{"arxiv_id":"2009.03363","incoming":{"papers":31,"sentences":55,"groups":[{"kind":"comparison","label":"Compares with it","papers":1,"sentences":3,"quotes":[{"arxiv_id":"2406.08728","title":"Exploring Faraday rotation signatures and population bounds for primordial magnetic black holes","url":"/paper/2406.08728","section":"Summary and conclusions","sentence":"Although Parker-type bounds on MBHs have previously been explored —for instance, from galactic magnetic fields [ref] , yielding a limit on their dark matter fraction $f_DM ≲𝒪(10^-3)$— we find that constraints from cosmic void and cosmic filament magnetic fields provide novel and more stringent bounds on the dark matter fraction than those extant in the literature [ref] .","intent_p":0.93,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":15,"sentences":19,"quotes":[{"arxiv_id":"2406.08728","title":"Exploring Faraday rotation signatures and population bounds for primordial magnetic black holes","url":"/paper/2406.08728","section":"Theoretical framework for Parker-type bounds","sentence":"This concept forms the essence of Parker bounds and has been widely employed in previous studies [ref] .","intent_p":0.85,"contests_p":null},{"arxiv_id":"2210.15564","title":"Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Hyperbolic orbits on a cone","url":"/paper/2210.15564","section":"Introduction","sentence":"Recently, there has been an increasing interest in charged BHs; see Refs. [ref] and references therein.","intent_p":0.94,"contests_p":null},{"arxiv_id":"2307.07553","title":"Parker Bounds on Monopoles with Arbitrary Charge from Galactic and Primordial Magnetic Fields","url":"/paper/2307.07553","section":"Introduction","sentence":"The phenomenology of black holes with magnetic charge has recently been discussed in [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"2209.06060","title":"Stability and Observability of Magnetic Primordial Black Hole-Neutron Star Collisions","url":"/paper/2209.06060","section":"Introduction","sentence":"Some recent works have discussed observable astrophysical signatures of magnetically charged BHs [ref] .","intent_p":0.92,"contests_p":null},{"arxiv_id":"2504.09304","title":"Black holes with electroweak hair -- the detailed derivation","url":"/paper/2504.09304","section":"INTRODUCTION","sentence":"Following this scenario, various aspects of magnetic black holes have been discussed, but always at a phenomenological level [ref] .","intent_p":0.94,"contests_p":null}]}],"unlabelled_sentences":33},"outgoing":{"papers":56,"sentences":117,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":4,"sentences":4,"quotes":[{"arxiv_id":"0810.3114","title":"Evolution of magnetic fields in galaxies and future observational tests with the Square Kilometre Array","url":"/paper/0810.3114","section":"Quantum field theoretic and phenomenological aspects of MBH","sentence":"Note that the above bounds on the DM fraction are derived assuming parameter values corresponding to Andromeda galaxy (M31), for which $l_c = 10 kpc$, $t_reg = 10 Gyr$, $ρ_DM = 0.4 GeV/cm^3$ and $v = 10^-3c$ [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"1208.5712","title":"Stellar mass map and dark matter distribution in M31","url":"/paper/1208.5712","section":"Quantum field theoretic and phenomenological aspects of MBH","sentence":"Note that the above bounds on the DM fraction are derived assuming parameter values corresponding to Andromeda galaxy (M31), for which $l_c = 10 kpc$, $t_reg = 10 Gyr$, $ρ_DM = 0.4 GeV/cm^3$ and $v = 10^-3c$ [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"astro-ph/0110390","title":"LCDM-based models for the Milky Way and M31 I: Dynamical Models","url":"/paper/astro-ph/0110390","section":"Quantum field theoretic and phenomenological aspects of MBH","sentence":"Note that the above bounds on the DM fraction are derived assuming parameter values corresponding to Andromeda galaxy (M31), for which $l_c = 10 kpc$, $t_reg = 10 Gyr$, $ρ_DM = 0.4 GeV/cm^3$ and $v = 10^-3c$ [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"astro-ph/0310258","title":"The magnetic field of M31 from multi-wavelength radio polarization observations","url":"/paper/astro-ph/0310258","section":"Quantum field theoretic and phenomenological aspects of MBH","sentence":"Note that the above bounds on the DM fraction are derived assuming parameter values corresponding to Andromeda galaxy (M31), for which $l_c = 10 kpc$, $t_reg = 10 Gyr$, $ρ_DM = 0.4 GeV/cm^3$ and $v = 10^-3c$ [ref] .","intent_p":0.99,"contests_p":null}]},{"kind":"comparison","label":"Compares with","papers":1,"sentences":2,"quotes":[{"arxiv_id":"2007.03703","title":"Phenomenology of Magnetic Black Holes with Electroweak-Symmetric Coronas","url":"/paper/2007.03703","section":"Summary and conclusions","sentence":"Within astrophysical and modelling uncertainties, our results are consistent with the seminal result found in [ref] .","intent_p":0.95,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":28,"sentences":42,"quotes":[{"arxiv_id":"2007.03703","title":"Phenomenology of Magnetic Black Holes with Electroweak-Symmetric Coronas","url":"/paper/2007.03703","section":"Quantum field theoretic and phenomenological aspects of MBH","sentence":"A comprehensive exploration of the phenomenology of MBHs, with electroweak coronas, in this low-mass region is presented in [ref] .","intent_p":0.83,"contests_p":null},{"arxiv_id":"2008.02326","title":"Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Circular orbits on a cone","url":"/paper/2008.02326","section":"Introduction","sentence":"The effective one-body motion of a dyonic black hole binary system, along with some aspects of the corresponding electromagnetic and gravitational radiation, incorporating post-Newtonian corrections, was studied recently in [ref] .","intent_p":0.88,"contests_p":null},{"arxiv_id":"2006.14628","title":"How does a dark compact object ringdown?","url":"/paper/2006.14628","section":"Summary and conclusions","sentence":"An understanding of these aspects [ref] is especially pertinent in the broader context of understanding the nature of dark compact objects [ref] .","intent_p":0.93,"contests_p":null},{"arxiv_id":"1904.05363","title":"Testing the nature of dark compact objects: a status report","url":"/paper/1904.05363","section":"Summary and conclusions","sentence":"An understanding of these aspects [ref] is especially pertinent in the broader context of understanding the nature of dark compact objects [ref] .","intent_p":0.93,"contests_p":null},{"arxiv_id":"1307.1628","title":"A Population of Fast Radio Bursts at Cosmological Distances","url":"/paper/1307.1628","section":"Electromagnetic emissions from MBH binary inspirals","sentence":"Fast Radio Bursts [ref] are mysterious, radio transients that last for $𝒪(1) ms$, whose origins are not currently understood.","intent_p":0.9,"contests_p":null}]}],"unlabelled_sentences":69},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":null,"_links":{"html":"https://pith.science/paper/2009.03363"}}