Absorption and quasinormal modes of classical fields propagating on 3D and 4D de Sitter spacetime

We extensively study the exact solutions of the massless Dirac equation in 3D de Sitter spacetime that we published recently. Using the Newman-Penrose formalism, we find exact solutions of the equations of motion for the massless classical fields of spin s=1/2,1,2 and to the massive Dirac equation in 4D de Sitter metric. Employing these solutions, we analyze the absorption by the cosmological horizon and de Sitter quasinormal modes. We also comment on the results given by other authors.Comment: 31 page

Efeito da adição de trolox e pentoxifilina na motilidade, integridade do acrossoma e do DNA de espermatozoides equinos após descongelação Effect of trolox and pentoxifylline on motility and integrity of, acrossome and DNA of equine spermatozoa after thawing

Três garanhões foram utilizados para estudar o efeito da adição de trolox e pentoxifilina na motilidade, integridade do acrossoma e DNA de espermatozoides pós-descongelação. Para congelação, utilizou-se Tris-gema com glicerol (5%) em máquina de congelação de sêmen. As amostras foram descongeladas a 37ºC durante 30 segundos e tratadas com: T1= 150µL de sêmen + 150µL de Tris; T2= 150µL de sêmen + 150µL de Tris + 120µM/mL de trolox; T3= 150µL de sêmen + 150µL de Tris + 3,5mM de pentoxifilina e T4= 150µL de sêmen + 150µL de Tris + 3,5mM de pentoxifilina + 120µM/mL de trolox. Após 0, 60 e 120 minutos de incubação (37ºC), as amostras foram analisadas quanto à motilidade, vigor, integridade de acrossoma e DNA. Não houve diferença (P>0,05) entre tratamentos após 0 e 60 minutos de incubação em todos os parâmetros estudados. Após 120 minutos de incubação, verificou-se maior porcentual (P<0,05) de células com motilidade total e progressiva nas amostras do T2. Conclui-se que a adição de trolox após descongelação do sêmen equino preserva a motilidade total e progressiva dos espermatozoides submetidos à incubação a 37ºC durante 120 minutos.<br>Three stallions were used to study the effect of trolox and pentoxifylline addition on the motility and integrity of acrossome and DNA equine spermatozoa after thawing. Tris-egg-yolg diluent with glycerol (5%) were used to freeze the semen samples in a freezing machine. The samples were thawed at 37ºC during 30 seconds and treated with: T1=150µL of semen + 150µL of Tris; T2= 150µL of semen + 150µL of Tris +150mM/mL of trolox; T3= 150µL of semen + 150µL Tris +3.5mM of pentoxifylline; and T4= 150µL of semen + 150µL of Tris + 3.5mM of pentoxifylline + 150mM of trolox. After 0, 60, and 120 minutes of incubation (37ºC), the samples were analyzed to motility, vigor, and integrity of acrossome and DNA. There was no difference (P>0.05) among treatments considering 0 and 60 minutes of incubation in all studied parameters. After 120 minutes of incubation, it was observed higher percentage (P<0.05) of cells with total and progressive motility in the samples of T2. It can be concluded that the trolox addition after thawing of equine semen preserved total and progressive motility of the sperm incubated at 37ºC during 120 minutes

Ultralight vector dark matter search using data from the KAGRA O3GK run

International audienceAmong the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for $U(1)_{B-L}$ gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the $U(1)_{B-L}$ gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation time scale of DM

Ultralight vector dark matter search using data from the KAGRA O3GK run

International audienceAmong the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for $U(1)_{B-L}$ gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the $U(1)_{B-L}$ gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation time scale of DM

Ultralight vector dark matter search using data from the KAGRA O3GK run

International audienceAmong the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for $U(1)_{B-L}$ gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the $U(1)_{B-L}$ gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation time scale of DM

Ultralight vector dark matter search using data from the KAGRA O3GK run

International audienceAmong the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for $U(1)_{B-L}$ gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the $U(1)_{B-L}$ gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation time scale of DM

Observation of Gravitational Waves from the Coalescence of a 2.5−4.5 M⊙2.5-4.5~M_\odot Compact Object and a Neutron Star

International audienceWe report the observation of a coalescing compact binary with component masses $2.5-4.5~M_\odot$ and $1.2-2.0~M_\odot$ (all measurements quoted at the 90% credible level). The gravitational-wave signal GW230529_181500 was observed during the fourth observing run of the LIGO-Virgo-KAGRA detector network on 2023 May 29 by the LIGO Livingston Observatory. The primary component of the source has a mass less than $5~M_\odot$ at 99% credibility. We cannot definitively determine from gravitational-wave data alone whether either component of the source is a neutron star or a black hole. However, given existing estimates of the maximum neutron star mass, we find the most probable interpretation of the source to be the coalescence of a neutron star with a black hole that has a mass between the most massive neutron stars and the least massive black holes observed in the Galaxy. We estimate a merger rate density of $55^{+127}_{-47}~\text{Gpc}^{-3}\,\text{yr}^{-1}$ for compact binary coalescences with properties similar to the source of GW230529_181500; assuming that the source is a neutron star-black hole merger, GW230529_181500-like sources constitute about 60% of the total merger rate inferred for neutron star-black hole coalescences. The discovery of this system implies an increase in the expected rate of neutron star-black hole mergers with electromagnetic counterparts and provides further evidence for compact objects existing within the purported lower mass gap