16 research outputs found

    Search for gravitational-lensing signatures in the full third observing run of the LIGO-Virgo network

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    Gravitational lensing by massive objects along the line of sight to the source causes distortions of gravitational wave-signals; such distortions may reveal information about fundamental physics, cosmology and astrophysics. In this work, we have extended the search for lensing signatures to all binary black hole events from the third observing run of the LIGO--Virgo network. We search for repeated signals from strong lensing by 1) performing targeted searches for subthreshold signals, 2) calculating the degree of overlap amongst the intrinsic parameters and sky location of pairs of signals, 3) comparing the similarities of the spectrograms amongst pairs of signals, and 4) performing dual-signal Bayesian analysis that takes into account selection effects and astrophysical knowledge. We also search for distortions to the gravitational waveform caused by 1) frequency-independent phase shifts in strongly lensed images, and 2) frequency-dependent modulation of the amplitude and phase due to point masses. None of these searches yields significant evidence for lensing. Finally, we use the non-detection of gravitational-wave lensing to constrain the lensing rate based on the latest merger-rate estimates and the fraction of dark matter composed of compact objects

    Observation of gravitational waves from the coalescence of a 2.5−4.5 M⊙ compact object and a neutron star

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    Search for eccentric black hole coalescences during the third observing run of LIGO and Virgo

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    Despite the growing number of confident binary black hole coalescences observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Orbital eccentricity is one of the clearest tracers of binary formation channels. Identifying binary eccentricity, however, remains challenging due to the limited availability of gravitational waveforms that include effects of eccentricity. Here, we present observational results for a waveform-independent search sensitive to eccentric black hole coalescences, covering the third observing run (O3) of the LIGO and Virgo detectors. We identified no new high-significance candidates beyond those that were already identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total mass M>70 M⊙) binaries covering eccentricities up to 0.3 at 15 Hz orbital frequency, and use this to compare model predictions to search results. Assuming all detections are indeed quasi-circular, for our fiducial population model, we place an upper limit for the merger rate density of high-mass binaries with eccentricities 0<e≤0.3 at 0.33 Gpc−3 yr−1 at 90\% confidence level

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

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    Among 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

    Eficiencia de mercado en la bolsa chilena

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    Tesis (Ingeniero en Administración de Empresas)"El mercado de capitales es un conjunto de mercados formales e informales formado por instituciones e instrumentos de financiación e inversión. En estos mercados existe transferencia de recursos desde aquellos agentes económicos que tienen superávit de recursos financieros hacia aquellos que necesitan cubrir déficit de recursos financieros . Por esta razón el mercado de capitales es esencial para asignar eficientemente los recursos de ahorro hacia los distintos proyectos de inversión que crean empleo y riqueza para los chilenos. En los últimos años, el mercado de capitales chileno ha experimentado un fuerte crecimiento gracias a un conjunto de políticas económicas que se han implementado, constituyendo una defensa contra las turbulencias financieras sufridas recientemente en los mercados internacionales. La hipótesis de los mercados eficientes tiene importantes implicaciones para la teoría financiera, tanto en el contexto de los mercados financieros y las decisiones de los inversores individuales, como en el ámbito de la dirección financiera de la empresa. Si los mercados son eficientes, los precios reflejan toda la información disponible sobre el valor intrínseco de cada título, protegiendo al inversor de los posibles efectos perjudiciales que se podrían dar por falta de conocimiento o experiencia sobre el funcionamiento del mercado. Es así como un mercado eficiente es un mercado equitativo en el que todos los inversores, especializados o no, tienen el mismo grado de información y, por tanto, tienen las mismas posibilidades de ganar o perder. La predicción en el cambio de precios siempre ha sido un tema de gran importancia en el estudio de las finanzas, esto se refleja en la hipótesis de la caminata aleatoria, el cual indica que el movimiento de precios de los activos financieros es imprevisible o recorre un camino aleatorio, es decir, no hay ninguna tendencia perceptible en el movimiento de los activos. Si esta tendencia existiera, los inversores podrían utilizarla para poder obtener beneficios extraordinarios. Esto nos llevaría a la problemática de la eficiencia de mercado, la cual indica que este tipo de mercado es clave para la determinación del precio real de los activos, así las empresas y los inversionistas deberán esperar recibir solo un precio justo por los activos financieros que se ponen en venta en el mercado. El mejor indicador de un mercado de capitales es su grado de liquidez, un mayor grado de liquidez se traduce en primer lugar en una reducción del riesgo de no poder liquidar la inversión. Así también, una mayor liquidez genera una externalidad positiva puesto que genera una mayor confianza en el mercado como indicador del verdadero valor de las empresas y una menor probabilidad de enfrentar abusos y manipulaciones de precios. La mayor liquidez y la confianza en el mercado se retroalimentan mutuamente en un círculo virtuoso. Lo anterior nos lleva a preguntar ¿Existe eficiencia de mercado en la Bolsa Chilena? El presente Seminario de Título pretende estudiar y analizar esta interrogante, para ello se investigaran las Normas, Organismos y Marco Regulatorio del Mercado de Capitales chileno. Además, en este mismo sentido nos enfocaremos en la Bolsa de Comercio de Santiago de Chile, por que es ella la que concentra históricamente la organización del Mercado de Valores en Chile. En segundo punto, analizaremos el complemento de lo descrito anteriormente a través de una de las maneras en que se manifiesta la eficiencia de mercado a través del Test de los Signos, Test de Hurst, Test Durbin Watson y el Test Kolmogorov-Smimov. Todo esto nos dará una aproximación para saber si existe eficiencia de mercado en la Bolsa de Comercio de Santiago

    Longitudinal assessment of bacterial vaginosis prior to and during incident pregnancy: an observational study in Kenyan adolescent girls and young women

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    Objective To determine bacterial vaginosis (BV) status at multiple time points among adolescent girls and young women (AGYW) and assess the impact of pregnancy on their BV status.Design Longitudinal cohort study.Setting Thika, Kenya.Participants AGYW aged 16–20 years enrolled prior to first sex or reporting only a single lifetime partner.Main outcome measures The primary outcome was relative risk (RR) of BV during pregnancy compared with before pregnancy by analysing longitudinal trends in BV over time. BV risk was estimated using Poisson regression models.Results A total of 121 AGYW became pregnant in the parent cohort and had BV results before, during or after pregnancy. Point prevalence of BV was 11.0% at visits >12 months pre-pregnancy, 13.0% at 3–12 months pre-pregnancy, 22.1% at <3 months pre-pregnancy and 13.4% during pregnancy. Compared with visits during pregnancy, RR of BV was 1.65 (95% CI: 1.00 to 2.71; p=0.05) at visits <3 months pre-pregnancy, 0.97 (95% CI: 0.62 to 1.52; p=0.90) at visits 3–12 months pre-pregnancy and 0.82 (95% CI: 0.44 to 1.53; p=0.53) at visits 12 months pre-pregnancy. An adjusted analysis including age, income, residence, date of first sex, recent sexual activity and positive sexually transmitted infection test resulted in small changes in risk estimates, with adjusted RR of BV of 1.66 (95% CI: 1.04 to 2.67; p=0.04) at visits <3 months pre-pregnancy compared with visits during pregnancy.Conclusions BV risk during pregnancy was lower than during the immediate pre-pregnancy period. Hormonal changes in pregnancy may reduce BV
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