Articles with "solar mass" as a keyword



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J1342+0928 supports the timeline in the R h = ct cosmology

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Published in 2018 at "Astronomy and Astrophysics"

DOI: 10.1051/0004-6361/201832752

Abstract: The discovery of quasar J1342+0928 (z=7.54) reinforces the time compression problem associated with the premature formation of structure in LCDM. Adopting the Planck parameters, we see this quasar barely 690 Myr after the big bang,… read more here.

Keywords: j1342 0928; cosmology; seed; solar mass ... See more keywords
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Tracking Advanced Planetary Systems (TAPAS) with HARPS-N

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Published in 2021 at "Astronomy and Astrophysics"

DOI: 10.1051/0004-6361/202037892

Abstract: We present the current status of and new results from our search for exoplanets in a sample of solar-mass, evolved stars observed with the HARPS-N and the 3.6-m Telescopio Nazionale Galileo (TNG), and the High… read more here.

Keywords: planetary systems; solar mass; mass; advanced planetary ... See more keywords
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Detectability of subsolar mass neutron stars through a template bank search

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Published in 2022 at "Physical Review D"

DOI: 10.1103/physrevd.107.103012

Abstract: We study the detectability of gravitational-wave signals from sub-solar mass binary neutron star systems by the current generation of ground-based gravitational-wave detectors. We find that finite size effects from large tidal deformabilities of the neutron… read more here.

Keywords: neutron stars; sub solar; solar mass; search ... See more keywords
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Methods for the detection of gravitational waves from subsolar mass ultracompact binaries

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Published in 2018 at "Physical Review D"

DOI: 10.1103/physrevd.98.103024

Abstract: We describe detection methods for extensions of gravitational wave searches to sub-solar mass compact binaries. Sub-solar mass searches were previously carried out using Initial LIGO, and Advanced LIGO boasts a detection volume approximately 1000 times… read more here.

Keywords: methods detection; sub solar; gravitational waves; solar mass ... See more keywords
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Test for the Origin of Solar Mass Black Holes.

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Published in 2021 at "Physical review letters"

DOI: 10.1103/physrevlett.126.071101

Abstract: Solar-mass black holes with masses in the range of ∼1-2.5  M_{⊙} are not expected from conventional stellar evolution, but can be produced naturally via neutron star (NS) implosions induced by capture of small primordial black holes… read more here.

Keywords: black holes; mass black; mass; bhs ... See more keywords