Home > Research > Publications & Outputs > Primordial black hole formation during slow reh...

Associated organisational unit

Electronic data

  • 1804.08639

    Accepted author manuscript, 569 KB, PDF document

    Available under license: CC BY-NC: Creative Commons Attribution-NonCommercial 4.0 International License

  • PRD22

    Final published version, 325 KB, PDF document

    Available under license: Unspecified

Links

Text available via DOI:

View graph of relations

Primordial black hole formation during slow reheating after inflation

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

Primordial black hole formation during slow reheating after inflation. / Carr, Bernard; Dimopoulos, Konstantinos; Owen, Charlotte et al.
In: Physical Review D – Particles and Fields, Vol. 97, 123535, 26.06.2018.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Carr, B, Dimopoulos, K, Owen, C & Tenkanen, T 2018, 'Primordial black hole formation during slow reheating after inflation', Physical Review D – Particles and Fields, vol. 97, 123535. https://doi.org/10.1103/PhysRevD.97.123535

APA

Carr, B., Dimopoulos, K., Owen, C., & Tenkanen, T. (2018). Primordial black hole formation during slow reheating after inflation. Physical Review D – Particles and Fields, 97, Article 123535. https://doi.org/10.1103/PhysRevD.97.123535

Vancouver

Carr B, Dimopoulos K, Owen C, Tenkanen T. Primordial black hole formation during slow reheating after inflation. Physical Review D – Particles and Fields. 2018 Jun 26;97:123535. doi: 10.1103/PhysRevD.97.123535

Author

Carr, Bernard ; Dimopoulos, Konstantinos ; Owen, Charlotte et al. / Primordial black hole formation during slow reheating after inflation. In: Physical Review D – Particles and Fields. 2018 ; Vol. 97.

Bibtex

@article{067308934cc24eb5ae930804061b2abf,
title = "Primordial black hole formation during slow reheating after inflation",
abstract = "We study the formation of primordial black holes (PBHs) in the early Universe during a period of slow reheating after inflation. We demonstrate how the PBH formation mechanism may change even before the end of the matter-dominated phase and calculate the expected PBH mass function. We find that there is a threshold for the variance of the density contrast, σ_c ≃ 0.05, below which the transition occurs even before reheating, with this having important consequences for the PBH mass function. We also show that there is a maximum cutoff for the PBH mass at around 100 M⊙, below which the subdominant radiation bath affects PBH production, making the scenario particularly interesting for the recent LIGO observations of black hole mergers.",
keywords = "primordial black holes, reheating",
author = "Bernard Carr and Konstantinos Dimopoulos and Charlotte Owen and Tommi Tenkanen",
year = "2018",
month = jun,
day = "26",
doi = "10.1103/PhysRevD.97.123535",
language = "English",
volume = "97",
journal = "Physical Review D – Particles and Fields",
issn = "2470-0010",
publisher = "American Physical Society",

}

RIS

TY - JOUR

T1 - Primordial black hole formation during slow reheating after inflation

AU - Carr, Bernard

AU - Dimopoulos, Konstantinos

AU - Owen, Charlotte

AU - Tenkanen, Tommi

PY - 2018/6/26

Y1 - 2018/6/26

N2 - We study the formation of primordial black holes (PBHs) in the early Universe during a period of slow reheating after inflation. We demonstrate how the PBH formation mechanism may change even before the end of the matter-dominated phase and calculate the expected PBH mass function. We find that there is a threshold for the variance of the density contrast, σ_c ≃ 0.05, below which the transition occurs even before reheating, with this having important consequences for the PBH mass function. We also show that there is a maximum cutoff for the PBH mass at around 100 M⊙, below which the subdominant radiation bath affects PBH production, making the scenario particularly interesting for the recent LIGO observations of black hole mergers.

AB - We study the formation of primordial black holes (PBHs) in the early Universe during a period of slow reheating after inflation. We demonstrate how the PBH formation mechanism may change even before the end of the matter-dominated phase and calculate the expected PBH mass function. We find that there is a threshold for the variance of the density contrast, σ_c ≃ 0.05, below which the transition occurs even before reheating, with this having important consequences for the PBH mass function. We also show that there is a maximum cutoff for the PBH mass at around 100 M⊙, below which the subdominant radiation bath affects PBH production, making the scenario particularly interesting for the recent LIGO observations of black hole mergers.

KW - primordial black holes

KW - reheating

U2 - 10.1103/PhysRevD.97.123535

DO - 10.1103/PhysRevD.97.123535

M3 - Journal article

VL - 97

JO - Physical Review D – Particles and Fields

JF - Physical Review D – Particles and Fields

SN - 2470-0010

M1 - 123535

ER -