Metodologia para germinação de sementes de Leonurus sibiricus L Methodology for Leonurus sibiricus L. seed germination

O objetivo do trabalho foi investigar a influência de diferentes temperaturas, o comportamento fotoblástico e a absorção de água de sementes de Leonurus sibiricus L. Essa espécie medicinal é originária da Índia, distribuída pela Ásia, África e América, utilizada no tratamento de reumatismo, problemas dermatológicos e respiratórios. Para tanto, as sementes foram submetidas a temperaturas entre 5 a 40ºC, com intervalos de 5ºC, e alternadas de 20/30, 20/25 e 25/30ºC, com 5 repetições de 50 sementes cada, em condições de luz e escuro. No estudo da absorção de água as sementes foram colocadas para germinar na temperatura de 20ºC e na presença da luz e pesadas para avaliar o ganho de água durante todo o processo germinativo, até a protrusão da radícula. Pelos resultados verificou-se que os maiores porcentuais de germinação e índice de velocidade de germinação ocorreram na temperatura constante de 20ºC, e nas temperaturas alternadas 20/25, 25/30, 25/30ºC sob luz. Houve germinação na temperatura mínima de 10ºC e na máxima 40ºC. No ensaio de absorção de água verificou-se que as sementes iniciam a protrusão da radícula com 65 horas de exposição e seguem padrão trifásico na curva de absorção. O modelo estatístico ajustado para a espécie foi y = 1,869 (1 - 0,414 exp ( -0,201t) + exp [-2,397 + 0,037 (t - 65)], com R²= 0,9998.<br>The aim of this study was to investigate the influence of different temperatures on the photoblastic response and water uptake of Leonurus sibiricus L. seeds. This medicinal species is from India and has been distributed over Asia, Africa and America, where it is used in the treatment of rheumatic, dermatological and respiratory disorders. Thus, seeds were subjected to temperatures between 5 and 40ºC, at 5ºC intervals, and 20/30, 20/25 and 25/30ºC alternate temperatures, with five replicates of 50 seeds each, under light and dark conditions. In the study of water uptake, seeds were allowed to germinate at 20ºC under light and weighed throughout the germinative process until radicle protrusion. The highest germination percentage and speed index were detected at 20ºC constant temperature and at 20/25, 25/30 and 25/30ºC alternate temperatures under light. There was germination at 10ºC (minimum temperature) and at 40ºC (maximum temperature). The study on water uptake showed that seeds began radicle protrusion at 65h exposure and follow the triphasic pattern in the uptake curve. The statistical model fit for the species was y = 1.869 (1 - 0.414 exp (-0.201 t) + exp [-2.397 + 0.037 (t - 65)], R² = 0.9998

Search for multimessenger sources of gravitational waves and high-energy neutrinos with Advanced LIGO during its first observing run, ANTARES, and IceCube

Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta