15 research outputs found
Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA
- Author
- Abbott
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- and Abbott R.
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- Casanueva and Casentini J.
- Cerboni and Cerretani L.
- Da Silva and Dattilo C. F.
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- Fernandez and Ferrante A.
- Gonzalez and Gopakumar J. M.
- Marchesoni F.
- R. and E. A.
- R. J
- Travasso F.
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- 01/01/2018
- Field of study
Get PDFWe present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron star systems, which are the most promising targets for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90% credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5– 20 deg2 requires at least three detectors of sensitivity within a factor of ∼2 of each other and with a broad frequency bandwidth. When all detectors, including KAGRA and the third LIGO detector in India, reach design sensitivity, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone
Search for eccentric binary black hole mergers with Advanced LIGO and Advanced Virgo during their first and second observing runs
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- Publication venue
- 'American Astronomical Society'
- Publication date
- 01/01/2019
- Field of study
Get PDFWhen formed through dynamical interactions, stellar-mass binary black holes (BBHs) may retain eccentric orbits (e > 0.1 at 10 Hz) detectable by ground-based gravitational-wave detectors. Eccentricity can therefore be used to differentiate dynamically formed binaries from isolated BBH mergers. Current template-based gravitational-wave searches do not use waveform models associated with eccentric orbits, rendering the search less efficient for eccentric binary systems. Here we present the results of a search for BBH mergers that inspiral in eccentric orbits using data from the first and second observing runs (O1 and O2) of Advanced LIGO and Advanced Virgo. We carried out the search with the coherent WaveBurst algorithm, which uses minimal assumptions on the signal morphology and does not rely on binary waveform templates. We show that it is sensitive to binary mergers with a detection range that is weakly dependent on eccentricity for all bound systems. Our search did not identify any new binary merger candidates. We interpret these results in light of eccentric binary formation models. We rule out formation channels with rates greater than about 100 Gpc−3 yr−1 for e > 0.1, assuming a black hole mass spectrum with a power-law index less than about 2
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A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo
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- Publication venue
- 'Organisation for Economic Co-Operation and Development (OECD)'
- Publication date
- 26/05/2021
- Field of study
Get PDFAbstract: This paper presents the gravitational-wave measurement of the Hubble constant (H 0) using the detections from the first and second observing runs of the Advanced LIGO and Virgo detector network. The presence of the transient electromagnetic counterpart of the binary neutron star GW170817 led to the first standard-siren measurement of H 0. Here we additionally use binary black hole detections in conjunction with galaxy catalogs and report a joint measurement. Our updated measurement is H 0 = 69−8+16 km s−1 Mpc−1 (68.3% of the highest density posterior interval with a flat-in-log prior) which is an improvement by a factor of 1.04 (about 4%) over the GW170817-only value of 69−8+17 km s−1 Mpc−1. A significant additional contribution currently comes from GW170814, a loud and well-localized detection from a part of the sky thoroughly covered by the Dark Energy Survey. With numerous detections anticipated over the upcoming years, an exhaustive understanding of other systematic effects are also going to become increasingly important. These results establish the path to cosmology using gravitational-wave observations with and without transient electromagnetic counterparts
A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo
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- Publication venue
- The Astrophysical Journal
- Publication date
- 10/03/2020
- Field of study
Get PDFAbstract: This paper presents the gravitational-wave measurement of the Hubble constant (H 0) using the detections from the first and second observing runs of the Advanced LIGO and Virgo detector network. The presence of the transient electromagnetic counterpart of the binary neutron star GW170817 led to the first standard-siren measurement of H 0. Here we additionally use binary black hole detections in conjunction with galaxy catalogs and report a joint measurement. Our updated measurement is H 0 = 69−8+16 km s−1 Mpc−1 (68.3% of the highest density posterior interval with a flat-in-log prior) which is an improvement by a factor of 1.04 (about 4%) over the GW170817-only value of 69−8+17 km s−1 Mpc−1. A significant additional contribution currently comes from GW170814, a loud and well-localized detection from a part of the sky thoroughly covered by the Dark Energy Survey. With numerous detections anticipated over the upcoming years, an exhaustive understanding of other systematic effects are also going to become increasingly important. These results establish the path to cosmology using gravitational-wave observations with and without transient electromagnetic counterparts
Recommended from our members
A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo
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- Publication venue
- The Astrophysical Journal
- Publication date
- 19/03/2021
- Field of study
Get PDFAbstract: This paper presents the gravitational-wave measurement of the Hubble constant (H 0) using the detections from the first and second observing runs of the Advanced LIGO and Virgo detector network. The presence of the transient electromagnetic counterpart of the binary neutron star GW170817 led to the first standard-siren measurement of H 0. Here we additionally use binary black hole detections in conjunction with galaxy catalogs and report a joint measurement. Our updated measurement is H 0 = 69−8+16 km s−1 Mpc−1 (68.3% of the highest density posterior interval with a flat-in-log prior) which is an improvement by a factor of 1.04 (about 4%) over the GW170817-only value of 69−8+17 km s−1 Mpc−1. A significant additional contribution currently comes from GW170814, a loud and well-localized detection from a part of the sky thoroughly covered by the Dark Energy Survey. With numerous detections anticipated over the upcoming years, an exhaustive understanding of other systematic effects are also going to become increasingly important. These results establish the path to cosmology using gravitational-wave observations with and without transient electromagnetic counterparts
Blood lead levels and male reproductive hormones: A systematic review and meta-analysis
- Author
- Ahamed
- Altman DG
- Assennato
- Assennato
- Atasoy
- Bero
- Bhavani Shankara Bagepally
- Bleecker
- Braunstein
- Catalani
- Centers for Disease C. and Prevention
- De Rosa
- Deeks
- DerSimonian
- Dobrakowski
- document Cl
- Doumouchtsis
- Egger
- Erfurth
- Gandhi
- Gennart
- Gill-Sharma
- Govoni
- Gustafson
- Haghighi
- Hermanns
- Hozo
- Jahan
- Kasperczyk
- Kumar
- Kuo
- Lucchini
- Madhumitha Haridoss
- Mahmoud
- McGregor
- Naha
- Naha
- Naha
- Naha
- Needleman Hl Fau-Landrigan
- Ng
- Nkomo
- Rakesh Balachandar
- Ramos-Trevino
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No full textXenobiotic mediated diabetogenesis: Developmental exposure to dichlorvos or atrazine leads to type 1 or type 2 diabetes in Drosophila
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No full textAnthrax vaccines: present status and future prospects
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- Centers for Disease Control and Prevention.
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No full textSearch for Subsolar Mass Ultracompact Binaries in Advanced LIGO's Second Observing Run
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- Zweizig J
- Publication venue
- 'American Physical Society (APS)'
- Publication date
- 01/01/2019
- Field of study
Get PDFWe present a search for subsolar mass ultracompact objects in data obtained during Advanced LIGO's second observing run. In contrast to a previous search of Advanced LIGO data from the first observing run, this search includes the effects of component spin on the gravitational waveform. We identify no viable gravitational-wave candidates consistent with subsolar mass ultracompact binaries with at least one component between 0.2 M-circle dot-1.0 M-circle dot. We use the null result to constrain the binary merger rate of (0.2 M-circle dot, 0.2 M-circle dot) binaries to be less than 3.7 x 10(5) Gpc(-3) yr(-1) and the binary merger rate of (1.0 M-circle dot, 1.0 M-circle dot) binaries to be less than 5.2 x 10(3) Gpc(-3) yr(-1). Subsolar mass ultracompact objects are not expected to form via known stellar evolution channels, though it has been suggested that primordial density fluctuations or particle dark matter with cooling mechanisms and/or nuclear interactions could form black holes with subsolar masses. Assuming a particular primordial black hole (PBH) formation model, we constrain a population of merging 0.2 M-circle dot black holes to account for less than 16% of the dark matter density and a population of merging 1.0 M-circle dot black holes to account for less than 2% of the dark matter density. We discuss how constraints on the merger rate and dark matter fraction may be extended to arbitrary black hole population models that predict subsolar mass binaries
All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run
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- Zweizig J
- Publication venue
- 'American Physical Society (APS)'
- Publication date
- 01/01/2019
- Field of study
Get PDFWe present the results of a search for short-duration gravitational-wave transients in the data from the second observing run of Advanced LIGO and Advanced Virgo. We search for gravitational-wave transients with a duration of milliseconds to approximately one second in the 32-4096 Hz frequency band with minimal assumptions about the signal properties, thus targeting a wide variety of sources. We also perform a matched-filter search for gravitational-wave transients from cosmic string cusps for which the waveform is well modeled. The unmodeled search detected gravitational waves from several binary black hole mergers which have been identified by previous analyses. No other significant events have been found by either the unmodeled search or the cosmic string search. We thus present the search sensitivities for a variety of signal waveforms and report upper limits on the source rate density as a function of the characteristic frequency of the signal. These upper limits are a factor of 3 lower than the first observing run, with a 50% detection probability for gravitational-wave emissions with energies of 3c10-9 Mc2 at 153 Hz. For the search dedicated to cosmic string cusps we consider several loop distribution models, and present updated constraints from the same search done in the first observing run
