Methods and results of a search for gravitational waves associated with gamma-ray bursts using the GEO 600, LIGO, and Virgo detectors

In this paper we report on a search for short-duration gravitational wave bursts in the frequency range 64 Hz-1792 Hz associated with gamma-ray bursts (GRBs), using data from GEO 600 and one of the LIGO or Virgo detectors. We introduce the method of a linear search grid to analyze GRB events with large sky localization uncertainties, for example the localizations provided by the Fermi Gamma-ray Burst Monitor (GBM). Coherent searches for gravitational waves (GWs) can be computationally intensive when the GRB sky position is not well localized, due to the corrections required for the difference in arrival time between detectors. Using a linear search grid we are able to reduce the computational cost of the analysis by a factor of O(10) for GBM events. Furthermore, we demonstrate that our analysis pipeline can improve upon the sky localization of GRBs detected by the GBM, if a high-frequency GW signal is observed in coincidence. We use the method of the linear grid in a search for GWs associated with 129 GRBs observed satellite-based gamma-ray experiments between 2006 and 2011. The GRBs in our sample had not been previously analyzed for GW counterparts. A fraction of our GRB events are analyzed using data from GEO 600 while the detector was using squeezed-light states to improve its sensitivity; this is the first search for GWs using data from a squeezed-light interferometric observatory. We find no evidence for GW signals, either with any individual GRB in this sample or with the population as a whole. For each GRB we place lower bounds on the distance to the progenitor, under an assumption of a fixed GW emission energy of 10(-2)M circle dot c(2), with a median exclusion distance of 0.8 Mpc for emission at 500 Hz and 0.3 Mpc at 1 kHz. The reduced computational cost associated with a linear search grid will enable rapid searches for GWs associated with Fermi GBM events once the advanced LIGO and Virgo detectors begin operation.

Search for Gravitational Waves Associated with gamma-ray Bursts Detected by the Interplanetary Network

We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M(circle dot)c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.

The NINJA-2 project: detecting and characterizing gravitational waveforms modelled using numerical binary black hole simulations

The Numerical INJection Analysis (NINJA) project is a collaborative effort between members of the numerical relativity and gravitational-wave (GW) astrophysics communities. The purpose of NINJA is to study the ability to detect GWs emitted from merging binary black holes (BBH) and recover their parameters with next-generation GW observatories. We report here on the results of the second NINJA project, NINJA-2, which employs 60 complete BBH hybrid waveforms consisting of a numerical portion modelling the late inspiral, merger, and ringdown stitched to a post-Newtonian portion modelling the early inspiral. In a 'blind injection challenge' similar to that conducted in recent Laser Interferometer Gravitational Wave Observatory (LIGO) and Virgo science runs, we added seven hybrid waveforms to two months of data recoloured to predictions of Advanced LIGO (aLIGO) and Advanced Virgo (AdV) sensitivity curves during their first observing runs. The resulting data was analysed by GW detection algorithms and 6 of the waveforms were recovered with false alarm rates smaller than 1 in a thousand years. Parameter-estimation algorithms were run on each of these waveforms to explore the ability to constrain the masses, component angular momenta and sky position of these waveforms. We find that the strong degeneracy between the mass ratio and the BHs' angular momenta will make it difficult to precisely estimate these parameters with aLIGO and AdV. We also perform a large-scale Monte Carlo study to assess the ability to recover each of the 60 hybrid waveforms with early aLIGO and AdV sensitivity curves. Our results predict that early aLIGO and AdV will have a volume-weighted average sensitive distance of 300 Mpc (1 Gpc) for 10M circle dot + 10M circle dot (50M circle dot + 50M circle dot) BBH coalescences. We demonstrate that neglecting the component angular momenta in the waveform models used in matched-filtering will result in a reduction in sensitivity for systems with large component angular momenta. This reduction is estimated to be up to similar to 15% for 50M circle dot + 50M circle dot BBH coalescences with almost maximal angular momenta aligned with the orbit when using early aLIGO and AdV sensitivity curves.

Redox dysregulation and bioaccumulation of copper in tilapia Oreocromis niloticus

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Intraspecific, interspecific, and seasonal differences in the diet of three mid-sized carnivores in a large neotropical wetland

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Feasibility of RF Sputtering and PIIID for production of thin films from red mud

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Doença de Forestier: uma causa de disfagia a ser lembrada

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Parâmetros erosividade da chuva e da enxurrada correlacionados com as perdas de solo de um solo Bruno Não-Cálcico Vértico em Sumé (PB)

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Parâmetros erosividade da chuva, da enxurrada e da chuva-enxurrada correlacionados com as perdas de solo de um luvissolo

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Indicadores de stress e sobrecarga em cuidadores formais e informais de pacientes oncológicos

The present study aimed to identify the presence of indicators of stress, levels of stress and overload with the formal and informal caregivers of cancer patients. Participated in the survey 33 caregivers of cancer patients in total, 16 formal and 17 informal. To collect data, we used: 1) Roadmap for characterization of participants; 2) Inventory of Stress Symptoms Lipp - ISSL and 3) Protocol Zarit Burden Interview - ZBT. The results revealed that 43 % of informal carers were in the resistance phase, 29 % in the burnout stage, 14 % at the stage of exhaustion and almost 14 % in the alert phase. Formal caregivers 25 % are in the exhaustion phase and 75 % in the resistance. The overload has also performed on a larger scale in informal than formal caregivers, 47 % to 18,7 % charge respectively. However, the results revealed no statistically significant difference between groups for the incidence of stress but indicated a difference against overloading pointing out that professional caregivers in the incidence is lower. The results suggest the need to implement support for informal and formal caregivers programs, develop coping strategies, handling the situations of overload and stress, aiming to better quality of life for the caregiver, and consequently for the patient who is receiving care.

A educação de jovens e adultos: desafios de uma proposta de educação inclusiva: perfil do aluno

The inclusion of students with disabilities in youth and adult education is still new and there is little literature on the issue, which makes it both nationally relevant, and timely in the context of the construction of inclusive schools for all. The present study aimed to characterize the profile of the student of Youth and Adult Education in a medium size city of São Paulo, between the years 2011 and 2013. For the study documentary analysis was carried out using the Student Registration System of the State of São Paulo (PRODESP) for the study. A roadmap for the characterization of students was used, as a research instrument. It was possible to obtain data regarding the total enrolment per year, number of students with disabilities, types of disabilities, gender and age. Youth and Adult Education’s search for people with disabilities is increasing and accordingly, we observe that the target audience of YAE today has changed, including people with disabilities, indicating the need to consider development of teaching practices in line with the needs and demands of new YAE students.

Avaliação da sobrecarga em cuidadores familiares de pacientes de um Centro de Atenção Psicossocial

Com a reforma psiquiátrica o modelo de atenção à saúde mental sofreu transformações, retirando a centralização do poder do hospital psiquiátrico por meio da implantação de programas e serviços substitutivos de atenção e cuidado aos sujeitos em sofrimento psíquico, sendo que uma das principais estratégias adotadas é a consolidação dos Centros de Atenção Psicossocial. O retorno do sujeito ao convívio familiar após longos anos de internação coloca em questão a dificuldade do convívio social e familiar, assim como a retomada dos cuidados da família em relação a este. Assumir os cuidados de um paciente psiquiátrico pode gerar sobrecarga e muitas vezes, significa renunciar às próprias necessidades, projetos e desejos, colocando os do paciente/familiar em primeiro plano. A presente pesquisa tem por objetivo investigar a presença de indicadores de sobrecarga em cuidadores informais de pessoas com transtornos mentais atendidas em um Centro de Atenção Psicossocial - CAPS de um município do interior de São Paulo. Participaram da presente pesquisa 37 cuidadores informais de pessoas com transtornos mentais. Para coleta de dados foram utilizados dois instrumentos: um roteiro de entrevista para caracterização da amostra e o protocolo ZaritBurden Interview (ZBT) para avaliar a presença de indicadores de sobrecarga. Os dados foram analisados de acordo com os escores atribuídos no manual de aplicação da escala padronizada. Os resultados obtidos revelam o predomínio da sobrecarga moderada e modera da severa (78%), indicando a necessidade de intervenção junto aos cuidadores no sentido de desenvolver estratégias que favoreçam o cuidado e ao mesmo tempo preservem sua saúde.

A new tuning fork with different vibration frequencies as an aid to bronchopulmonary hygiene physiotherapy

Background: The main function of the mucociliary system is the removal of particles or substances that are potentially harmful to the respiratory tract. The tuning fork therapeutic for the purpose of bronchial hygiene has still not been described in the literature. The optimal vibration frequency to mobilize secretions is widely debated and varies between 3 and 25 Hz. It is expected that a tuning fork is able to generate vibrations in the thorax, facilitating bronchial hygiene. The aim of the present study is to develop tuning forks with different frequencies, for use in bronchopulmonary hygiene therapy. Methods: The first tuning fork was made with a fixed frequency of 25 Hz and it was recorded in the Brazilian institution of patent registration. This device generated a frequency of 25 Hz and had a weight of 521 g, with dimensions of 600 mm in total length. The device is characterized by a bottom end containing a transducer with a diameter of 62 mm and a thickness of 5/16 mm (8''), a rod removable 148 mm, fork length of 362 mm and an extension at the upper end of sinuous shape bilaterally.The tuning forks must be applied at an angle of 90° directly on the chest wall of the patient after pulmonary auscultation for location of secretions. The tuning fork is activated by squeezing the tips of the extensions together and releasing them in a sudden movement. Results: This study shows the result of the development of others three tuning forks of different dimensions to generate different frequencies. Each equipment reaches a fixed frequency preset of 12, 15 and 20 Hz measured by digital oscilloscope. Conclusions: The tuning fork models developed in this study generated different frequencies proposed by the scientific literature as effective in the mobilization of pulmonary secretions.