10 research outputs found

    The 2020 Revision of the Puerto Rican Civil Code: A Brief Explanation of Major Changes

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    Puerto Rico is with Louisiana one of the two United States jurisdictions having kept the civil law tradition as the bedrock of its private law. One of the last Spanish colonies, Puerto Rico became a US Territory in 1899. The Spanish Civil Code was replaced by a Puerto Rican Civil Code in 1930. A revision process spanned over a period of 23 years, ending with the adoption of a new Civil Code in 2020. After a presentation of the revision process, this report presents and discusses the changes and innovations in family law, property, contractual obligations, torts, and successions, also discussing the transitory provisions. It focuses on changes. The report also shows that in order not to weaken the US inspired commercial legislation, Spanish-speaking Puerto Rico resisted a contemporary trend of merging the Commercial Code into the Civil Code

    Aplicación práctica de métodos estereológicos renales en modelos animales experimentales

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    The kidneys are vital organs responsible for excretion, fluid and electrolyte balance and hormone production. The nephrons are the kidney's functional and structural units. The number, size and distribution of the nephron components contain relevant information on renal function. Stereology is a branch of morphometry that applies mathematical principles to obtain three-dimensional information from serial, parallel and equidistant two-dimensional microscopic sections. Because of the complexity of stereological studies and the lack of scientific literature on the subject, the aim of this paper is to clearly explain, through animal models, the basic concepts of stereology and how to calculate the main kidney stereological parameters that can be applied in future experimental studies

    Currículo Educación Secundaria Obligatoria y relaciones entre sus elementos

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    Se recoge el articulado del Decreto 43/2015, de 10 de junio, por el que se regula la ordenación y se establece el currículo de Educación Secundaria Obligatoria en el Principado de Asturias, publicado en el BOPA (Boletín Oficial del Principado de Asturias) el 30 de junio de 2015. La publicación incluye además la metodología didáctica, los contenidos, los criterios de valuación y estándares de aprendizaje evaluables de las distintas materias troncales, específicas y de aquéllas de libre configuración autonómica, y el total de sesiones lectivas de las distintas asignaturas de los ciclos educativos de la Educación Secundaria Obligatoria.ES

    Currículo Bachillerato y relaciones entre sus elementos

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    Contiene el Decreto 42/2015, de 10 de junio, por el que se regula la ordenación y se establece el currículo del Bachillerato en el Principado de Asturias. Publicado en el BOPA (Boletín Oficial del Principado de Asturias) el 29 de junio de 2015. Incluye además, la metodología didáctica, los contenidos, los criterios de valuación y estándares de aprendizaje evaluables de las distintas materias troncales, específicas y de aquéllas de libre configuración autonómica, y el total de sesiones lectivas de las distintas asignaturas del Bachillerato.ES

    High-energy and ultra-high-energy neutrinos: A Snowmass white paper

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    Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years

    High-Energy and Ultra-High-Energy Neutrinos

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    Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years

    High-energy and ultra-high-energy neutrinos:A Snowmass white paper

    No full text
    Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years

    High-Energy and Ultra-High-Energy Neutrinos

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    International audienceAstrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years
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