FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4313332384> ?p ?o ?g. }

• W4313332384 abstract "Recent population studies have searched for a subpopulation of primordial black holes (PBHs) in the gravitational-wave (GW) events so far detected by LIGO/Virgo/KAGRA (LVK), in most cases adopting a phenomenological PBH mass distribution. When deriving such population from first principles in the standard scenario, however, the equation of state of the Universe at the time of PBH formation may strongly affect the PBH abundance and mass distribution, which ultimately depend on the power spectrum of cosmological perturbations. Here we improve on previous population studies on several aspects: (i) we adopt state-of-the-art PBH formation models describing the collapse of cosmological perturbations across the QCD epoch; (ii) we perform the first Bayesian multi-population inference on GW data including PBHs and directly using power spectrum parameters instead of phenomenological distributions; (iii) we critically confront the PBH scenario with LVK phenomenological models describing the GWTC-3 catalog both in the neutron-star and in the BH mass ranges, also considering PBHs as subpopulation of the total events. Our results confirm that LVK observations prevent the majority of the dark matter to be in the form of stellar mass PBHs. We find that the best fit PBH model can comprise a small fraction of the total events, in particular it can naturally explain events in the mass gaps. If the lower mass-gap event GW190814 is interpreted as a PBH binary, we predict that LVK should detect up to a few subsolar mergers and one to $approx 30$ lower mass gap events during the upcoming O4 and O5 runs. Finally, mapping back the best-fit power spectrum into an ultra slow-roll inflationary scenario, we show that the latter predicts detectable PBH mergers in the LVK band, a stochastic GW background detectable by current and future instruments, and may include the entirety of dark matter in asteroid-mass PBHs." @default.
• W4313332384 created "2023-01-06" @default.
• W4313332384 creator A5016911084 @default.
• W4313332384 creator A5036764767 @default.
• W4313332384 creator A5046178863 @default.
• W4313332384 creator A5070365050 @default.
• W4313332384 date "2022-12-29" @default.
• W4313332384 modified "2023-10-17" @default.
• W4313332384 title "From inflation to black hole mergers and back again: Gravitational-wave data-driven constraints on inflationary scenarios with a first-principle model of primordial black holes across the QCD epoch" @default.
• W4313332384 cites W1134494461 @default.
• W4313332384 cites W1509168094 @default.
• W4313332384 cites W1517784139 @default.
• W4313332384 cites W1638753340 @default.
• W4313332384 cites W1640843629 @default.
• W4313332384 cites W1749804791 @default.
• W4313332384 cites W1965202898 @default.
• W4313332384 cites W1969823825 @default.
• W4313332384 cites W1973852867 @default.
• W4313332384 cites W1974098534 @default.
• W4313332384 cites W1983380408 @default.
• W4313332384 cites W1983471014 @default.
• W4313332384 cites W1996004845 @default.
• W4313332384 cites W1998388948 @default.
• W4313332384 cites W1999809938 @default.
• W4313332384 cites W2005783817 @default.
• W4313332384 cites W2016770316 @default.
• W4313332384 cites W2018252185 @default.
• W4313332384 cites W2039930002 @default.
• W4313332384 cites W2041390637 @default.
• W4313332384 cites W2047402280 @default.
• W4313332384 cites W2050287430 @default.
• W4313332384 cites W2051694884 @default.
• W4313332384 cites W2055558232 @default.
• W4313332384 cites W2057037672 @default.
• W4313332384 cites W2058841045 @default.
• W4313332384 cites W2062182342 @default.
• W4313332384 cites W2062470943 @default.
• W4313332384 cites W2063498033 @default.
• W4313332384 cites W2065805883 @default.
• W4313332384 cites W2065913386 @default.
• W4313332384 cites W2075228395 @default.
• W4313332384 cites W2081835848 @default.
• W4313332384 cites W2082497072 @default.
• W4313332384 cites W2084112171 @default.
• W4313332384 cites W2096367114 @default.
• W4313332384 cites W2111818973 @default.
• W4313332384 cites W2131213682 @default.
• W4313332384 cites W2141106168 @default.
• W4313332384 cites W2150408793 @default.
• W4313332384 cites W2157427998 @default.
• W4313332384 cites W2159350339 @default.
• W4313332384 cites W2166472966 @default.
• W4313332384 cites W2256095203 @default.
• W4313332384 cites W2289010674 @default.
• W4313332384 cites W2322170955 @default.
• W4313332384 cites W2330523759 @default.
• W4313332384 cites W2481968765 @default.
• W4313332384 cites W2512413576 @default.
• W4313332384 cites W2551138164 @default.
• W4313332384 cites W2559835926 @default.
• W4313332384 cites W2562346410 @default.
• W4313332384 cites W2564153216 @default.
• W4313332384 cites W2566112626 @default.
• W4313332384 cites W2591485485 @default.
• W4313332384 cites W2616219306 @default.
• W4313332384 cites W2736993946 @default.
• W4313332384 cites W2754075545 @default.
• W4313332384 cites W2754382496 @default.
• W4313332384 cites W2757338357 @default.
• W4313332384 cites W2762521314 @default.
• W4313332384 cites W2765081049 @default.
• W4313332384 cites W2766013620 @default.
• W4313332384 cites W2781084618 @default.
• W4313332384 cites W2783576719 @default.
• W4313332384 cites W2787174546 @default.
• W4313332384 cites W2787820091 @default.
• W4313332384 cites W2788563157 @default.
• W4313332384 cites W2789206622 @default.
• W4313332384 cites W2789797553 @default.
• W4313332384 cites W2801940103 @default.
• W4313332384 cites W2804915303 @default.
• W4313332384 cites W2809734150 @default.
• W4313332384 cites W2809820731 @default.
• W4313332384 cites W2810661833 @default.
• W4313332384 cites W2857345734 @default.
• W4313332384 cites W2886963303 @default.
• W4313332384 cites W2891084346 @default.
• W4313332384 cites W2891865365 @default.
• W4313332384 cites W2891993472 @default.
• W4313332384 cites W2898313720 @default.
• W4313332384 cites W2898584704 @default.
• W4313332384 cites W2902744094 @default.
• W4313332384 cites W2903375752 @default.
• W4313332384 cites W2905116979 @default.
• W4313332384 cites W2905384843 @default.
• W4313332384 cites W2913239535 @default.
• W4313332384 cites W2920511893 @default.
• W4313332384 cites W2921425065 @default.
• W4313332384 cites W2929819542 @default.
• W4313332384 cites W2930873487 @default.

• next