Self-regulated reionization
Recently, we have presented the first, truly large-scale radiative transfer simulations of inhomogeneous cosmic reionization which resolve all the possible halo sources down to the dwarf galaxy mass range, M≳ 109 M⊙, in a comoving volume (100 h−1 Mpc)3. This is large enough to sample the global mean...
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| Published in | Monthly notices of the Royal Astronomical Society Vol. 376; no. 2; pp. 534 - 548 |
|---|---|
| Main Authors | , , , |
| Format | Journal Article |
| Language | English |
| Published |
Oxford, UK
Blackwell Publishing Ltd
01.04.2007
Blackwell Science Oxford University Press |
| Subjects | |
| Online Access | Get full text |
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| Abstract | Recently, we have presented the first, truly large-scale radiative transfer simulations of inhomogeneous cosmic reionization which resolve all the possible halo sources down to the dwarf galaxy mass range, M≳ 109 M⊙, in a comoving volume (100 h−1 Mpc)3. This is large enough to sample the global mean history, geometry and statistical properties of reionization fairly and accurately for the first time. Here we present new simulations which extend the source halo mass range downward to 108 M⊙, to capture the full range of halo masses thought to be primarily responsible for reionization by their star formation following atomic hydrogen radiative cooling and gravitational collapse. Haloes below about 109 M⊙, however, are subject to Jeans-mass filtering in the ionized regions, which suppresses their baryonic content and their ability to release ionizing radiation. By including these smaller mass haloes but accounting for their suppression, too, we find that reionization is ‘self-regulating’, as follows. As the mean ionized fraction rises, so does the fraction of the volume within which suppression occurs. Hence, the degree of suppression is related to the mean ionized fraction. Since low-mass haloes with high efficiency (i.e. high emissivity) achieve a given mean ionized fraction earlier than do those with low efficiency, Jeans-mass filtering compensates for the difference in the emissivity of the suppressible haloes in these two cases. As a result, in the presence of lower mass source haloes, reionization begins earlier, but the later stages of reionization and the time of overlap are dictated by the efficiency of the higher mass haloes, independent of the efficiency of the suppressible, lower mass haloes. Hence, while the lower mass haloes do not alter the overlap redshift, zov, they serve to boost the electron-scattering optical depth of the universe, τes. This may explain why observations of quasar absorption spectra at high redshift find that reionization ended late (zov < 7), while cosmic microwave background polarization measurements report a large enough τes that reionization must have begun much earlier (z > 11). We present results for the Lambda cold dark matter universe with cosmological parameters from both 1- and 3-yr data releases of Wilkinson Microwave Anisotropy Probe. Reionization histories consistent with current constraints on zov and τes are shown to be achievable with standard stellar sources in haloes above 108 M⊙. Neither minihaloes nor exotic sources are required, and the phenomenon of ‘double reionization’ previously suggested does not occur. |
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| AbstractList | Recently, we have presented the first, truly large-scale radiative transfer simulations of inhomogeneous cosmic reionization which resolve all the possible halo sources down to the dwarf galaxy mass range, M≳ 109 M⊙, in a comoving volume (100 h−1 Mpc)3. This is large enough to sample the global mean history, geometry and statistical properties of reionization fairly and accurately for the first time. Here we present new simulations which extend the source halo mass range downward to 108 M⊙, to capture the full range of halo masses thought to be primarily responsible for reionization by their star formation following atomic hydrogen radiative cooling and gravitational collapse. Haloes below about 109 M⊙, however, are subject to Jeans-mass filtering in the ionized regions, which suppresses their baryonic content and their ability to release ionizing radiation. By including these smaller mass haloes but accounting for their suppression, too, we find that reionization is ‘self-regulating’, as follows. As the mean ionized fraction rises, so does the fraction of the volume within which suppression occurs. Hence, the degree of suppression is related to the mean ionized fraction. Since low-mass haloes with high efficiency (i.e. high emissivity) achieve a given mean ionized fraction earlier than do those with low efficiency, Jeans-mass filtering compensates for the difference in the emissivity of the suppressible haloes in these two cases. As a result, in the presence of lower mass source haloes, reionization begins earlier, but the later stages of reionization and the time of overlap are dictated by the efficiency of the higher mass haloes, independent of the efficiency of the suppressible, lower mass haloes. Hence, while the lower mass haloes do not alter the overlap redshift, zov, they serve to boost the electron-scattering optical depth of the universe, τes. This may explain why observations of quasar absorption spectra at high redshift find that reionization ended late (zov < 7), while cosmic microwave background polarization measurements report a large enough τes that reionization must have begun much earlier (z > 11). We present results for the Lambda cold dark matter universe with cosmological parameters from both 1- and 3-yr data releases of Wilkinson Microwave Anisotropy Probe. Reionization histories consistent with current constraints on zov and τes are shown to be achievable with standard stellar sources in haloes above 108 M⊙. Neither minihaloes nor exotic sources are required, and the phenomenon of ‘double reionization’ previously suggested does not occur. ABSTRACT Recently, we have presented the first, truly large‐scale radiative transfer simulations of inhomogeneous cosmic reionization which resolve all the possible halo sources down to the dwarf galaxy mass range, M≳ 109 M⊙, in a comoving volume (100 h−1 Mpc)3. This is large enough to sample the global mean history, geometry and statistical properties of reionization fairly and accurately for the first time. Here we present new simulations which extend the source halo mass range downward to 108 M⊙, to capture the full range of halo masses thought to be primarily responsible for reionization by their star formation following atomic hydrogen radiative cooling and gravitational collapse. Haloes below about 109 M⊙, however, are subject to Jeans‐mass filtering in the ionized regions, which suppresses their baryonic content and their ability to release ionizing radiation. By including these smaller mass haloes but accounting for their suppression, too, we find that reionization is ‘self‐regulating’, as follows. As the mean ionized fraction rises, so does the fraction of the volume within which suppression occurs. Hence, the degree of suppression is related to the mean ionized fraction. Since low‐mass haloes with high efficiency (i.e. high emissivity) achieve a given mean ionized fraction earlier than do those with low efficiency, Jeans‐mass filtering compensates for the difference in the emissivity of the suppressible haloes in these two cases. As a result, in the presence of lower mass source haloes, reionization begins earlier, but the later stages of reionization and the time of overlap are dictated by the efficiency of the higher mass haloes, independent of the efficiency of the suppressible, lower mass haloes. Hence, while the lower mass haloes do not alter the overlap redshift, zov, they serve to boost the electron‐scattering optical depth of the universe, τes. This may explain why observations of quasar absorption spectra at high redshift find that reionization ended late (zov < 7), while cosmic microwave background polarization measurements report a large enough τes that reionization must have begun much earlier (z > 11). We present results for the Lambda cold dark matter universe with cosmological parameters from both 1‐ and 3‐yr data releases of Wilkinson Microwave Anisotropy Probe. Reionization histories consistent with current constraints on zov and τes are shown to be achievable with standard stellar sources in haloes above 108 M⊙. Neither minihaloes nor exotic sources are required, and the phenomenon of ‘double reionization’ previously suggested does not occur. Recently, we have presented the first, truly large-scale radiative transfer simulations of inhomogeneous cosmic reionization which resolve all the possible halo sources down to the dwarf galaxy mass range, M[gsim] 10 super(9) M sub([odot]), in a comoving volume (100 h super(-1) Mpc) super(3). This is large enough to sample the global mean history, geometry and statistical properties of reionization fairly and accurately for the first time. Here we present new simulations which extend the source halo mass range downward to 10 super(8) M sub([odot]), to capture the full range of halo masses thought to be primarily responsible for reionization by their star formation following atomic hydrogen radiative cooling and gravitational collapse. Haloes below about 10 super(9) M sub([odot]), however, are subject to Jeans-mass filtering in the ionized regions, which suppresses their baryonic content and their ability to release ionizing radiation. By including these smaller mass haloes but accounting for their suppression, too, we find that reionization is 'self-regulating', as follows. As the mean ionized fraction rises, so does the fraction of the volume within which suppression occurs. Hence, the degree of suppression is related to the mean ionized fraction. Since low-mass haloes with high efficiency (i.e. high emissivity) achieve a given mean ionized fraction earlier than do those with low efficiency, Jeans-mass filtering compensates for the difference in the emissivity of the suppressible haloes in these two cases. As a result, in the presence of lower mass source haloes, reionization begins earlier, but the later stages of reionization and the time of overlap are dictated by the efficiency of the higher mass haloes, independent of the efficiency of the suppressible, lower mass haloes. Hence, while the lower mass haloes do not alter the overlap redshift, z sub(ov), they serve to boost the electron-scattering optical depth of the universe, tau sub(es). This may explain why observations of quasar absorption spectra at high redshift find that reionization ended late (z sub(ov) < 7), while cosmic microwave background polarization measurements report a large enough tau sub(es) that reionization must have begun much earlier (z > 11). We present results for the Lambda cold dark matter universe with cosmological parameters from both 1- and 3-yr data releases of Wilkinson Microwave Anisotropy Probe. Reionization histories consistent with current constraints on z sub(ov) and tau sub(es) are shown to be achievable with standard stellar sources in haloes above 10 super(8) M sub([odot]). Neither minihaloes nor exotic sources are required, and the phenomenon of 'double reionization' previously suggested does not occur. Recently, we have presented the first, truly large-scale radiative transfer simulations of inhomogeneous cosmic reionization which resolve all the possible halo sources down to the dwarf galaxy mass range, M[> ~] 109 M[middot in circle], in a comoving volume (100 h-1 Mpc)3. This is large enough to sample the global mean history, geometry and statistical properties of reionization fairly and accurately for the first time. Here we present new simulations which extend the source halo mass range downward to 108 M[middot in circle], to capture the full range of halo masses thought to be primarily responsible for reionization by their star formation following atomic hydrogen radiative cooling and gravitational collapse. Haloes below about 109 M[middot in circle], however, are subject to Jeans-mass filtering in the ionized regions, which suppresses their baryonic content and their ability to release ionizing radiation. By including these smaller mass haloes but accounting for their suppression, too, we find that reionization is 'self-regulating', as follows. As the mean ionized fraction rises, so does the fraction of the volume within which suppression occurs. Hence, the degree of suppression is related to the mean ionized fraction. Since low-mass haloes with high efficiency (i.e. high emissivity) achieve a given mean ionized fraction earlier than do those with low efficiency, Jeans-mass filtering compensates for the difference in the emissivity of the suppressible haloes in these two cases. As a result, in the presence of lower mass source haloes, reionization begins earlier, but the later stages of reionization and the time of overlap are dictated by the efficiency of the higher mass haloes, independent of the efficiency of the suppressible, lower mass haloes. Hence, while the lower mass haloes do not alter the overlap redshift, z ov, they serve to boost the electron-scattering optical depth of the universe, tau es. This may explain why observations of quasar absorption spectra at high redshift find that reionization ended late (zov < 7), while cosmic microwave background polarization measurements report a large enough tau es that reionization must have begun much earlier (z > 11). We present results for the Lambda cold dark matter universe with cosmological parameters from both 1- and 3-yr data releases of Wilkinson Microwave Anisotropy Probe. Reionization histories consistent with current constraints on z ov and tau es are shown to be achievable with standard stellar sources in haloes above 108 M[middot in circle]. Neither minihaloes nor exotic sources are required, and the phenomenon of 'double reionization' previously suggested does not occur. [PUBLICATION ABSTRACT] Recently, we have presented the first, truly large-scale radiative transfer simulations of inhomogeneous cosmic reionization which resolve all the possible halo sources down to the dwarf galaxy mass range, M≳ 109 M⊙, in a comoving volume (100 h −1 Mpc)3. This is large enough to sample the global mean history, geometry and statistical properties of reionization fairly and accurately for the first time. Here we present new simulations which extend the source halo mass range downward to 108 M⊙, to capture the full range of halo masses thought to be primarily responsible for reionization by their star formation following atomic hydrogen radiative cooling and gravitational collapse. Haloes below about 109 M⊙, however, are subject to Jeans-mass filtering in the ionized regions, which suppresses their baryonic content and their ability to release ionizing radiation. By including these smaller mass haloes but accounting for their suppression, too, we find that reionization is 'self-regulating', as follows. As the mean ionized fraction rises, so does the fraction of the volume within which suppression occurs. Hence, the degree of suppression is related to the mean ionized fraction. Since low-mass haloes with high efficiency (i.e. high emissivity) achieve a given mean ionized fraction earlier than do those with low efficiency, Jeans-mass filtering compensates for the difference in the emissivity of the suppressible haloes in these two cases. As a result, in the presence of lower mass source haloes, reionization begins earlier, but the later stages of reionization and the time of overlap are dictated by the efficiency of the higher mass haloes, independent of the efficiency of the suppressible, lower mass haloes. Hence, while the lower mass haloes do not alter the overlap redshift, z ov, they serve to boost the electron-scattering optical depth of the universe, τes. This may explain why observations of quasar absorption spectra at high redshift find that reionization ended late (z ov < 7), while cosmic microwave background polarization measurements report a large enough τes that reionization must have begun much earlier (z > 11). We present results for the Lambda cold dark matter universe with cosmological parameters from both 1- and 3-yr data releases of Wilkinson Microwave Anisotropy Probe. Reionization histories consistent with current constraints on z ov and τes are shown to be achievable with standard stellar sources in haloes above 108 M⊙. Neither minihaloes nor exotic sources are required, and the phenomenon of 'double reionization' previously suggested does not occur. |
| Author | Iliev, Ilian T. Mellema, Garrelt Pen, Ue-Li Shapiro, Paul R. |
| Author_xml | – sequence: 1 givenname: Ilian T. surname: Iliev fullname: Iliev, Ilian T. email: iliev@cita.utoronto.ca, * iliev@cita.utoronto.ca organization: Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St George Street, Toronto, Canada ON M5S 3H8 – sequence: 2 givenname: Garrelt surname: Mellema fullname: Mellema, Garrelt organization: Stockholm Observatory, AlbaNova University Centre, Stockholm University, SE-106 91 Stockholm, Sweden – sequence: 3 givenname: Paul R. surname: Shapiro fullname: Shapiro, Paul R. organization: Department of Astronomy, University of Texas, Austin, TX 78712-1083, USA – sequence: 4 givenname: Ue-Li surname: Pen fullname: Pen, Ue-Li organization: Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St George Street, Toronto, Canada ON M5S 3H8 |
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| Keywords | galaxies: formation radio lines: galaxies intergalactic medium radiative transfer large-scale structure of Universe cosmology: theory Intergalactic matter Polarization Red shift Ionizing radiations Cosmic background radiation WMAP satellite Large-scale structure Extended source Star formation Galaxy formation Cold dark matter Cosmic radio sources Radiative transfer Optical thickness Absorption spectra Optical scattering Quasars Electron scattering Radio galaxies Cosmological parameter Dwarf galaxies Gravitational collapse Cosmology |
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| Snippet | Recently, we have presented the first, truly large-scale radiative transfer simulations of inhomogeneous cosmic reionization which resolve all the possible... ABSTRACT Recently, we have presented the first, truly large‐scale radiative transfer simulations of inhomogeneous cosmic reionization which resolve all the... |
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| SubjectTerms | Astronomy Astrophysics cosmology: theory Earth, ocean, space Exact sciences and technology galaxies: formation intergalactic medium Ions large-scale structure of Universe radiative transfer radio lines: galaxies Simulation Stars & galaxies |
| Title | Self-regulated reionization |
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