| Шығарылым |
Атауы |
Файл |
| Том 24, № 2 (2018) |
Bianchi Type-I Dust-Filled Accelerating Brans–Dicke Cosmology |
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Sharma U., Goswami G., Pradhan A.
|
| Том 23, № 2 (2017) |
Calculating luminosity distance versus redshift in FLRW cosmology via homotopy perturbation method |
|
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Shchigolev V.
|
| Том 23, № 2 (2017) |
Can bigravity gravitational baryogenesis explain the CMB 143 GHz excess line? |
|
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Oikonomou V.
|
| Том 22, № 3 (2016) |
Can gravity distinguish between Dirac and Majorana neutrinos? |
|
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Alavi S., Abbasnezhad A.
|
| Том 22, № 2 (2016) |
Centenary of Einstein’s general relativity. Its present extensions |
|
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Melnikov V.
|
| Том 22, № 1 (2016) |
Chameleon scalar field in LRS Bianchi type I cosmological model |
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Chaubey R., Singh A., Raushan R.
|
| Том 25, № 3 (2019) |
Chiral Cosmological Model of f(R) Gravity with a Kinetic Curvature Scalar |
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Chervon S., Fomin I., Mayorova T.
|
| Том 22, № 3 (2016) |
Chronometric measurement of orthometric height differences by means of atomic clocks |
|
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Kopeikin S., Kanushin V., Karpik A., Tolstikov A., Gienko E., Goldobin D., Kosarev N., Ganagina I., Mazurova E., Karaush A., Hanikova E.
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| Том 24, № 3 (2018) |
Classical Electromagnetic Potential as a Part of Gravitational Connection: Ideas and History |
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Kharuk N., Paston S., Sheykin A.
|
| Том 22, № 1 (2016) |
Collisionless self-gravitating statistical systems of scalarly interacting particles |
|
|
Ignat’ev Y.
|
| Том 22, № 2 (2016) |
Conformal representations of the general scalar-tensor theory and cosmological models |
|
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Chubaryan E., Avagyan R., Harutyunyan G., Hovsepyan A., Kotanjyan A.
|
| Том 25, № 4 (2019) |
Conservative Relativistic Algebrodynamics Induced on an Implicitly Defined World Line |
|
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Chala A., Kassandrov V., Markova N.
|
| Том 23, № 2 (2017) |
Constraints on scalar coupling to electromagnetism |
|
|
Antoniou I.
|
| Том 23, № 3 (2017) |
Cosmological acceleration from a scalar field and classical and quantum gravitational waves (Inflation and dark energy) |
|
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Marochnik L.
|
| Том 24, № 2 (2018) |
Cosmological Exact Solutions in Some Modified Gravitational Theories |
|
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Bisabr Y.
|
| Том 25, № 2 (2019) |
Cosmological Solutions in 2 + 1-Dimensional New Massive Gravity in the Presence of the Dirac Field |
|
|
Gecim G., Sucu Y.
|
| Том 23, № 1 (2017) |
Cosmological solutions in low-energy effective field theory for type IIA superstrings |
|
|
Brandyshev P.
|
| Том 22, № 1 (2016) |
Curvature correction to vacuum fluctuations and cosmic evolution with cosmological duality |
|
|
Kalita S.
|
| Том 22, № 1 (2016) |
Dark energy and inflation in a gravitational wave dominated universe |
|
|
Marochnik L.
|
| Том 23, № 3 (2017) |
Dark energy or local acceleration? |
|
|
Feoli A., Benedetto E.
|
| Том 25, № 4 (2019) |
Dark Matter Particles: Properties and Detections |
|
|
Ennadifi S., Douhou K.
|
| Том 25, № 3 (2019) |
Dark Matter: the Problem of Motion |
|
|
Kahil M.
|
| Том 25, № 2 (2019) |
De Sitter-Invariant Special Relativity and Galaxy Rotation Curves |
|
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Araujo A., López D., Pereira J.
|
| Том 24, № 2 (2018) |
DE-DM Unification Based on Space-Time Symmetry |
|
|
Dymnikova I.
|
| Том 22, № 3 (2016) |
Dilatonic (quasi-) black holes without scalar charge |
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|
Bronnikov K., Israpilov D.
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| Нәтижелер 216 - 26/50 |
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