Women's views of a fertility awareness and hormonal support approach to subfertility

The aim of this study was to determine the satisfaction among subfertile women of a fertility awareness-based approach, including hormonal therapy to achieve a pregnancy by natural conception. Eighty four women attending a natural fertility service completed a postal questionnaire exploring (1) the acceptability of the sympto-thermal method and (2) the acceptability of using hormone support. Acceptability rates for the fertility charting, clinical service and clinical care were 64.9-91.6%. Acceptability rates were higher in women who did conceive or had experienced past recurrent miscarriages. Taking hormonal luteal support, by any method, was more acceptable for women over 35 years compared to those under 35 years (100% vs. 69.4%, p = 0.014). Vaginal pessaries were the preferred route of administration. The use of a fertility awareness-based method appears to be acceptable amongst subfertile women intending to conceive naturally. Most women using such a method for conception would be open to the use of hormonal support during the fertility cycle or early pregnancy

Search for intermediate-mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo

International audienceIntermediate-mass black holes (IMBHs) span the approximate mass range 100−105 M⊙, between black holes (BHs) that formed by stellar collapse and the supermassive BHs at the centers of galaxies. Mergers of IMBH binaries are the most energetic gravitational-wave sources accessible by the terrestrial detector network. Searches of the first two observing runs of Advanced LIGO and Advanced Virgo did not yield any significant IMBH binary signals. In the third observing run (O3), the increased network sensitivity enabled the detection of GW190521, a signal consistent with a binary merger of mass ∼150 M⊙ providing direct evidence of IMBH formation. Here, we report on a dedicated search of O3 data for further IMBH binary mergers, combining both modeled (matched filter) and model-independent search methods. We find some marginal candidates, but none are sufficiently significant to indicate detection of further IMBH mergers. We quantify the sensitivity of the individual search methods and of the combined search using a suite of IMBH binary signals obtained via numerical relativity, including the effects of spins misaligned with the binary orbital axis, and present the resulting upper limits on astrophysical merger rates. Our most stringent limit is for equal mass and aligned spin BH binary of total mass 200 M⊙ and effective aligned spin 0.8 at 0.056 Gpc−3 yr−1 (90% confidence), a factor of 3.5 more constraining than previous LIGO-Virgo limits. We also update the estimated rate of mergers similar to GW190521 to 0.08 Gpc−3 yr−1.Key words: gravitational waves / stars: black holes / black hole physicsCorresponding author: W. Del Pozzo, e-mail: [email protected]† Deceased, August 2020