MD
M. Demianski
astro-phastro-ph.COastro-ph.HE
On Valency
published · living versionsW_bf8s9eqa·v1 · currentpublished
Model-independent calibration of gamma-ray bursts with Bayesian neural networks
with P. Caterino, E. Piedipalumbo, L. Amati, D. De Cicco +1
1 version
Preprints & journals
40 papers in the corpus · 1986–2024Formation of the first halos, galaxies and magnetic fields2405.19910v2 · M. Demia'nski, A. Doroshkevich, T. Larchenkova2024 · 0 citationsarXiv
Investigating Dark Energy Equation of State With High Redshift Hubble Diagram2010.05289v1 · Marek Demianski, Elisabeta Lusso, Maurizio Paolillo et al.2020 · 24 citationsFrontiers in Astronomy and Space Sciences (2020), 7, 69
The patch like model of galaxies formation: the virial paradox, core-cusp and missing satellite problems2009.04256v2 · M. Demia'nski, A. Doroshkevich2020 · 0 citationsarXiv
Prospects of high redshift constraints on dark energy models with the Ep- Eiso correlation in long Gamma Ray Bursts1911.08228v2 · M. Demianski, E.Piedipalumbo, D.Sawant et al.2019 · 43 citationsarXiv
High redshift constraints on dark energy models from the -- correlation in GRBs1802.01694v1 · Marek Demianski, Ester Piedipalumbo, Disha Sawant et al.2018 · 1 citationarXiv
Self similarity of the dark matter dominated objects and the shape of small scale power spectrum1701.03474v1 · M. Demia'nski, A. Doroshkevich2017 · 3 citationsarXiv
Cosmology with gamma-ray bursts: I. The Hubble diagram through the calibrated - correlation1610.00854v1 · Marek Demianski, Ester Piedipalumbo, Disha Sawant et al.2016 · 183 citationsarXiv
Cosmology with gamma-ray bursts: II Cosmography challenges and cosmological scenarios for the accelerated Universe1609.09631v2 · Marek Demianski, Ester Piedipalumbo, Disha Sawant et al.2016 · 103 citationsarXiv
Beyond the standard CDM cosmology: the observed structure of DM halos and the shape of the power spectrum1511.07989v6 · M. Demia'nski, A.G. Doroshkevich2015 · 3 citationsarXiv
Beyond the CDM cosmology: complex composition of dark matter1404.3362v2 · M. Demianski, A.Doroshkevich2014 · 1 citationarXiv
Semi analytical description of formation of galaxies and clusters of galaxies1307.7980v2 · Marek Demia'nski, Andrey Doroshkevich2013 · 4 citationsarXiv
High redshift cosmography: new results and implication for dark energy1206.7046v1 · Marek Demianski, Ester Piedipalumbo, Claudio Rubano et al.2012 · 54 citationsMonthly Notices of the Royal Astronomical Society, 426, pp. 1396-1415 (2012)
Standardizing the GRBs with the Amati Ep,i - Eiso relation: the updated Hubble diagram and implications for cosmography1104.5614v1 · Marek Demianski, Ester Piedipalumbo2011 · 34 citationsarXiv
Simulated evolution of the dark matter large-scale structure1102.2951v1 · M. Demia'nski, A. Doroshkevich, S. Pilipenko et al.2011 · 16 citationsarXiv
Statistical characteristics of the observed metal systems and problems of reionization0712.3454v2 · M. Demia'nski, A.G. Doroshkevich2007 · 0 citationsarXiv
Cosmological models in scalar tensor theories of gravity and observations: a class of general solutions0711.1043v1 · M.Demianski, E. Piedipalumbo, C.Rubano et al.2007 · 21 citationsAstron.Astrophys.481:279-294,2008
Possible extensions of the standard cosmological model: anisotropy, rotation, and magnetic fieldastro-ph/0702381v2 · M. Demia'nski, A.G. Doroshkevich2007 · 40 citationsPhys.Rev.D75:123517,2007
Accelerating universe in scalar tensor models - confrontation of theoretical predictions with observationsastro-ph/0604026v1 · M. Demianski, E. Piedipalumbo, C. Rubano et al.2006 · 45 citationsAstron.Astrophys.454:55-66,2006
Statistical characteristics of observed Ly- forest and the shape of linear power spectrumastro-ph/0506058v3 · M. Demianski, A.G. Doroshkevich, V.I.Turchaninov2005 · 9 citationsMon.Not.Roy.Astron.Soc.371:915-934,2006
Two viable quintessence models of the Universe: confrontation of theoretical predictions with observational dataastro-ph/0410445v1 · M. Demianski, E. Piedipalumbo, C. Rubano et al.2004 · 41 citationsAstron.Astrophys. 431 (2005) 27-43
Approximate angular diameter distance in a locally inhomogeneous universe with nonzero cosmological constantastro-ph/0310830v1 · M. Demianski, R. de Ritis, A.A. Marino et al.2003 · 32 citationsAstron.Astrophys. 411 (2003) 33-40
Observational estimates of the initial power spectrum at small scale from Lyman- absorbersastro-ph/0304484v2 · M. Demia'nski, A.G. Doroshkevich2003 · 14 citationsAstrophys.J. 597 (2003) 81-97
Statistical characteristics of observed Ly- forest and the shape of initial power spectrumastro-ph/0207136v2 · M. Demia'nski, A. Doroshkevich & V.Turchaninov2002 · 9 citationsarXiv
Properties of observed Ly- forestastro-ph/0006311v1 · M. Demianski, A. Doroshkevich, & V.Turchaninov2000 · 2 citationsMon.Not.Roy.Astron.Soc. 318 (2000) 1189
Redshift distribution of {\bf Ly-} lines and metal systemsastro-ph/0006312v1 · M. Demianski, A.G. Doroshkevich, & V.Turchaninov2000 · 4 citationsMon.Not.Roy.Astron.Soc. 318 (2000) 1177
Statistical characteristics of simulated wallsastro-ph/0005291v1 · M.Demianski, A.G. Doroshkevich, V.Mueller et al.2000 · 5 citationsMon.Not.Roy.Astron.Soc. 318 (2000) 665
The cosmological lens equation in a universe with non zero cosmological constantastro-ph/0004376v1 · M. Demianski, R. de Ritis, A.A. Marino et al.2000 · 0 citationsarXiv
Cosmological perturbations in exact-Noether background solutions.10019555 · Capozziello, Demianski, de Ritis R et al.2019 · 32 citationsPhysical review. D, Particles and fields. 1995;52(6):3288-3297
Instability of Langmuir waves in plasma irradiated by directed gamma rays.10057876 · Beloborodov, Demianski2019 · 4 citationsPhysical review letters. 1995;74(12):2232-2235
Resonance scales in the galaxy correlation function and the nature of dark matter.10017882 · Demianski, Ivanov, Novikov2019 · 2 citationsPhysical review. D, Particles and fields. 1994;50(4):2488-2495
Evolution of multidimensional flat anisotropic cosmological models.10016276 · Beloborodov, Demianski, Ivanov et al.2019 · 11 citationsPhysical review. D, Particles and fields. 1993;48(2):503-512
Gravitational-wave background in multidimensional cosmological models.10015549 · Demianski, Polnarev, Naselsky2019 · 14 citationsPhysical review. D, Particles and fields. 1993;47(12):5275-5279
Scalar fields and anisotropy in cosmological models.10015056 · Demianski, de Ritis R, Rubano et al.2019 · 57 citationsPhysical review. D, Particles and fields. 1992;46(4):1391-1398
Scalar field, nonminimal coupling, and cosmology.10013769 · Demianski, de Ritis R, Marmo et al.2019 · 52 citationsPhysical review. D, Particles and fields. 1991;44(10):3136-3146
Dynamical dimensional reduction induced by changing equation of state.10012229 · Demianski, Polnarev2019 · 11 citationsPhysical review. D, Particles and fields. 1990;41(10):3003-3011
Motion of test particles and light rays around massive conducting cosmic string.9959193 · Demianski2019 · 10 citationsPhysical review. D, Particles and fields. 1988;38(2):698-701
Dynamics of multidimensional generalization of Bianchi type-IX cosmological models.9958059 · Demianski, Heller, Szydlowski2019 · 18 citationsPhysical review. D, Particles and fields. 1987;36(10):2945-2954
Inflation in a Bianchi type-I Einstein-Cartan cosmological model.9957774 · Demianski, de Ritis R, Platania et al.2019 · 30 citationsPhysical review. D, Particles and fields. 1987;35(4):1181-1184
Erratum: How to measure the curvature of space-time9971970 · Ciufolini, Demianski2019 · 1 citationPhysical review. D, Particles and fields. 1987;35(2):773
How to measure the curvature of space-time.9957244 · Ciufolini, Demianski2019 · 28 citationsPhysical review. D, Particles and fields. 1986;34(4):1018-1020
Career total: 172 works. 40 are in this corpus.
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