This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility:

fact-checked

peer-reviewed publication

proofread

Hunting for supermassive black holes in the early universe

Hunting for supermassive black holes in the early universe
A supermassive black hole (SMBH; the small black dot at the center) absorbs surrounding material, which forms a spiral disk-like shape as it flows in. The gravitational energy of the material is converted to radiation and emitted away from the disk. SMBHs with such shining outskirts are called "quasars." Credit: Yoshiki Matsuoka, Ehime University

Supermassive black holes (SMBHs)—black holes with masses exceeding a million times that of the sun—are known to prevail in the universe today. However, it is not clear yet when, where, and how they formed during the 13.8 billion years of cosmic history.

Observations in the past few decades have revealed that every galaxy harbors a SMBH in the center, and that the black hole mass is almost always one-thousandth of the host galaxy mass. This close relationship implies that galaxies and SMBHs have co-evolved together. Revealing the origin of SMBHs is thus crucial not only to understand SMBHs themselves, but also to elucidate the formation processes of galaxies, the major constituents of the visible universe.

A key to addressing this issue lies in the , where the time elapse since the Big Bang (i.e., the beginning of the universe) was less than a billion years. Thanks to the finite speed of light, we can look back at the past by observing the distant universe. Did SMBHs already exist when the universe was only a billion years old or less? Is it possible for a black hole to acquire such a large mass (exceeding a million solar masses and sometimes reaching billions of solar masses) in such a short time? If so, what are the underlying physical mechanisms and conditions?

In order to close in on the origin of SMBHs, we need to observe them and compare their properties with predictions from . And in order to do so, we first need to find where they are in the sky.

We used the Subaru Telescope at the top of Maunakea, Hawaii, for the present study. One of the biggest advantages of Subaru is its widefield observing capability, which is particularly suited for our purpose. Since SMBHs do not emit light, we looked for a special class called "quasars"—SMBHs with shining outskirts where the infalling material releases .

We observed a wide sky area equivalent to 5,000 times the full moon, and successfully discovered 162 quasars residing in the early universe. In particular, 22 of them lived in the era when the universe was less than 800 million years old—the most ancient period in which quasars have been recognized to date.

The large number of quasars we discovered has allowed us to determine the most fundamental measure called the "luminosity function," which describes the space density of quasars as a function of radiation energy. We found that quasars were forming very rapidly in the early universe, while the overall shape of the luminosity function (except for the amplitude) remained unchanged over time.

This characteristic behavior of the luminosity function provides strong constraints on theoretical models, which could ultimately reproduce all the observables and describe the origin of SMBHs. Our study is published in The Astrophysical Journal Letters.

On the other hand, the universe was known to have experienced a major phase transition called "cosmic reionization" in its early stage. Past observations suggest that the whole intergalactic space was ionized in this event. The source of the ionization energy is still under debate, with radiation from quasars being considered as a promising candidate.

By integrating the above luminosity function, we found that quasars emit 1028 photons per second in a unit volume of 1 light-year on a side in the early . This is less than 1% of the photons needed to maintain the ionized state of the intergalactic space at that time, and thus indicates that made only a minor contribution to cosmic reionization. Other are critically needed, which, according to other recent observations, may be the integrated radiation from massive hot stars in forming galaxies.

More information: Yoshiki Matsuoka et al, Quasar Luminosity Function at z = 7, The Astrophysical Journal Letters (2023). DOI: 10.3847/2041-8213/acd69f

Journal information: Astrophysical Journal Letters

Provided by Ehime University

Citation: Hunting for supermassive black holes in the early universe (2023, September 1) retrieved 23 April 2024 from https://phys.org/news/2023-09-supermassive-black-holes-early-universe.html
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.

Explore further

Starlight and the first black holes: Researchers detect the host galaxies of quasars in the early universe

2644 shares

Feedback to editors