Growth of Central Massive Black Holes and Feedback on Host Galaxies using Cosmological Simulations
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| Format: | Recurso digital |
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Zenodo
2026
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| _version_ | 1866901359380398080 |
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| author | Barai, Paramita |
| author_facet | Barai, Paramita |
| contents | Supermassive Black Holes (SMBHs) at the centers of high-z quasars are observed to have grown to masses >= 10^9 Msun by redshifts z=6-7. Recent JWST observations are additionally revealing the existence of central intermediate-mass BHs (10^7 - 10^8 Msun) at even earlier epochs z~10-12; some of which sources have BH mass comparable to the mass of the host galaxy. At the same time, very recent JWST observations have detected a population of normal-mass central SMBHs at z~3-5, with the mean SMBH-to stellar mass ratio consistent with the local relation. The formation of such supermassive (overmassive and normal-mass) BHs at the centers of their host galaxies involves unresolved questions. |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18804799 |
| institution | Zenodo |
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| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Growth of Central Massive Black Holes and Feedback on Host Galaxies using Cosmological Simulations Barai, Paramita Supermassive Black Holes (SMBHs) at the centers of high-z quasars are observed to have grown to masses >= 10^9 Msun by redshifts z=6-7. Recent JWST observations are additionally revealing the existence of central intermediate-mass BHs (10^7 - 10^8 Msun) at even earlier epochs z~10-12; some of which sources have BH mass comparable to the mass of the host galaxy. At the same time, very recent JWST observations have detected a population of normal-mass central SMBHs at z~3-5, with the mean SMBH-to stellar mass ratio consistent with the local relation. The formation of such supermassive (overmassive and normal-mass) BHs at the centers of their host galaxies involves unresolved questions. |
| title | Growth of Central Massive Black Holes and Feedback on Host Galaxies using Cosmological Simulations |
| url | https://doi.org/10.5281/zenodo.18804799 |