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researcher

E. Mikheeva

8 papers hereh-index 10393 citations99 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author3
  • last author4

Across the 8 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO4
  • gr-qc3
  • astro-ph.GA1
same name
  • E. Mikheeva — 2 papers, h 2
  • E. Mikheeva — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators
Showing astro-ph.COShow all

4 papers · 1 filter

astro-ph.CO2025

High-z SMBHs in Cosmological Models with Enhanced Power Spectra

M. V. Tkachev, S. V. Pilipenko, E. V. Mikheeva +1

We consider the impact of non-power-law spectra of matter perturbations with a bump or with a blue tilt at small scales on the evolution of supermassive black holes (SMBHs) located…

astro-ph.CO2025

Constraints on primordial black holes from interstellar dust temperature in the Galaxy

A. N. Melikhov, E. V. Mikheeva

The photons emitted by primordial black holes (PBHs) can be a heating factor for interstellar dust. Assuming that dust in the Galaxy has a homogeneous distribution and that PBHs ha…

astro-ph.CO2025

Constraints on the Number of Primordial Black Holes Due to Interaction with Dust

A. N. Melikhov, E. V. Mikheeva

Photons emitted by primordial black holes (PBHs) due to the Hawking effect are among the factors of interstellar dust heating. Based on the data on the temperature of dust, constra…

astro-ph.CO2024

Inner structure of dark matter halos at high z in cosmological models with non-power-law primordial spectra

M. V. Tkachev, S. V. Pilipenko, E. V. Mikheeva +1

We consider three cosmological models with non-power-law spectra of primordial density perturbations and test them against I^›CDM in density profiles of dark matter halos. We foun…

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