Narrowband Searches for Continuous and Long-duration Transient Gravitational Waves from Known Pulsars in the LIGO-Virgo Third Observing Run

Isolated neutron stars that are asymmetric with respect to their spin axis are possible sources of detectable continuous gravitational waves. This paper presents a fully coherent search for such signals from eighteen pulsars in data from LIGO and Virgo's third observing run (O3). For known pulsars, efficient and sensitive matched-filter searches can be carried out if one assumes the gravitational radiation is phase-locked to the electromagnetic emission. In the search presented here, we relax this assumption and allow both the frequency and the time derivative of the frequency of the gravitational waves to vary in a small range around those inferred from electromagnetic observations. We find no evidence for continuous gravitational waves, and set upper limits on the strain amplitude for each target. These limits are more constraining for seven of the targets than the spin-down limit defined by ascribing all rotational energy loss to gravitational radiation. In an additional search, we look in O3 data for long-duration (hours-months) transient gravitational waves in the aftermath of pulsar glitches for six targets with a total of nine glitches. We report two marginal outliers from this search, but find no clear evidence for such emission either. The resulting duration-dependent strain upper limits do not surpass indirect energy constraints for any of these targets. © 2022. The Author(s). Published by the American Astronomical Society

Constraints on the cosmic expansion history from GWTC–3

We use 47 gravitational wave sources from the Third LIGO–Virgo–Kamioka Gravitational Wave Detector Gravitational Wave Transient Catalog (GWTC–3) to estimate the Hubble parameter H(z), including its current value, the Hubble constant H0. Each gravitational wave (GW) signal provides the luminosity distance to the source, and we estimate the corresponding redshift using two methods: the redshifted masses and a galaxy catalog. Using the binary black hole (BBH) redshifted masses, we simultaneously infer the source mass distribution and H(z). The source mass distribution displays a peak around 34 M⊙, followed by a drop-off. Assuming this mass scale does not evolve with the redshift results in a H(z) measurement, yielding ${H}_{0}={68}_{-8}^{+12}\,\mathrm{km}\ \,\ {{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$ (68% credible interval) when combined with the H0 measurement from GW170817 and its electromagnetic counterpart. This represents an improvement of 17% with respect to the H0 estimate from GWTC–1. The second method associates each GW event with its probable host galaxy in the catalog GLADE+, statistically marginalizing over the redshifts of each event's potential hosts. Assuming a fixed BBH population, we estimate a value of ${H}_{0}={68}_{-6}^{+8}\,\mathrm{km}\ \,\ {{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$ with the galaxy catalog method, an improvement of 42% with respect to our GWTC–1 result and 20% with respect to recent H0 studies using GWTC–2 events. However, we show that this result is strongly impacted by assumptions about the BBH source mass distribution; the only event which is not strongly impacted by such assumptions (and is thus informative about H0) is the well-localized event GW190814

Composição florística de pastagem natural afetada por fontes de fósforo, calagem e introdução de espécies forrageiras de estação fria Botanical composition of natural pasture as afected by phosphorus sources, lime and introduction of winter forage species

Uma das características das pastagens naturais do Rio Grande do Sul é a baixa produtividade de forragem no período do outono-inverno. Uma das alternativas para melhorar os sistemas de produção baseados nessas pastagens é a introdução de espécies forrageiras de crescimento inverno-primaveril e a fertilização e correção da acidez do solo. O presente trabalho teve por objetivo avaliar o efeito de fontes de fósforo, calcário e introdução de espécies forrageiras de inverno na dinâmica das espécies de uma pastagem natural. Os tratamentos testados foram: T1 - superfosfato simples + calcário + introdução de espécies; T2 - superfosfato triplo + calcário + introdução de espécies; T3 - superfosfato triplo + introdução de espécies; T4 - hiperfosfato de Gafsa + introdução de espécies; T5 - introdução de espécies sem fósforo ou calagem; T6 - testemunha com pastagem natural. Para a avaliação da composição florística da pastagem foram realizados levantamentos botânicos periódicos, durante vinte e dois meses, utilizando-se o método BOTANAL. Os resultados mostraram que os tratamentos testados não provocaram mudanças na composição botânica das espécies nativas no período de tempo avaliado.<br>Natural pastures of Rio Grande do Sul State, South of Brazil, have low forage productivity in the autumn-winter. An alternative to improve systems based on these pastures is introduction of winter forage species, fertilization and liming of soil. The present work had the objective of evaluating the effect of phosphorus sources, lime and introduction of winter forage species in the pasture botanical composition dynamics. The treatments used were: T1 - simple superphosphate + lime + winter forage species introduction; T2 - triple superphosphate + lime + winter forage species introduction; T3 - triple superphosphate + winter forage species introduction; T4 - Gafsa rock phosphate + winter forage species introduction; T5 - winter forage species introduction without phosphorus and lime; T6 - reference only with natural pasture. To evaluate the botanical composition dynamics, periodic botanical evaluations were done during twenty two months, using BOTANAL method. The results showed that treatments did not modify the botanical composition of natural pasture during the evaluation period