-
101por Georgescu, Iulia“…As the third LIGO–Virgo operating run (O3) finishes earlier than planned owing to the COVID-19 pandemic, we look at the ups and down of the past 12 months.…”
Publicado 2020
Enlace del recurso
Enlace del recurso
Enlace del recurso
Online Artículo Texto -
102por Badurina, Leonardo, Buchmueller, Oliver, Ellis, John, Lewicki, Marek, McCabe, Christopher, Vaskonen, Ville“…We compare the sensitivities of LIGO and LISA with those of the 100 m and 1 km stages of the AION terrestrial AI project, as well as two options for the proposed AEDGE AI space mission with cold atom clouds either inside or outside the spacecraft, considering as possible sources the mergers of black holes and neutron stars, supernovae, phase transitions in the early Universe, cosmic strings and quantum fluctuations in the early Universe that could have generated primordial black holes. …”
Publicado 2021
Enlace del recurso
Enlace del recurso
-
103por Giovannini, Massimo“…The obtained results are compared with the primary gravitational wave spectra of the concordance model and of its neighboring extensions as well as with the direct Ligo/Virgo bounds on stochastic backgrounds of relic gravitons. …”
Publicado 2010
Enlace del recurso
Enlace del recurso
-
104por Sperhake, Ulrich“…This observation by the LIGO interferometric detectors marks the dawn of a new era in our observational study of the cosmos as a qualitatively new window to its exploration has been opened. …”
Publicado 2016
Enlace del recurso
-
105por Hughes, Scott“…--HTML-->In the past year, the LIGO-Virgo Collaboration announced the first secure detection of gravitational waves. …”
Publicado 2016
Enlace del recurso
-
106por Mohanty, Subhendra“…Cosmology and astroparticle physics have seen an avalanche of discoveries in the past decade (IceCube - high energy neutrinos, LIGO - gravitational waves, Fermi- gamma-ray telescope, Xenon-1T - dark matter detection, PLANCK- cosmic microwave radiation, EHT picture of black hole, SDSS -galaxy surveys), all of which require a multidisciplinary background for analyzing the phenomena. …”
Publicado 2020
Enlace del recurso
Enlace del recurso
-
107“…This broad mass distribution of PBH as Dark Matter will be tested in the future by AdvLIGO and LISA interferometers.…”
Enlace del recurso
Enlace del recurso
-
108“…For GUT-scale string tensions, G$_{μ}$ ∼ 10$^{-8…-7}$, metastable strings predict a SGWB in the LIGO-Virgo-KAGRA band that could be discovered in the near future.…”
Enlace del recurso
Enlace del recurso
-
109por Bellomo, Nicola, Bertacca, Daniele, Jenkins, Alexander C., Matarrese, Sabino, Raccanelli, Alvise, Regimbau, Tania, Ricciardone, Angelo, Sakellariadou, Mairi“…We apply our numerical tools to robustly compute the angular power spectrum of the anisotropies of the gravitational wave background generated by astrophysical sources in the LIGO-Virgo frequency band. The end-to-end theoretical framework we present can be easily applied to different sources and detectors in other frequency bands. …”
Publicado 2021
Enlace del recurso
Enlace del recurso
-
110por Piga, Lorenzo, Lucca, Matteo, Bellomo, Nicola, Bosch-Ramon, Valentì, Matarrese, Sabino, Raccanelli, Alvise, Verde, Licia“…As a result, we show that the presence of such outflows introduces an additional layer of uncertainty that needs to be taken into account when quoting cosmological constraints on the PBH abundance, with important consequences in particular in the LIGO-Virgo-KAGRA observational window.…”
Publicado 2022
Enlace del recurso
Enlace del recurso
-
111por Metzger, Brian D.“…The coalescence of double neutron star (NS–NS) and black hole (BH)–NS binaries are prime sources of gravitational waves (GW) for Advanced LIGO/Virgo and future ground-based detectors. Neutron-rich matter released from such events undergoes rapid neutron capture (r-process) nucleosynthesis as it decompresses into space, enriching our universe with rare heavy elements like gold and platinum. …”
Publicado 2019
Enlace del recurso
Enlace del recurso
Enlace del recurso
Online Artículo Texto -
112por Banks, Hannah“…I will demonstrate that the cumulative signal from the inspirals of the LIGO-Virgo stellar-mass binaries is well within reach of typical terrestrial LBAI and may have much to reveal about the Universe. …”
Publicado 2023
Enlace del recurso
-
113por Porto, Rafael“…--HTML--><p>Abstract: </p> <p>The era of gravitational wave science began in spectacular fashion with several detections already reported by the LIGO-Virgo-KAGRA collaboration, and many more yet to come with the future planned observatories such as LISA and the Einstein Telescope. …”
Publicado 2022
Enlace del recurso
-
114por Iacovelli, Francesco“…--HTML-->Primordial Black Holes (PBH) have attracted much attention in the last years as they may explain some of the LIGO/Virgo/KAGRA observations and significantly contribute to the dark matter in our universe. …”
Publicado 2023
Enlace del recurso
-
115por Giudice, Gian F“…The LIGO observation of gravitational waves from a binary black hole merger has begun a new era in fundamental physics. …”
Publicado 2017
Enlace del recurso
Enlace del recurso
-
116“…The main theme of this review is a discussion of the mechanical and optical principles used in the various long baseline systems being built around the world — LIGO (USA), VIRGO (Italy/France), TAMA 300 (Japan) and GEO 600 (Germany/UK) — and in LISA, a proposed space-borne interferometer.…”
Enlace del recurso
Enlace del recurso
Enlace del recurso
Online Artículo Texto -
117“…We summarize present constraints and their impact on DE models, including those arising from the binary neutron star merger GW170817. Upgrades of LIGO-Virgo detectors to design sensitivity and the next generation facilities such as LISA or Einstein Telescope will significantly improve these constraints in the next two decades.…”
Enlace del recurso
Enlace del recurso
-
118“…The GW spectrum in this model would be detectable in the low-frequency range, e.g., by LISA, and in the mid-frequency range, e.g., by AION/MAGIS and AEDGE, and in the high-frequency range by LIGO and ET. The peak frequency of the signal is limited from below by collider constraints on the mass of the U(1)B−L gauge boson, while at high frequencies the slow decay of the scalar field and the resulting matter-dominated era diminishes the GW signal.…”
Enlace del recurso
Enlace del recurso
-
119
-
120“…Volume II provides an in-depth look at the Advanced LIGO and Advanced Virgo interferometers that have just finished construction, as well as examining future interferometric detector concepts. …”
Enlace del recurso