Strong-field tests of f (R)-gravity in binary pulsars

被引:1
|
作者
Dyadina, Polina I. [1 ,2 ]
Alexeyev, Stanislav O. [1 ]
Capozziello, Salvatore [3 ,4 ,5 ]
De Laurentis, Mariafelicia [3 ,6 ]
Rannu, Kristina A. [1 ]
机构
[1] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Univ Sky Prospekt 13, Moscow 119991, Russia
[2] Moscow MV Lomonosov State Univ, Dept Phys, Moscow 119991, Russia
[3] Univ Naples Federico II, Dipartimento Sci Fis, I-80126 Naples, Italy
[4] Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy
[5] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Via F Crispi 7, I-67100 Laquila, Italy
[6] Tomsk State Pedag Univ, Ul Kievskaya 60, Tomsk 634061, Russia
关键词
Binary pulsars; f (R)-gravity; post-Keplerian formalism; RELATIVISTIC GRAVITY; PRINCIPLE;
D O I
10.1142/S2010194516601319
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We develop the parameterized post-Keplerian approach for class of analytic f(R)-gravity models. Using the double binary pulsar system PSR J0737-3039 data we obtain restrictions on the parameters of this class of f(R)-models and show that f(R)-gravity is not ruled out by the observations in strong field regime. The additional and more strong corresponding restriction is extracted from solar system data.
引用
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页数:9
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