並列摘要
We study the matter power spectrum in cosmology based on the expo- nential f(R) gravity model by using the program, Modication of Growth with CAMB (MGCAMB). We also examine the eect of the matter power spectrum when a massive neutrino is considered. By comparing the spectra between the theoretical expectations and the observation of the luminous red galaxies (lrg) from the Sloan Digital Sky Survey (SDSS) of the Seventh Data Release (DR7), we nd that the exponential f(R) gravity model is compatible with larger neutrino mass than the CDM model.
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延伸閱讀
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- 陳依婷 (2009). Neutrino Masses Through Zee Mechanism in 5D Split Fermion Model [master's thesis, National Tsing Hua University]. Airiti Library. https://doi.org/10.6843/NTHU.2009.00448
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- Bernardini, E., Camilleri, L., Flaminio, V., Goswami, S., & Seo, S. H. (2014). Neutrino Masses and Oscillations. Advances in High Energy Physics, 2014(), 559-562-154. https://doi.org/10.1155/2014/823127