Scalar and vector perturbations in a universe with nonlinear perfect fluid von Canay, Ezgi, Brilenkov, Ruslan, Eingorn, Maxim, Arapoğlu, A. Savaş, Zhuk, Alexander

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Scalar perturbations in cosmological f(R) models: the cosmic screening approach von Akarsu, Özgür, Brilenkov, Ruslan, Eingorn, Maxim, Shulga, Valerii, Zhuk, Alexander

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Second-order Cosmological Perturbations Engendered by Point-like Masses von Brilenkov, Ruslan, Eingorn, Maxim

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Perfect fluids with ω=const as sources of scalar cosmological perturbations von Eingorn, Maxim, Brilenkov, Ruslan

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Scalar perturbations in cosmological f von Akarsu, Özgür, Brilenkov, Ruslan, Eingorn, Maxim, Shulga, Valerii, Zhuk, Alexander

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Scalar perturbations in the late Universe: viability of the Chaplygin gas models von Bouhmadi-López, Mariam, Brilenkov, Maxim, Brilenkov, Ruslan, Morais, João, Zhuk, Alexander

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Are dark energy models with variable EoS parameter w compatible with the late inhomogeneous Universe? von Akarsu, Özgür, Bouhmadi-López, Mariam, Brilenkov, Maxim, Brilenkov, Ruslan, Eingorn, Maxim, Zhuk, Alexander

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Second-order Cosmological Perturbations Engendered by Point-like Masses von Brilenkov, Ruslan, Eingorn, Maxim

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Perfect fluids with $\omega=\mathrm{const}$ as sources of scalar cosmological perturbations von Eingorn, Maxim, Brilenkov, Ruslan

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Scalar and vector perturbations in a universe with nonlinear perfect fluid von Canay, Ezgi, Brilenkov, Ruslan, Eingorn, Maxim, Arapoğlu, A Savaş, Zhuk, Alexander

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Perfect fluids with \(\omega=\mathrm{const}\) as sources of scalar cosmological perturbations von Eingorn, Maxim, Brilenkov, Ruslan

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Scalar perturbations in cosmological $f(R)$ models: the cosmic screening approach von Akarsu, Ozgur, Brilenkov, Ruslan, Eingorn, Maxim, Shulga, Valerii, Zhuk, Alexander

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Dark and visible matter distribution in Coma cluster: theory vs observations von Brilenkov, Ruslan, Eingorn, Maxim, Zhuk, Alexander

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Dark and visible matter distribution in Coma cluster: theory vs observations von Brilenkov, Ruslan, Eingorn, Maxim, Zhuk, Alexander

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Scalar perturbations in the late Universe: viability of the Chaplygin gas models von Bouhmadi-López, Mariam, Brilenkov, Maxim, Brilenkov, Ruslan, Morais, João, Zhuk, Alexander

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Are dark energy models with variable EoS parameter $w$ compatible with the late inhomogeneous Universe? von Akarsu, Ozgur, Bouhmadi-López, Mariam, Brilenkov, Maxim, Brilenkov, Ruslan, Eingorn, Maxim, Zhuk, Alexander

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Scalar perturbations in cosmological \(f(R)\) models: the cosmic screening approach von Akarsu, Ozgur, Brilenkov, Ruslan, Eingorn, Maxim, Shulga, Valerii, Zhuk, Alexander

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Are dark energy models with variable EoS parameter \(w\) compatible with the late inhomogeneous Universe? von Akarsu, Ozgur, Bouhmadi-López, Mariam, Brilenkov, Maxim, Brilenkov, Ruslan, Eingorn, Maxim, Zhuk, Alexander

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