Abstract
The effects implied for the structure of compact objects by the modification of General Relativity (GR) produced by the generalization of the Lagrangian density to the form \(f(R)=R+\alpha R^2\), where \(R\) is the Ricci curvature scalar, have been recently explored. It seems likely that this squared-gravity may allow heavier Neutron Stars (NSs) than GR. In addition, these objects can be useful to constrain free parameters of modified-gravity theories. The differences between alternative gravity theories are enhanced in the strong gravitational regime. In this regime, because of the complexity of the field equations, perturbative methods become a good choice to treat the problem. Following previous works in the field, we performed a numerical integration of the structure equations that describe NSs in \(f(R)\)-gravity, recovering their mass-radius relations, but focusing on particular features that arise from this approach in the profiles of the NS interior. We show that these profiles run in correlation with the second-order derivative of the analytic approximation to the Equation of State (EoS), which leads to regions where the enclosed mass decreases with the radius in a counter-intuitive way. We reproduce all computations with a simple polytropic EoS to separate zeroth-order modified gravity effects.
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Notes
The Ricci scalar in terms of the functions of the metric (1) is:
$$\begin{aligned} R=\frac{2\,e^{-2\Lambda }\!\! \left[r^2 \left\{ \varPhi ^{\prime } \Lambda ^{\prime }+ (\varPhi ^{\prime })^2\!\!+ \varPhi ^{\prime \prime }\!\right\} \!+\!2r\left(\varPhi ^{\prime } - \Lambda ^{\prime }\,\right) -e^{2\Lambda }\!\!+1\right]}{r^2}. \end{aligned}$$
References
Amanullah, R., Lidman, C., Rubin, D., Aldering, G., Astier, P., Barbary, K., Burns, M. S., Conley, A., Dawson, K. S., Deustua, S. E., Doi, M., Fabbro, S., Faccioli, L., Fakhouri, H. K., Folatelli, G., Fruchter, A. S., Furusawa, H., Garavini, G., Goldhaber, G., Goobar, A., Groom, D. E., Hook, I., Howell, D. A., Kashikawa, N., Kim, A. G., Knop, R. A., Kowalski, M., Linder, E., Meyers, J., Morokuma, T., Nobili, S., Nordin, J., Nugent, P. E., Östman, L., Pain, R., Panagia, N., Perlmutter, S., Raux, J., Ruiz-Lapuente, P., Spadafora, A. L., Strovink, M., Suzuki, N., Wang, L., Wood-Vasey, W. M., Yasuda, N., and Supernova Cosmology Project, T.: ApJ 716, 712 (2010)
Arapoğlu, S., Deliduman, C., Yavuz Ekşi, K.: J. Cosmol. Astropart. Phys. 7, 20 (2011)
Babichev, E., Langlois, D.: Phys. Rev. D 81(12), 124051 (2010)
Bolejko, K., Célérier, M.-N., Krasiński, A.: Class. Quantum Gravit. 28(16), 164002 (2011)
Capozziello, S., Faraoni, V.: Beyond Einstein Gravity. A survey of Gravitational Theories for Cosmology and Astrophysics. Springer, Berlin (2011)
Cooney, A., Dedeo, S., Psaltis, D.: Phys. Rev. D 79(4), 044033 (2009)
Cooney, A., Dedeo, S., Psaltis, D.: Phys. Rev. D 82(6), 064033 (2010)
de Felice, A., Tsujikawa, S.: Living Rev. Relativ. 13, 3 (2010)
DeDeo, S., Psaltis, D.: Phys. Rev. Lett. 90(14), 141101 (2003)
Deliduman, C., Ekşi, K.Y., Keleş, V.: J. Cosmol. Astropart. Phys. 5, 36 (2011).
Demorest, P.B., Pennucci, T., Ransom, S.M., Roverts, M.S.E, Hesseks, J.W.T: Nature 467, 1081 (2010)
Douchin, F., Haensel, P.: A &A 380, 151 (2001)
Gungor, C. Yavuz Eksi, K.: ArXiv e-prints /1108.2166 (2011)
Haensel, P., Potekhin, A.Y.: A &A 428, 191 (2004)
Hu, W., Sawicki, I.: Phys. Rev. D 76(6), 064004 (2007)
Jaime, L.G., Patiño, L., Salgado, M.: Phys. Rev. D 83(2), 024039 (2011)
Komatsu, E., Smith, K.M., Dunkley, J., Bennett, C.L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Nolta, M.R., Page, L., Spergel, D.N., Halpern, M., Hill, R.S., Kogut, A., Limon, M., Meyer, S.S., Odegard, N., Tucker, G.S., Weiland, J.L., Wollack, E., Wright, E.L.: ApJS 192, 18 (2011)
Larson, D., Dunkley, J., Hinshaw, G., Komatsu, E., Nolta, M.R., Bennett, C.L., Gold, B., Halpern, M., Hill, R.S., Jarosik, N., Kogut, A., Limon, M., Meyer, S.S., Odegard, N., Page, L., Smith, K.M., Spergel, D.N., Tucker, G.S., Weiland, J.L., Wollack, E., Wright, E.L.: ApJS 192, 16 (2011)
Miranda, V., Jorás, S.E., Waga, I., Quartin, M.: Phys. Rev. Lett. 102(22), 221101 (2009)
Oppenheimer, J.R., Volkoff, G.M.: Phys. Rev. 55, 374–381 (1939)
Percival, W.J., Reid, B.A., Eisenstein, D.J., Bahcall, N.A., Budavari, T., Frieman, J.A., Fukugita, M., Gunn, J.E., Ivezić, Ž., Knapp, G.R., Kron, R.G., Loveday, J., Lupton, R.H., McKay, T.A., Meiksin, A., Nichol, R.C., Pope, A.C., Schlegel, D.J., Schneider, D.P., Spergel, D.N., Stoughton, C., Strauss, M.A., Szalay, A.S., Tegmark, M., Vogeley, M.S., Weinberg, D.H., York, D.G., Zehavi, I.: MNRAS 401, 2148 (2010)
Read, J.S., Lackey, B.D., Owen, B.J., Friedman, J.L.: Phys. Rev. D 79(12), 124032 (2009)
Riess, A.G., Macri, L., Casertano, S., Sosey, M., Lampeitl, H., Ferguson, H.C., Filippenko, A.V., Jha, S.W., Li, W., Chornock, R., Sarkar, D.: ApJ 699, 539 (2009)
Santos, E.: Phys. Rev. D 81(6), 064030 (2010)
Santos, E.: AP & SS, 341, 411 (2012)
Silbar, R.R., Reddy, S.: Am. J. Phys. 72, 892 (2004)
Sotiriou, T.P., Faraoni, V.: Rev. Mod. Phys. 82, 451 (2010)
Starobinsky, A.A.: Sov. J. Exp. Theor. Phys. Lett. 86, 157 (2007)
Tolman, R.C.: Astrophys. J. 90, 568 (1939)
Wen, D.-H., Li, B.-A., Chen, L.-W.: ArXiv e-prints /1101.1504 (2011)
Acknowledgments
We thank Dr. Arapoğlu for explanations. The authors appreciate helpful comments from Prof. Santiago E. Pérez Bergliaffa. M.O. acknowledge support by the Argentine Agency CONICET and ANPCyT through grants PICT 2010-0213/ Prestamo BID and PICT-2007-00848. G.E.R. was supported by PIP 2010-0078 (CONICET) and the Spanish Ministerio de Innovación y Tecnología under grant AYA 2010-21782-C03-01.
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Mariana Orellana, Gustavo E. Romero: Member of CONICET.
Federico García, Florencia A. Teppa Pannia: Fellow of CONICET.
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Orellana, M., García, F., Teppa Pannia, F.A. et al. Structure of neutron stars in \(R\)-squared gravity. Gen Relativ Gravit 45, 771–783 (2013). https://doi.org/10.1007/s10714-013-1501-5
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DOI: https://doi.org/10.1007/s10714-013-1501-5