11 research outputs found
Constraints on cosmic strings using data from the first Advanced LIGO observing run
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- Publication venue
- Publication date
- 01/01/2018
- Field of study
Cosmic strings are topological defects which can be formed in grand unified theory scale phase transitions in the early universe. They are also predicted to form in the context of string theory. The main mechanism for a network of Nambu-Goto cosmic strings to lose energy is through the production of loops and the subsequent emission of gravitational waves, thus offering an experimental signature for the existence of cosmic strings. Here we report on the analysis conducted to specifically search for gravitational-wave bursts from cosmic string loops in the data of Advanced LIGO 2015-2016 observing run (O1). No evidence of such signals was found in the data, and as a result we set upper limits on the cosmic string parameters for three recent loop distribution models. In this paper, we initially derive constraints on the string tension Gμ and the intercommutation probability, using not only the burst analysis performed on the O1 data set but also results from the previously published LIGO stochastic O1 analysis, pulsar timing arrays, cosmic microwave background and big-bang nucleosynthesis experiments. We show that these data sets are complementary in that they probe gravitational waves produced by cosmic string loops during very different epochs. Finally, we show that the data sets exclude large parts of the parameter space of the three loop distribution models we consider
Full band all-sky search for periodic gravitational waves in the O1 LIGO data
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- Publication venue
- Publication date
- 01/01/2018
- Field of study
We report on a new all-sky search for periodic gravitational waves in the frequency band 475–2000 Hz and with a frequency time derivative in the range of ½−1.0; þ0.1 × 10−8 Hz=s. Potential signals could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. This search uses the data from Advanced LIGO’s first observational run O1. No gravitational-wave signals were observed, and upper limits were placed on their strengths. For completeness, results from the separately published low-frequency search 20–475 Hz are included as well. Our lowest upper limit on worst-case (linearly polarized) strain amplitude h0 is ∼4 × 10−25 near 170 Hz, while at the high end of our frequency range, we achieve a worst-case upper limit of 1.3 × 10−24. For a circularly polarized source (most favorable orientation), the smallest upper limit obtained is ∼1.5 × 10−25
Surviving Sepsis Campaign: International guidelines for management of severe sepsis and septic shock: 2008
- Author
- A Bidani
- A Bufalari
- A Djillali
- A El-Nawawy
- A Esteban
- A Esteban
- A Evans
- A Kortgen
- A Kumar
- A Liberati
- A O'Brien
- A Pesenti
- A Quartin
- AB Nathens
- AD Brook
- AD Oxman
- AF Connors Jr
- AF Shorr
- AG Pittas
- AG Turpie
- AJ Pollard
- American Society of Anaesthesiologists Task Force on Blood Component Therapy
- American Thoracic Society
- AP Goldman
- AP Wheeler
- B Allolio
- B Gardlund
- B Goldstein
- B Jonghe De
- B Krafte-Jacobs
- B Levy
- B Misset
- B Regnier
- B. Taylor Thompson
- BA Shapiro
- BA Wills
- BE Kreger
- BL Warren
- BM Patel
- BP Markovitz
- BT Thompson
- C Guerin
- C Guerin
- C Martin
- C Martin
- C Richard
- C Ronco
- C Strange
- C Vinsonneau
- CA Lindsay
- CA Nieuwenhoven van
- Canadian Critical Care Trials Group and the Canadian Critical Care Society
- CF Pizarro
- Christian Brun-Buisson
- CJ Fernandes Jr
- CJ Friedman
- CJ Wiedermann
- CL Holmes
- CL Holmes
- CL Sprung
- CL Sprung
- CM Pierce
- CMJ Vandenbroucke-Grauls
- College of American Pathologists
- CS Bouman
- CS King
- CW Colwell Jr
- D Annane
- D Backer De
- D Backer De
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- L Brochard
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- Margaret M. Parker
- Maurene Harvey
- MB Amato
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- Mitchell M. Levy
- MJ Levy
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- ML Malbrain
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- MM Levy
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- MP Weinstein
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- MW Dunser
- MW Dunser
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- N Basso
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- N Safdar
- ND Ferguson
- NI Shapiro
- NM Dung
- NP Day
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- NP O'Grady
- NT Ngo
- O Agu
- O Yildiz
- OI Abdel-Wahab
- P Barton
- P Jolliet
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- PE Bollaert
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- R Bellomo
- R Bellomo
- R Bellomo
- R Booy
- R D'Amico
- R Dahan
- R Hatala
- R MacLaren
- R Redman
- R Stocker
- R. Phillip Dellinger
- RC Bone
- RC Bone
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- RG Branco
- RG Brower
- RH Bartlett
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- Richard Beale
- RK Kanter
- RL Mehta
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- Roman Jaeschke
- RP Dellinger
- RP Dellinger
- RP Dellinger
- RS Bresalier
- RS Watson
- S Finfer
- S Harvey
- S John
- S Kanji
- S Kanji
- S Magder
- S Masutani
- S Nadel
- S Ranjit
- S Trzeciak
- S Trzeciak
- Sean Townsend
- Selective Decontamination of the Digestive Tract Trialists' Collaborative Group
- SJ Finney
- SJ Mackenzie
- SK Pingleton
- SM Hollenberg
- SR Keeley
- ST Micek
- SX Zhou
- T Al-Kharrat
- T Sharshar
- T Weber
- T Yamazaki
- TE Stewart
- The Acute Respiratory Distress Syndrome Network
- The National Heart Lung, and Blood Institute ARDS Clinical Trials Network
- The Veterans Administration Systemic Sepsis Cooperative Study Group
- Thierry Calandra
- TJ Iberti
- TJ Parke
- UK Misra
- V Gasparovic
- VW Vanek
- VY Dombrovskiy
- W Geerts
- W Mauritz
- WH Geerts
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- WJ Lamm
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- WR McCabe
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- Y Kupfer
- Y Sakr
- Y Tulzo Le
- YY Han
- Publication venue
- Springer-Verlag
- Publication date
- 01/01/2007
- Field of study
SCOPUS: ar.jinfo:eu-repo/semantics/publishe
FIRST SEARCHES FOR OPTICAL COUNTERPARTS TO GRAVITATIONAL-WAVE CANDIDATE EVENTS
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- Ćwiek A.
- Ćwiok M.
- Publication venue
- Publication date
- 01/01/2014
- Field of study
During the LIGO and Virgo joint science runs in 2009-2010, gravitational wave (GW) data from three interferometer detectors were analyzed within minutes to select GW candidate events and infer their apparent sky positions. Target coordinates were transmitted to several telescopes for follow-up observations aimed at the detection of an associated optical transient. Images were obtained for eight such GW candidates. We present the methods used to analyze the image data as well as the transient search results. No optical transient was identified with a convincing association with any of these candidates, and none of the GW triggers showed strong evidence for being astrophysical in nature. We compare the sensitivities of these observations to several model light curves from possible sources of interest, and discuss prospects for future joint GW-optical observations of this type
A search for tensor, vector, and scalar polarizations in the stochastic gravitational-wave background
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- I
- I
- Magana and Magana-Sandoval I.
- Magana and Magee L.
- Marchesoni F.
- Travasso F.
- V
- V
- V
- V
- V
- V
- V
- Publication venue
- 'Cornell University Library'
- Publication date
- 01/01/2018
- Field of study
The detection of gravitational waves with Advanced LIGO and Advanced Virgo has enabled novel tests of general relativity, including direct study of the polarization of gravitational waves. While general relativity allows for only two tensor gravitational-wave polarizations, general metric theories can additionally predict two vector and two scalar polarizations. The polarization of gravitational waves is encoded in the spectral shape of the stochastic gravitational-wave background, formed by the superposition of cosmological and individually-unresolved astrophysical sources. Using data recorded by Advanced LIGO during its first observing run, we search for a stochastic background of generically-polarized gravitational waves. We find no evidence for a background of any polarization, and place the first direct bounds on the contributions of vector and scalar polarizations to the stochastic background. Under log-uniform priors for the energy in each polarization, we limit the energy-densities of tensor, vector, and scalar modes at 95% credibility to ΩT0<5.6×10−8, ΩV0<6.4×10−8, and ΩS0<1.1×10−7 at a reference frequency f0=25 Hz.by Anand Sengupta et al
On the Requirements for Successful GPS Spoofing Attacks
- Author
- A. A. and Shahriar
- A. A. and Vardaro
- A. and Ajith
- A. and Altin
- A. and Ananyeva
- A. and Anderson
- A. and Babak
- A. and Batch
- A. and Betzwieser
- A. and Bitossi
- A. and Bondu
- A. and Bradaschia
- A. and Brinkmann
- A. and Bulik
- A. and Buskulic
- A. and Chiummo
- A. and Chmiel
- A. and Clara
- A. and Collette
- A. and Cortese
- A. and Costa
- A. and Cunningham
- A. and Di Pace
- A. and Eggenstein
- A. and Ferrante
- A. and Frey
- A. and George
- A. and Gill
- A. and Gorodetsky
- A. and Graef
- A. and Gras
- A. and Gupta
- A. and Heintze
- A. and Hu
- A. and Korobko
- A. and Kuehn
- A. and Kwang
- A. and Lasky
- A. and Lazzaro
- A. and Leonardi
- A. and Maros
- A. and Martelli
- A. and Massinger
- A. and Matichard
- A. and Mendell
- A. and Mogushi
- A. and Munch
- A. and Nevin
- A. and Noack
- A. and Nocera
- A. and Pai
- A. and Pan
- A. and Papa
- A. and Parker
- A. and Passaquieti
- A. and Penn
- A. and Perri
- A. and Powell
- A. and Rapagnani
- A. and Rolland
- A. and Ruggi
- A. and Sammut
- A. and Schale
- A. and Schreiber
- A. and Shaddock
- A. and Shoemaker
- A. and Singhal
- A. and Sintes
- A. and Steinke
- A. and Sturani
- A. and Tasson
- A. and Torrie
- A. and Vedovato
- A. and Viets
- A. and Zanolin
- A. B. and Nissanke
- A. C. and Gretarsson
- A. D. and Singer
- A. D. and Vinciguerra
- A. E. and Page
- A. F. and Brown
- A. J. and Kennedy
- A. J. and Weiss
- A. J. K. and Chua
- A. K. and Staats
- A. K. W. and Chung
- A. L. and Miller
- A. L. and Summerscales
- A. L. and Usman
- A. M. and Slagmolen
- A. P. and Lynch
- A. P. and Srivastava
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- Publication venue
- Publication date
- 01/10/2011
- Field of study
An increasing number of wireless applications rely on GPS signals for localization, navigation, and time synchronization. However, civilian GPS signals are known to be susceptible to spoofing attacks which make GPS receivers in range believe that they reside at locations different than their real physical locations. In this paper, we investigate the requirements for successful GPS spoofing attacks on individuals and groups of victims with civilian or military GPS receivers. In particular, we are interested in identifying from which locations and with which precision the attacker needs to generate its signals in order to successfully spoof the receivers. We will show, for example, that any number of receivers can easily be spoofed to one arbitrary location; however, the attacker is restricted to only few transmission locations when spoofing a group of receivers while preserving their constellation. In addition, we investigate the practical aspects of a satellite-lock takeover, in which a victim receives spoofed signals after first being locked on to legitimate GPS signals. Using a civilian GPS signal generator, we perform a set of experiments and find the minimal precision of the attacker's spoofing signals required for covert satellite-lock takeover
GW170817: Measurements of neutron star radii and equation of state
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- Publication venue
- HAL CCSD
- Publication date
- 01/01/2018
- Field of study
International audienceOn 17 August 2017, the LIGO and Virgo observatories made the first direct detection of gravitational waves from the coalescence of a neutron star binary system. The detection of this gravitational-wave signal, GW170817, offers a novel opportunity to directly probe the properties of matter at the extreme conditions found in the interior of these stars. The initial, minimal-assumption analysis of the LIGO and Virgo data placed constraints on the tidal effects of the coalescing bodies, which were then translated to constraints on neutron star radii. Here, we expand upon previous analyses by working under the hypothesis that both bodies were neutron stars that are described by the same equation of state and have spins within the range observed in Galactic binary neutron stars. Our analysis employs two methods: the use of equation-of-state-insensitive relations between various macroscopic properties of the neutron stars and the use of an efficient parametrization of the defining function p(ρ) of the equation of state itself. From the LIGO and Virgo data alone and the first method, we measure the two neutron star radii as R1=10.8-1.7+2.0 km for the heavier star and R2=10.7-1.5+2.1 km for the lighter star at the 90% credible level. If we additionally require that the equation of state supports neutron stars with masses larger than 1.97 M⊙ as required from electromagnetic observations and employ the equation-of-state parametrization, we further constrain R1=11.9-1.4+1.4 km and R2=11.9-1.4+1.4 km at the 90% credible level. Finally, we obtain constraints on p(ρ) at supranuclear densities, with pressure at twice nuclear saturation density measured at 3.5-1.7+2.7×1034 dyn cm-2 at the 90% level
Б1.В.ДВ.2.1 ФОС Организация государственных учреждений
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- Publication venue
- Publication date
- 01/01/2018
- Field of study
International audienc
Tests of general relativity with GW170817
- Author
- A
- A
- A
- A. S
- Abbott B. P
- Abbott R
- Abbott T. D
- Abhirup and Ghosh
- Acernese F
- Ackley K
- Adams C
- Adams T
- Addesso P
- Adhikari R. X
- Adya V. B
- Affeldt C
- Agarwal B
- Agathos M
- Agatsuma K
- Aggarwal N
- Aguiar O. D
- Aiello L
- Ain A
- Ajith P
- Allen B
- Allen G
- Allocca A
- Aloy M. A
- Altin P. A
- Amato A
- Ananyeva A
- Anderson S. B
- Anderson W. G
- Angelova
- Antier S
- Appert S
- Arai K
- Araya M. C
- Archisman and Ghosh
- Areeda J. S
- Arene M
- Arnaud N
- Arun K. G
- Arunava and Mukherjee
- Ascenzi S
- Ashton G
- Ast M
- Aston S. M
- Astone P
- Atallah
- Aubin F
- Aufmuth P
- Aulbert C
- AultONeal K
- Austin C
- Avila-Alvarez A
- B
- B
- B
- Babak S
- Bacon P
- Badaracco F
- Bader M. K. M
- Bae S
- Baker P. T
- Baldaccini F
- Ballardin G
- Ballmer S. W
- Banagiri S
- Barayoga J. C
- Barclay S. E
- Barish B. C
- Barker D
- Barkett K
- Barnum S
- Barone F
- Barr B
- Barsotti L
- Barsuglia M
- Barta D
- Bartlett J
- Bartos
- Basti A
- Batch J. C
- Bawaj M
- Bayley J. C
- Bazzan M
- Becsy B
- Beer C
- Bejger M
- Belahcene
- Beniwal D
- Bensch M
- Berger B. K
- Bergmann G
- Bernuzzi S
- Bero J. J
- Berry C. P. L
- Bersanetti D
- Bertolini A
- Betzwieser J
- Bhandare R
- Bilenko I. A
- Bilgili S. A
- Billingsley G
- Billman C. R
- Birch J
- Birney R
- Birnholtz O
- Biscans S
- Biscoveanu S
- Bisht A
- Bitossi M
- Bizouard M. A
- Blackburn J. K
- Blackman J
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- Blair D. G
- Blair R. M
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- Boer M
- Boetzel Y
- Bogaert G
- Bohe A
- Bondu F
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- Publication venue
- 'American Physical Society (APS)'
- Publication date
- 01/01/2019
- Field of study
The recent discovery by Advanced LIGO and Advanced Virgo of a gravitational wave signal from a binary neutron star inspiral has enabled tests of general relativity (GR) with this new type of source. This source, for the first time, permits tests of strong-field dynamics of compact binaries in the presence of matter. In this Letter, we place constraints on the dipole radiation and possible deviations from GR in the post-Newtonian coefficients that govern the inspiral regime. Bounds on modified dispersion of gravitational waves are obtained; in combination with information from the observed electromagnetic counterpart we can also constrain effects due to large extra dimensions. Finally, the polarization content of the gravitational wave signal is studied. The results of all tests performed here show good agreement with GR.by Anand Sengupta et a
A gravitational-wave standard siren measurement of the Hubble constant
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- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- 01/01/2017
- Field of study
On 17 August 2017, the Advanced LIGO(1) and Virgo(2) detectors observed the gravitational-wave event GW170817-a strong signal from the merger of a binary neutron-star system(3). Less than two seconds after the merger, a gamma-ray burst (GRB 170817A) was detected within a region of the sky consistent with the LIGO-Virgo-derived location of the gravitational-wave source(4-6). This sky region was subsequently observed by optical astronomy facilities(7), resulting in the identification(8-13) of an optical transient signal within about ten arcseconds of the galaxy NGC 4993. This detection of GW170817 in both gravitational waves and electromagnetic waves represents the first ''multi-messenger'' astronomical observation. Such observations enable GW170817 to be used as a ''standard siren''(14-18) (meaning that the absolute distance to the source can be determined directly from the gravitational-wave measurements) to measure the Hubble constant. This quantity represents the local expansion rate of the Universe, sets the overall scale of the Universe and is of fundamental importance to cosmology. Here we report a measurement of the Hubble constant that combines the distance to the source inferred purely from the gravitational-wave signal with the recession velocity inferred from measurements of the redshift using the electromagnetic data. In contrast to previous measurements, ours does not require the use of a cosmic ''distance ladder''(19): the gravitational-wave analysis can be used to estimate the luminosity distance out to cosmological scales directly, without the use of intermediate astronomical distance measurements. We determine the Hubble constant to be about 70 kilometres per second per megaparsec. This value is consistent with existing measurements(20,21), while being completely independent of them. Additional standard siren measurements from future gravitational-wave sources will enable the Hubble constant to be constrained to high precision