Product
Help
Pricing
About
Jobs
Log in
Get started
Author
Add to collection
M. V. Tkachev
Observed names:
M V Tkachev,
M.V. Tkacev,
M. V. Tkachev,
Maxim Tkachev,
Maxim V Tkachev,
Tkachev, M. V.,
М. В. Ткачев
show all 7
Institutions:
P.N. Lebedev Physical Institute of the Russian Academy of Sciences,
Astro Space Center
Observed institutions:
P.N. Lebedev Physical Institute of the Russian Academy of Sciences,
Russian Academy of Sciences,
Astro Space Center
ORCID:
0000-0003-4446-0757
Observed ORCID:
0000-0003-4446-0757
OpenAlex ID:
A5063759475
Excess of high- z galaxies as a test for bumpy power spectrum of density perturbations
2023
·
M V Tkachev
, S V Pilipenko
, et al.
·
Monthly Notices of the Royal Astronomical Society
·
26
PDF
Dark matter simulations with primordial black holes in the early Universe
2020
·
Maxim V Tkachev
, Sergey V Pilipenko
, et al.
·
Monthly Notices of the Royal Astronomical Society
·
25
PDF
Evolution of a primordial binary black hole due to interaction with cold dark matter and the formation rate of gravitational wave events
2022
·
Sergey Pilipenko
, Maxim Tkachev
, et al.
·
Physical review. D/Physical review. D.
·
18
PDF
Inner structure of dark matter halos at high z in cosmological models with non-power-law primordial spectra
2024
·
M. V. Tkachev
, S. V. Pilipenko
, et al.
·
Physical review. D/Physical review. D.
·
10
PDF
A model of the cosmic infrared background produced by distant galaxies
2017
·
S. V. Pilipenko
, M. V. Tkachev
, et al.
·
Astronomy Letters
·
7
PDF
Cvoystva tsentral'nykh oblastey galo temnoy materii v modeli s bampom v spektre moshchnosti vozmushcheniy plotnosti
2024
·
Yu. N. Eroshenko
, V. N. Lukash
, et al.
·
Письма в Журнал экспериментальной и теоретической физики
·
5
PDF
Galaxies at $$\boldsymbol{z\gtrsim 10}$$ and New Opportunities for Testing Cosmological Models
2024
·
S. V. Pilipenko
, S. A. Drozdov
, et al.
·
Astrophysical Bulletin
·
4
PDF
Absorption in the 21 cm Hydrogen Line at $$\boldsymbol{z>10}$$ as a Sensitive Tool for the Construction of a Cosmological Model on Small Scales
2025
·
Yu. N. Eroshenko
, V. N. Lukash
, et al.
·
Astronomy Letters
·
2
PDF
On the Increase in the Density of Primordial Black Holes in the Halos of Dwarf Galaxies
2025
·
S. V. Pilipenko
, M. V. Tkachev
, et al.
·
Journal of Experimental and Theoretical Physics Letters
·
2
PDF
Constraints on Features in the Cosmological Power Spectrum from Observations of the Epoch of Reionization
2025
·
O. R. Skorikov
, S. V. Pilipenko
, et al.
·
Astronomy Letters
·
1
New Estimates of the Merger Rate of Primordial Black Holes with Allowance for Clustering Dark Matter
2022
·
M. V. Tkachev
, S. V. Pilipenko
·
Astronomy Letters
·
1
Do primordial black hole clusters survive the Galaxy? Collisional disruption and microlensing implications
2026
·
M. V. Tkachev
, S. V. Pilipenko
·
Physical review. D/Physical review. D.
PDF
Origin of monolithic high-z galaxies and UV luminosity of mergering high-z galaxies in the cosmological model with non-standard spectrum of density perturbations
2026
·
Eroshenko, Yu. N.
, Lukash, V. N.
, et al.
·
arXiv (Cornell University)
PDF
Constraints on features in the cosmological power spectrum from observations of the epoch of reionization
2026
·
O. R. Skorikov
, S. V. Pilipenko
, et al.
·
Physics of Space: All-Russian Student Scientific Conference with International Participation
PDF
High- z supermassive black holes in cosmological models with enhanced power spectra
2025
·
M. V. Tkachev
, S. V. Pilipenko
, et al.
·
Physical review. D/Physical review. D.
PDF
Ограничения На Особенности В Космологическом Спектре Мощности Из Наблюдений Эпохи Вторичной Ионизации
2025
·
O.R. Skorikov
, S.V. Pilipenko
, et al.
·
Astronomy Letters
Modeling Dark-Matter Halos. Verification of the Entropy Approach to the Cusp Problem
2019
·
M. V. Tkachev
, S. V. Pilipenko
, et al.
·
Astronomy Reports
Моделирование гало темной материи. Проверка энтропийного подхода к проблеме каспов
2019
·
М. В. Ткачев
, С. В. Пилипенко
, et al.
·
Astronomicheskii Zhurnal
Show more works
View as search
Works count:
18
Citation count:
101
H-index:
5
I10-index:
4
Year
Topic
Type