62 research outputs found

    Testing the gravitational phenomenology of compact objects: superradiance, scalarization and screening mechanisms

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    In the last decades, an interesting variety of extended models of gravity has been proposed with the goal of capturing cosmological effects such as the accelerated phases of expansion and/or the so-called "dark sector" of our universe. In parallel, the quest for a full-fledged theory of quantum gravity proceeds by investigating the low-energy limit of candidate models. Many of these modified gravity models might leave imprints in the physics of compact objects and with gravitational-wave astronomy we have the unprecedented opportunity to test them against data with improving accuracy. A popular class of models (scalar-tensor theories) extends the field content of general relativity with an additional scalar field. These theories provide multiple examples where black hole and neutron star physics deviates from general relativity and can be constrained with observations. In this sense, superradiance and spontaneous growth of scalar fields around black holes and neutron stars are potentially detectable signatures of new physics. Screening mechanisms can in principle hide scalar effects, but their effectiveness in the strong-field regime is still largely unmodeled. In this thesis I briefly review the traditional tests of gravity, from the weak-field observations to gravitational-wave tests, before moving to discuss in details a collection of personal contributions in modeling the aforementioned scalar effects

    Dynamical Chameleon Neutron Stars: stability, radial oscillations and scalar radiation in spherical symmetry

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    Scalar-tensor theories whose phenomenology differs significantly from general relativity on large (e.g. cosmological) scales do not typically pass local experimental tests (e.g. in the solar system) unless they present a suitable "screening mechanism". An example is provided by chameleon screening, whereby the local general relativistic behavior is recovered in high density environments, at least in weak-field and quasi-static configurations. Here, we test the validity of chameleon screening in strong-field and highly relativistic/dynamical conditions, by performing fully non-linear simulations of neutron stars subjected to initial perturbations that cause them to oscillate or even collapse to a black hole. We confirm that screened chameleon stars are stable to sufficiently small radial oscillations, but that the frequency spectrum of the latter shows deviations from the general relativistic predictions. We also calculate the scalar fluxes produced during collapse to a black hole, and comment on their detectability with future gravitational-wave interferometers.Comment: 21 pages, 17 figure

    Молниеносная печеночная недостаточность медикаментозного, токсиколлергического генеза, разрешенная пересадкой печени. Kлинический случай

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    USMF Nicolae Testemițanu, Spitalul Clinic Republican, Conferința naţională de gastroenterologie şi hepatologie cu participare internaţională ”Actualităţi în gastroenterologie şi hepatologie” 16 iunie 2016 Chișinău, Republica MoldovaAcute hepatic failure is a result of toxic effects of used medication, viral hepatic infections, autoimmune hepatitis, but also there are unknown underlining causes. Hereby we present a case of violent acute, toxic- allergic, drug induced (sulfasalazin, metilprednisolon) hepatic failure, addressed by liver transplantation.Наиболее распространенные причины молниеносной печеночной недостаточности являются токсические эффекты препаратов, вирусный гепатит, аутоиммунный гепатит, а также неизвестные или неопределенные причины. Мы представляем клинический случай молниеносной печеночной недостаточности токсикоаллергического, медикаментозного (сульфасалазин, метилпреднизолон) генеза, которая была решена путем трансплантации печени

    Arterial vascularization of the colon; a guide to surgical resection

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    Background. Colorectal cancer is a commonly diagnosed neoplasia in men and women worldwide. This study aims to rigorously map the arterial distribution of the colon in order to assess the implications of vascular patterns in surgical resection. Methods. Cadaveric dissections were performed to explore the arterial distribution (including collateral blood flow) of the colon. The study used standard dissection tools and photographic documentation to detail the vascular architecture supporting the large intestine. Results. The dissection revealed important arterial branches and anastomoses in the area of the superior and inferior mesenteric arteries, which are able to ensure continuous local blood supply especially in cases of arterial ischemia. An important arterial anastomosis was identified between the right branch of the middle colic artery and the ascending branch of the right colic artery, as well as the specific distribution of the marginal artery of Drummond and Haller-Riolan anastomotic arch. Conclusions. The blood supply of the colon derived from both mesenteric arteries includes redundant arterial anastomoses, but which are critical in specific situations such as the approach and results of surgical resection. Understanding these vascular patterns and collateral pathways, as well as careful intraoperative surgical exploration, are essential for oncologic surgeons to ensure successful colic resections with minimal complications and morbidity

    Experimental violations of Bell's inequalities with time-bin and polarization entanglement Violazione delle disuguaglianze di Bell con entanglement in polarizzazione e time-bin

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    In this thesis activity the candidate has explored the main aspects of Bell Inequalities theory and eventually executed an experimental Violation test. This work contains a brief overview of the theoretical aspects around Bell Inequalities: the doubts arisen by Einstein, Podolski and Rosen about Quantum Theory completeness; the hidden variable theories and the bounds on classical correlations; quantum correlations and violation of Bell inequalities; the response given by Bell to the EPR paradox by introducing its famous theorem. In addition, the entanglement phenomenon has been studied, in particular in those dof that are given an important role in the violation of Bell Inequalities. Some documentation work was also done on non linear optics in order to understand fundamental effects that is common practice to exploit in the photon entanglement generation: SHG for the pump photons, SPDC in non-linear crystals. Moreover, the candidate also explored in this thesis some issues more closely related to the experimental aspect:loopholes that could affect the integrity of Bell inequalities proofs; efficiency threshold estimates regarding detection loophole; loophole-free configurations. Eventually, here in this report are also showed, along with the experimental setup brief description and some comments on the apparatus and its setting, the results of an experimental test of the CHSH inequality violation using photons entangled at first in polarization and then in a time-bin entanglement configuration

    Nonlinear aspects of the effective theory of dark energy

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    The goal of this project is to study the effects predicted by scalar-tensor theories of dark energy on small scales. Scalar-tensor theories has been introduced to modify gravity in the infrared. However, large scale modifications of gravity are necessarily associated to short-scale ones. In order to be in accordance with current observational tests on small scales, one can introduce a screening mechanism that is effective in environments where nonlinearities of the scalar field become important, suppressing the extra degrees of freedom. The Vainshtein screening has been already proven to work in many scalar-tensor theories, in particular in the most general second-order covariant theory for gravity coupled to a scalar degree of freedom, the so-called Horndeski theory. The focus of this thesis is on the breaking of this mechanism in the extensions of Horndeski: we retrieve the failure of the screening for beyond Horndeski theories, starting from more general premises. Finally, we tackle the challenge of generalizing this result further to DHOST theories

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    Bucureşti : Fundaţia Regală pentru Literatură şi Artă, 1940. - 233 p. : il. ; 21 cm
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