FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2156317737> ?p ?o ?g. }

• W2156317737 abstract "Compact binaries that emit gravitational waves in the sensitivity band of ground-based detectors can have non-negligible eccentricities just prior to merger, depending on the formation scenario. We develop a purely analytic, frequency-domain model for gravitational waves emitted by compact binaries on orbits with small eccentricity, which reduces to the quasicircular post-Newtonian approximant TaylorF2 at zero eccentricity and to the postcircular approximation of Yunes et al. [Phys. Rev. D 80, 084001 (2009)] at small eccentricity. Our model uses a spectral approximation to the (post-Newtonian) Kepler problem to model the orbital phase as a function of frequency, accounting for eccentricity effects up to $mathcal{O}({e}^{8})$ at each post-Newtonian order. Our approach accurately reproduces an alternative time-domain eccentric waveform model for $eensuremath{in}[0,0.4]$ and binaries with total mass $ensuremath{lesssim}12{M}_{ensuremath{bigodot}}$. As an application, we evaluate the signal amplitude that eccentric binaries produce in different networks of existing and forthcoming gravitational waves detectors. Assuming a population of eccentric systems containing black holes and neutron stars that is uniformly distributed in comoving volume, we estimate that second-generation detectors like Advanced LIGO could detect approximately 0.1--10 events per year out to redshift $zensuremath{sim}0.2$, while an array of Einstein Telescope detectors could detect hundreds of events per year to redshift $zensuremath{sim}2.3$." @default.
• W2156317737 created "2016-06-24" @default.
• W2156317737 creator A5028335452 @default.
• W2156317737 creator A5048208658 @default.
• W2156317737 creator A5049074853 @default.
• W2156317737 creator A5052196996 @default.
• W2156317737 creator A5087296933 @default.
• W2156317737 date "2014-10-10" @default.
• W2156317737 modified "2023-10-17" @default.
• W2156317737 title "Accurate and efficient waveforms for compact binaries on eccentric orbits" @default.
• W2156317737 cites W1968795474 @default.
• W2156317737 cites W1973432807 @default.
• W2156317737 cites W1974291788 @default.
• W2156317737 cites W1974500985 @default.
• W2156317737 cites W1976222774 @default.
• W2156317737 cites W1976463280 @default.
• W2156317737 cites W1977459118 @default.
• W2156317737 cites W1977991023 @default.
• W2156317737 cites W1979733958 @default.
• W2156317737 cites W1987873991 @default.
• W2156317737 cites W1988355552 @default.
• W2156317737 cites W1990289273 @default.
• W2156317737 cites W1994021934 @default.
• W2156317737 cites W1994489827 @default.
• W2156317737 cites W2006230071 @default.
• W2156317737 cites W2008384093 @default.
• W2156317737 cites W2010268662 @default.
• W2156317737 cites W2012291066 @default.
• W2156317737 cites W2014664612 @default.
• W2156317737 cites W2016784890 @default.
• W2156317737 cites W2019114691 @default.
• W2156317737 cites W2019208447 @default.
• W2156317737 cites W2020219205 @default.
• W2156317737 cites W2020704736 @default.
• W2156317737 cites W2028815006 @default.
• W2156317737 cites W2029341305 @default.
• W2156317737 cites W2032715249 @default.
• W2156317737 cites W2033427105 @default.
• W2156317737 cites W2034856282 @default.
• W2156317737 cites W2042781085 @default.
• W2156317737 cites W2042865319 @default.
• W2156317737 cites W2044789805 @default.
• W2156317737 cites W2045565446 @default.
• W2156317737 cites W2045624689 @default.
• W2156317737 cites W2045943684 @default.
• W2156317737 cites W2049699970 @default.
• W2156317737 cites W2055220676 @default.
• W2156317737 cites W2058420621 @default.
• W2156317737 cites W2059751355 @default.
• W2156317737 cites W2061243145 @default.
• W2156317737 cites W2063480122 @default.
• W2156317737 cites W2064816908 @default.
• W2156317737 cites W2069063499 @default.
• W2156317737 cites W2069557347 @default.
• W2156317737 cites W2076844555 @default.
• W2156317737 cites W2077580067 @default.
• W2156317737 cites W2077590995 @default.
• W2156317737 cites W2081587002 @default.
• W2156317737 cites W2081895114 @default.
• W2156317737 cites W2083484739 @default.
• W2156317737 cites W2087010948 @default.
• W2156317737 cites W2087059232 @default.
• W2156317737 cites W2087168055 @default.
• W2156317737 cites W2088749022 @default.
• W2156317737 cites W2090689468 @default.
• W2156317737 cites W2094575668 @default.
• W2156317737 cites W2101084132 @default.
• W2156317737 cites W2106532428 @default.
• W2156317737 cites W2112341471 @default.
• W2156317737 cites W2112596327 @default.
• W2156317737 cites W2116789044 @default.
• W2156317737 cites W2117464438 @default.
• W2156317737 cites W2117598186 @default.
• W2156317737 cites W2128789238 @default.
• W2156317737 cites W2128789282 @default.
• W2156317737 cites W2128936003 @default.
• W2156317737 cites W2140058367 @default.
• W2156317737 cites W2140328803 @default.
• W2156317737 cites W2141835750 @default.
• W2156317737 cites W2144088263 @default.
• W2156317737 cites W2154444782 @default.
• W2156317737 cites W2156112894 @default.
• W2156317737 cites W2157763730 @default.
• W2156317737 cites W2157908049 @default.
• W2156317737 cites W2160855100 @default.
• W2156317737 cites W2160971573 @default.
• W2156317737 cites W2162549314 @default.
• W2156317737 cites W2162656068 @default.
• W2156317737 cites W2163068820 @default.
• W2156317737 cites W2164150189 @default.
• W2156317737 cites W2168505566 @default.
• W2156317737 cites W2174458751 @default.
• W2156317737 cites W2175159557 @default.
• W2156317737 cites W2593722288 @default.
• W2156317737 cites W2599113008 @default.
• W2156317737 cites W2963086359 @default.
• W2156317737 cites W3098797633 @default.
• W2156317737 cites W3098821728 @default.
• W2156317737 cites W3099186672 @default.
• W2156317737 cites W3099691601 @default.

• next