Модели аккреции в модифицированных теориях гравитации

Описание НИОКР

R_{\mu\nu} - \dfrac{R}{2}g_{\mu\nu} = \dfrac{8\pi G}{c^4}T_{\mu\nu}

R_{\mu\nu} - \dfrac{R}{2}g_{\mu\nu} + \Lambda g_{\mu\nu} = \dfrac{8\pi G}{c^4}T_{\mu\nu}

f\left(R_{\mu\nu}\right) - \dfrac{f(R)}{2}g_{\mu\nu} = \dfrac{8\pi G}{c^4}T_{\mu\nu}

Способы решения

1. Космологическая постоянная:

2. Модифицирование уравнений:

Имеющийся задел

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Имеющийся задел

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