equation of state parameter
w
< −1 or
w
> −1. We derive the main equations which govern the evolution of the universe and then discuss the evolution and attractor property of this model, and show a late time de Sitter attractor. Finally we rewrite them with the observable quantities. |
doi_str_mv | 10.1007/s10773-006-9128-x |
format | article |
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w
= −1. In this paper we discuss the possibility of treating a spinor field as dark energy to realize the equation of state parameter
w
< −1 or
w
> −1. We derive the main equations which govern the evolution of the universe and then discuss the evolution and attractor property of this model, and show a late time de Sitter attractor. Finally we rewrite them with the observable quantities.</description><identifier>ISSN: 0020-7748</identifier><identifier>EISSN: 1572-9575</identifier><identifier>DOI: 10.1007/s10773-006-9128-x</identifier><language>eng</language><publisher>New York: Springer New York</publisher><subject>Dark energy ; Elementary Particles ; Equations of state ; Evolution ; Mathematical and Computational Physics ; Physics ; Quantum Field Theory ; Quantum Physics ; Theoretical ; Universe</subject><ispartof>International journal of theoretical physics, 2023-10, Vol.62 (Suppl 1), Article S1</ispartof><rights>Springer Science+Business Media, Inc. 2006</rights><rights>Springer Science+Business Media, Inc. 2006.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c316t-8e0e0b245a5e54ed7d5975d04a82bd4e47654c8ed69440c5ee351b44d6c791333</citedby><cites>FETCH-LOGICAL-c316t-8e0e0b245a5e54ed7d5975d04a82bd4e47654c8ed69440c5ee351b44d6c791333</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, Zu-Yao</creatorcontrib><creatorcontrib>Shen, You-Gen</creatorcontrib><title>Dark Energy Cosmology with Spinor Field</title><title>International journal of theoretical physics</title><addtitle>Int J Theor Phys</addtitle><description>Recent observations have shown that our universe is currently undergoing a period of accelerating expansion. In view of the astrophysical data we find that the equation of state of the dark energy lies in a narrow range around
w
= −1. In this paper we discuss the possibility of treating a spinor field as dark energy to realize the equation of state parameter
w
< −1 or
w
> −1. We derive the main equations which govern the evolution of the universe and then discuss the evolution and attractor property of this model, and show a late time de Sitter attractor. Finally we rewrite them with the observable quantities.</description><subject>Dark energy</subject><subject>Elementary Particles</subject><subject>Equations of state</subject><subject>Evolution</subject><subject>Mathematical and Computational Physics</subject><subject>Physics</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Theoretical</subject><subject>Universe</subject><issn>0020-7748</issn><issn>1572-9575</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><recordid>eNp1kEFLAzEQhYMoWKs_wNuCB0_RSTLZJEeprQqCB_Uctptp3dpuatJi--_dsoInT_MO73sDH2OXAm4EgLnNAoxRHKDkTkjLd0dsILSR3Gmjj9kAQAI3Bu0pO8t5AQAO0A7Y9X2VPotxS2m-L0Yxr-Iydum72XwUr-umjamYNLQM5-xkVi0zXfzeIXufjN9Gj_z55eFpdPfMayXKDbcEBFOJutKkkYIJ2hkdACsrpwEJTamxthRKhwi1JlJaTBFDWRsnlFJDdtXvrlP82lLe-EXcprZ76aU1VgknSuxaom_VKeacaObXqVlVae8F-IMP3_vwnQ9_8OF3HSN7Jnfddk7pb_l_6AdkoGEj</recordid><startdate>20231001</startdate><enddate>20231001</enddate><creator>Sun, Zu-Yao</creator><creator>Shen, You-Gen</creator><general>Springer New York</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20231001</creationdate><title>Dark Energy Cosmology with Spinor Field</title><author>Sun, Zu-Yao ; Shen, You-Gen</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c316t-8e0e0b245a5e54ed7d5975d04a82bd4e47654c8ed69440c5ee351b44d6c791333</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Dark energy</topic><topic>Elementary Particles</topic><topic>Equations of state</topic><topic>Evolution</topic><topic>Mathematical and Computational Physics</topic><topic>Physics</topic><topic>Quantum Field Theory</topic><topic>Quantum Physics</topic><topic>Theoretical</topic><topic>Universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sun, Zu-Yao</creatorcontrib><creatorcontrib>Shen, You-Gen</creatorcontrib><collection>CrossRef</collection><jtitle>International journal of theoretical physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sun, Zu-Yao</au><au>Shen, You-Gen</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Dark Energy Cosmology with Spinor Field</atitle><jtitle>International journal of theoretical physics</jtitle><stitle>Int J Theor Phys</stitle><date>2023-10-01</date><risdate>2023</risdate><volume>62</volume><issue>Suppl 1</issue><artnum>S1</artnum><issn>0020-7748</issn><eissn>1572-9575</eissn><abstract>Recent observations have shown that our universe is currently undergoing a period of accelerating expansion. In view of the astrophysical data we find that the equation of state of the dark energy lies in a narrow range around
w
= −1. In this paper we discuss the possibility of treating a spinor field as dark energy to realize the equation of state parameter
w
< −1 or
w
> −1. We derive the main equations which govern the evolution of the universe and then discuss the evolution and attractor property of this model, and show a late time de Sitter attractor. Finally we rewrite them with the observable quantities.</abstract><cop>New York</cop><pub>Springer New York</pub><doi>10.1007/s10773-006-9128-x</doi></addata></record> |
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language | eng |
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source | Springer Nature |
subjects | Dark energy Elementary Particles Equations of state Evolution Mathematical and Computational Physics Physics Quantum Field Theory Quantum Physics Theoretical Universe |
title | Dark Energy Cosmology with Spinor Field |
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