Resummation of the hadronic tau decay width with the modified Borel transform method

A modified Borel transform of the Adler function is used to resum the hadronic tau decay width ratio. In contrast to the ordinary Borel transform, the integrand of the Borel integral is renormalization--scale invariant. We use an ansatz which explicitly accounts for the structure of the leading infrared renormalon. Further, we use judiciously chosen conformal transformations for the Borel variable, in order to map sufficiently away from the origin the other ultraviolet and infrared renormalon singularities. In addition, we apply Pade approximants for the corresponding truncated perturbation series of the modified Borel transform, in order to further accelerate the convergence. Comparing the results with the presently available experimental data on the tau hadronic decay width ratio, we obtain $\alpha_s(M^z) = 0.1192 +- 0.0007_{exp.} +- 0.0010_{EW+CKM} +- 0.0009_{th.} +- 0.0003_{evol.}$. These predictions virtually agree with those of our previous resummations where we used ordinary Borel transforms instead.Comment: 32 pages, 2 eps-figures, revtex; minor changes in the formulations; a typo in Eq.(47) corrected; version as appearing in Phys. Rev.

Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3b

We search for gravitational-wave signals associated with gamma-ray bursts (GRBs) detected by the Fermi and Swift satellites during the second half of the third observing run of Advanced LIGO and Advanced Virgo (2019 November 1 15:00 UTC-2020 March 27 17:00 UTC). We conduct two independent searches: A generic gravitational-wave transients search to analyze 86 GRBs and an analysis to target binary mergers with at least one neutron star as short GRB progenitors for 17 events. We find no significant evidence for gravitational-wave signals associated with any of these GRBs. A weighted binomial test of the combined results finds no evidence for subthreshold gravitational-wave signals associated with this GRB ensemble either. We use several source types and signal morphologies during the searches, resulting in lower bounds on the estimated distance to each GRB. Finally, we constrain the population of low-luminosity short GRBs using results from the first to the third observing runs of Advanced LIGO and Advanced Virgo. The resulting population is in accordance with the local binary neutron star merger rate. © 2022. The Author(s). Published by the American Astronomical Society

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

Search for light long-lived neutral particles that decay to collimated pairs of leptons or light hadrons in pp collisions at s√ = 13 TeV with the ATLAS detector

A search for light long-lived neutral particles with masses in the O(MeV–GeV) range is presented. The analysis targets the production of long-lived dark photons in the decay of a Higgs boson produced via gluon–gluon fusion or in association with a W boson. Events that contain displaced collimated Standard Model fermions reconstructed in the calorimeter or muon spectrometer are selected in 139 fb−1 of s√ = 13 TeV pp collision data collected by the ATLAS detector at the LHC. Background estimates for contributions from Standard Model processes and instrumental effects are extracted from data. The observed event yields are consistent with the expected background. Exclusion limits are reported on the production cross-section times branching fraction as a function of the mean proper decay length cτ of the dark photon, or as a function of the dark-photon mass and kinetic mixing parameter that quantifies the coupling between the Standard Model and potential hidden (dark) sectors. A Higgs boson branching fraction above 1% is excluded at 95% CL for a Higgs boson decaying into two dark photons for dark-photon mean proper decay lengths between 10 mm and 250 mm and dark photons with masses between 0.4 GeV and 2 GeV

Efeito do estresse climático sobre os parâmetros produtivos e fisiológicos de ovinos Santa Inês mantidos em confinamento na região litorânea do Nordeste do Brasil Effects of environmental stress on physiological parameters of feedlot sheep in the Northeast of Brazil

O presente estudo foi conduzido objetivando-se avaliar a influência do estresse climático sobre o desempenho produtivo e as respostas fisiológicas de ovinos da raça Santa Inês em confinamento. Foram avaliados dois ambientes (sombra e sol) e duas dietas com duas relações volumoso:concentrado (70C:30V: 70% de concentrado e 30% de volumoso; 30C:70V: 30% de concentrado e 70% de volumoso). Os animais mantidos à sombra e alimentados com dieta contendo alto teor de concentrado (70C:30V) apresentaram maior consumo de matéria seca (1258 g/animal/dia) e de proteína bruta (0,8% do peso vivo [PV] e 18 g/PV0,75) e maior ganho de peso (247 g/animal/dia). A temperatura nos ambientes de sol e sombra durante a tarde foi de 32,1 e 30,6:C e os valores do índice de temperatura e umidade (ITU), 82,3 e 81,1, respectivamente. Os animais alimentados com alto teor de concentrado (70C:30V) apresentaram maior freqüência respiratória (FR), tanto à sombra quanto ao sol (87 e 71 mov/min, respectivamente). Durante a tarde, a temperatura retal (TR) dos animais foi maior (39,1:C) que pela manhã (38,9:C). Porém, a TR mais elevada (39,3:C) foi observada nos animais mantidos à sombra e alimentados com alto percentual de concentrado (70C:30V). Independentemente do ambiente, os animais alimentados com alto teor de concentrado (70C:30V) apresentaram maior TR (39,2:C) do que aqueles alimentados com reduzido teor de concentrado (30C:70V) (38,8:C). O tipo de dieta teve efeito sobre a susceptibilidade dos animais ao estresse causado pelas condições ambientais críticas durante o experimento. Os animais da raça Santa Inês mostraram-se sensíveis ao estresse ambiental, uma vez que apresentaram menor desempenho produtivo, quando expostos a condições de ausência de sombra.<br>A study was conducted to determine the effect of environmental stress on physiological criteria of feedlot sheep. Treatments consisted of two different housing conditions (shade and no shade) and two levels of concentrate in the diet: high concentrate (70% of concentrate and 30% of roughage-70C:30R); low concentrate (30% of concentrate and 70% of roughage-30C:70R). Animals raised under shade and fed a high concentrate diet (70C:30R) had greater dry mater intake (1258 g/animal/day) and crude protein (0.8% of body weight (BW) and 18 g/BW0.75), as well as weight gain (247 g/animal/day). Air temperature in the afternoon was 30.6:C, under shade, and 32.1:C, under sun and values of temperature humidity index(THI), 82.3 and 81.1, respectively. Animals fed more concentrate (70C:30R) had also higher respiratory frequency (RF), either raised under shade (87 mov/min) or under the sun (71 mov/min.). Rectal temperature (RT) was higher in the afternoon (39.1:C) than in the morning (38.9:C), but animals raised under shade and fed diets with 70% concentrate (70C:30R) had the highest value of RT (39.3:C). Regardless of type of housing conditions, the animals that received more concentrate (70C:30R) had greater rectal temperature (39.2:C) than those fed a diet with less concentrate (30C:70R) (38.8:C). Therefore, the type of diet influenced the response of the animals to housing conditions. Moreover, Santa Inês sheep are susceptible to environmental stress because had lower performance when raised under no shade