We show that the presence of a nonminimal interaction between dark matter and dark energy may lead to a violation of the null energy condition and to the formation of a configuration with nontrivial topology (a wormhole). In this it is assumed that both dark matter and dark energy satisfy the null energy condition, a violation of which takes place only in the inner high-density regions of the configuration. This is achieved by assuming that, in a high-density environment, a nonminimal coupling function changes its sign in comparison with the case where dark matter and dark energy have relatively low densities which are typical for a cosmological background. For this case, we find regular static, spherically symmetric solutions describing wormholes supported by dark matter nonminimally coupled to dark energy in the form of a quintessence scalar field.
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Yunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R ChinaYunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R China
Liu, Yun
Liao, Shihong
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Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2, FI-00014 Helsinki, FinlandYunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R China
Liao, Shihong
Liu, Xiangkun
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Yunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R ChinaYunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R China
Liu, Xiangkun
Zhang, Jiajun
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Inst Basic Sci IBS, Ctr Theoret Phys Universe, Daejeon 34126, South Korea
Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R ChinaYunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R China
Zhang, Jiajun
An, Rui
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Univ Southern Calif, Dept Phys & Astron, Los Angeles, CA 90089 USAYunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R China
An, Rui
Fan, Zuhui
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Yunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R ChinaYunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R China
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Chinese Acad Sci, Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R ChinaChinese Acad Sci, Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China
Cai, Yi-Fu
Marciano, Antonino
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Fudan Univ, Dept Phys, Shanghai 200433, Peoples R China
Fudan Univ, Ctr Field Theory & Particle Phys, Shanghai 200433, Peoples R ChinaChinese Acad Sci, Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China
Marciano, Antonino
Wang, Dong-Gang
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Chinese Acad Sci, Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China
Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands
Leiden Univ, Inst Lorentz Theoret Phys, NL-2333 CA Leiden, NetherlandsChinese Acad Sci, Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China
Wang, Dong-Gang
Wilson-Ewing, Edward
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Albert Einstein Inst, Max Planck Inst Gravitat Phys, Muhlenberg 1, D-14476 Golm, GermanyChinese Acad Sci, Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China