We provide for the first time the growth index of linear matter fluctuations of the power law f (T) proportional to (-T)(b) gravity model. We find that the asymptotic form of this particular f (T) model is gamma approximate to 6/11-6b, which obviously extends that of the ACDM model, gamma(A) approximate to 6/11. Finally, we generalize the growth index analysis of f (T) gravity in the case where gamma is allowed to vary with redshift.
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CSIC, Inst Space Sci ICE, C Can Magrans S-N, Barcelona 08193, Spain
Inst Catalana Recerca & Estudis Avancats ICREA, Passeig Luis Companys 23, Barcelona 08010, SpainCSIC, Inst Space Sci ICE, C Can Magrans S-N, Barcelona 08193, Spain
Odintsov, Sergei D.
Oikonomou, V. K.
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Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki 54124, Greece
Tomsk State Univ Control Syst & Radioelect TUSUR, Int Lab Theoret Cosmol, Tomsk 634050, RussiaCSIC, Inst Space Sci ICE, C Can Magrans S-N, Barcelona 08193, Spain
Oikonomou, V. K.
Sharov, German S.
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Tomsk State Univ Control Syst & Radioelect TUSUR, Int Lab Theoret Cosmol, Tomsk 634050, Russia
Tver State Univ, Sadovyj per 35, Tver 170002, RussiaCSIC, Inst Space Sci ICE, C Can Magrans S-N, Barcelona 08193, Spain
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Univ Cape Town, Dept Math & Appl Math, ZA-7925 Cape Town, South AfricaUniv Cape Town, Dept Math & Appl Math, ZA-7925 Cape Town, South Africa
Goheer, Naureen
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Larena, Julien
Dunsby, Peter K. S.
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Univ Cape Town, Dept Math & Appl Math, ZA-7925 Cape Town, South Africa
S African Astron Observ, ZA-7925 Cape Town, South AfricaUniv Cape Town, Dept Math & Appl Math, ZA-7925 Cape Town, South Africa