TY - JOUR
T1 - Black holes as “time capsules”
T2 - A cosmological graviton background and the Hubble tension
AU - Piran, Tsvi
AU - Jimenez, Raul
N1 - Publisher Copyright:
© 2023 The Authors. Astronomische Nachrichten published by Wiley-VCH GmbH.
PY - 2023/1/1
Y1 - 2023/1/1
N2 - Minuscule primordial black holes (BHs) before the end and after inflation can serve as “time capsules” bringing back energy from the past to a later epoch when they evaporate. As these BHs behave like matter, while the rest of the universe's content behaves like radiation, the mass fraction of these BHs, which is tiny at formation, becomes significant later. If sufficiently small, these BHs will evaporate while the Universe is still radiation dominated. We revisit this process and point out that gravitons produced during evaporation behave as “dark radiation.” If the initial BHs are uniformly distributed so will the gravitons and in this case, they will be free of Silk damping and avoid current limits on “dark radiation” scenarios. Seeds for such BHs can arise during the last phases of inflation. We show here that with suitable parameters, this background graviton field can resolve the Hubble tension. We present current observational constraints on this scenario and suggest upcoming observational tests to prove or refute it. Finally, we also elaborate on the graviton background produced by particle annihilation during the Planck era or shortly after inflation.
AB - Minuscule primordial black holes (BHs) before the end and after inflation can serve as “time capsules” bringing back energy from the past to a later epoch when they evaporate. As these BHs behave like matter, while the rest of the universe's content behaves like radiation, the mass fraction of these BHs, which is tiny at formation, becomes significant later. If sufficiently small, these BHs will evaporate while the Universe is still radiation dominated. We revisit this process and point out that gravitons produced during evaporation behave as “dark radiation.” If the initial BHs are uniformly distributed so will the gravitons and in this case, they will be free of Silk damping and avoid current limits on “dark radiation” scenarios. Seeds for such BHs can arise during the last phases of inflation. We show here that with suitable parameters, this background graviton field can resolve the Hubble tension. We present current observational constraints on this scenario and suggest upcoming observational tests to prove or refute it. Finally, we also elaborate on the graviton background produced by particle annihilation during the Planck era or shortly after inflation.
UR - http://www.scopus.com/inward/record.url?scp=85148459444&partnerID=8YFLogxK
U2 - 10.1002/asna.20230033
DO - 10.1002/asna.20230033
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AN - SCOPUS:85148459444
SN - 0004-6337
VL - 344
JO - Astronomische Nachrichten
JF - Astronomische Nachrichten
IS - 1-2
M1 - e230033
ER -