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- Between approximately 50 and 130 solar massesIn the standard picture of stellar evolution, pair-instability -- the energy loss in stellar cores due to electron-positron pair production -- is predicted to prevent the collapse of massive stars into black holes with mass in the range between approximately 50 and 130 solar masses -- a range known as the " {em black hole mass gap}".
arxiv.org/abs/2208.08557 - People also ask
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See all on WikipediaFor very high-mass stars, with mass at least 130 and up to perhaps roughly 250 solar masses, a true pair-instability supernova can occur. In these stars, the first time that conditions support pair production instability, the situation runs out of control. See more
A pair-instability supernova is a type of supernova predicted to occur when pair production, the production of free electrons and positrons in the collision between atomic nuclei and energetic gamma rays, temporarily reduces … See more
For a star to undergo pair-instability supernova, the increased creation of positron/electron pairs by gamma ray collisions must … See more
Luminosity
Pair-instability supernovae are popularly thought to be highly luminous. This is only the case for the most … See morePhoton emission
Photons given off by a body in thermal equilibrium have a black-body spectrum with an energy … See moreSeveral sources describe the stellar behavior for large stars in pair-instability conditions.
Below 100 solar masses
Gamma rays … See moreSome supernovae candidates for classification as pair-instability supernovae include:
• See moreWikipedia text under CC-BY-SA license WEBMar 14, 2021 · Stellar evolution theory predicts a "gap" in the black hole birth function caused by the pair instability. Presupernova stars that have a core mass below some …
- Author: S. E. Woosley, Alexander Heger
- Publish Year: 2021
WEBMay 11, 2021 · Stellar evolution theory predicts a "gap" in the black hole birth function caused by the pair instability.
- Author: S. E. Woosley, Alexander Heger
- Publish Year: 2021
WEBMay 1, 2021 · Stellar evolution theory predicts a "gap" in the black hole birth function caused by the pair instability. Many presupernova stars that have a core mass below some …
- Author: S. E. Woosley, Alexander Heger
- Publish Year: 2021
WEBDec 21, 2022 · For these physical conditions, thermal energy is converted into mass of electron-positron pairs. Depending on the CO core mass, this sudden lack of thermal …
WEBMar 14, 2021 · Stellar evolution theory predicts a “gap” in the black hole birth function caused by the pair instability.
WEBAbstract. Standard stellar evolution models predict that black holes in the range of approximately 50. 140M should. not exist directly from stellar evolution. This gap …
WEBStellar evolution theory predicts a "gap"in the black hole birth function caused by the pair instability. Many presupernova stars that have a core mass below some limiting value, …
WEBMay 1, 2021 · These “super-kilonovae” (superKNe) herald the birth of massive black holes ≳ 60 M ⊙ , which—as a result of disk wind mass loss—can populate the pair-instability …
WEBAug 17, 2021 · We propose a new method to populate the BH mass gap. If an energy source is added throughout the star in addition to nuclear fusion, it is possible for the …
WEBIn standard stellar evolution, stars with masses ranging from approximately 150 to 240M are expected to evolve to a pair instability supernova with no black hole (BH) remnant. …
Formation of black holes in the pair-instability mass gap ...
WEBApr 7, 2022 · The detection of the binary black hole merger GW190521, with primary black hole mass $85^ {+21}_ {-14}$ $ {\rm M}_ {\odot}$, proved the existence of black holes in …
WEBAbstract The recent detection of GW190521 stimulated ideas on how to populate the predicted black hole (BH) pair- instability (PI) mass gap. One proposal is the …
The effect of pair-instability mass loss on black-hole mergers
WEBOct 18, 2016 · Abstract. 1. Introduction. 2. Pair-instability: pulsation supernovae and supernovae. 3. Model. 4. Mass of single BHs and BH-BH mergers. 5. BH-BH merger …
Hierarchical mergers of stellar-mass black holes and their
WEBJul 26, 2021 · Such a subpopulation of hierarchically assembled black holes presents distinctive gravitational-wave signatures, namely higher masses, possibly within the pair …
Binary black holes in the pair instability mass gap
WEBJul 13, 2020 · Pair instability (PI) and pulsational PI prevent the formation of black holes (BHs) with mass ≳60 M ⊙ from single star evolution. Here, we investigate the possibility …
WEBStellar evolution theory predicts a “gap” in the black hole birth function caused by the pair instability. Many presupernova stars that have a core mass below some limiting value, M
WEBA mechanism known as pair-instability (PI) supernova is expected to prevent the formation of black holes from stellar collapse with mass greater than 40 65 M and less than 120 M …
[2208.08557] Dark Black Holes in the Mass Gap - arXiv.org
WEBAug 17, 2022 · In the standard picture of stellar evolution, pair-instability -- the energy loss in stellar cores due to electron-positron pair production -- is predicted to prevent the …
Mind the Gap: The Location of the Lower Edge of the Pair …
WEBDec 10, 2019 · Theory predicts the existence of a gap in the BH mass distribution because of pair-instability supernovae. The maximum BH mass below the gap is the result of …
Mechanism for nonnuclear energy to fill in the black hole mass …
WEBMay 31, 2024 · In the standard picture of stellar evolution, pair-instability — the energy loss in stellar cores due to electron-positron pair production — is predicted to prevent …
[1911.01434] Binary black holes in the pair-instability mass gap
WEBNov 4, 2019 · Pair instability (PI) and pulsational PI prevent the formation of black holes (BHs) with mass M from single star evolution. Here, we investigate the possibility that …
Detection of LIGO-Virgo binary black holes in the pair-instability …
WEBOct 4, 2021 · A mechanism known as pair-instability (PI) supernova is expected to prevent the formation of black holes from stellar collapse with mass greater than ∼40–65 M ⊙ …
Mechanism for nonnuclear energy to fill in the black hole mass …
WEBThis gap appears because stars with masses between 100 and 240 M ⊙ are expected to undergo a pair instability supernova and leave behind no remnant, or a pulsational pair …
WEBPair instability (PI) and pulsational PI prevent the formation of black holes (BHs) with mass > 60 M from single star evolution. Here, we investigate the possibility that BHs with …
Related searches for pair instability mass gap
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