English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Tools annual

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

We derive analytic expressions that provide Fourier domain gravitational wave(GW) response function for compact binaries inspiraling along moderatelyeccentric orbits. These expressions include amplitude corrections to the two GWpolarization states that are accurate to the first post-Newtonian (PN) order.Additionally, our fully 3PN accurate GW phase evolution incorporateseccentricity effects up to sixth order at each PN order. Further, we develop aprescription to incorporate analytically the effects of 3PN accurate periastronadvance in the GW phase evolution. This is how we provide a ready-to-use andefficient inspiral template family for compact binaries in moderately eccentricorbits. Preliminary GW data analysis explorations suggest that our templatefamily should be required to construct analytic inspiral-merger-ringdowntemplates to model moderately eccentric compact binary coalescence.

Ready-to-use Fourier domain templates for compact binaries inspiraling along moderately eccentric orbits