Extra dimensions at the CERN LHC via mini-black holes: Effective Kerr-Newman brane-world effects

We solve Einstein equations on the brane to derive the exact form of the brane-world-corrected perturbations in Kerr-Newman singularities, using Randall-Sundrum and Arkani-Hamed-Dimopoulos-Dvali (ADD) models. It is a consequence of such models that Kerr-Newman mini-black holes can be produced in LHC. We use this approach to derive a normalized correction for the Schwarzschild Myers-Perry radius of a static (4+n)-dimensional mini-black hole, using more realistic approaches arising from Kerr-Newman mini-black hole analysis. Besides, we prove that there are four Kerr-Newman black hole horizons in the brane-world scenario we use, although only the outer horizon is relevant in the physical measurable processes. Parton cross sections in LHC and Hawking temperature are also investigated as functions of Planck mass (in the LHC range 1-10 TeV), mini-black hole mass, and the number of large extra dimensions in brane-world large extra-dimensional scenarios. In this case a more realistic brane-effect-corrected formalism can achieve more precisely the effective extra-dimensional Planck mass and the number of large extra dimensions-in the Arkani-Hamed-Dimopoulos-Dvali model-or the size of the warped extra dimension-in Randall-Sundrum formalism.

Kerr-Newman solution as a Dirac particle

For m(2) < a(2) + q(2), with m, a, and q respectively the source mass, angular momentum per unit mass, and electric charge, the Kerr-Newman (KN) solution of Einstein's equation reduces to a naked singularity of circular shape, enclosing a disk across which the metric components fail to be smooth. By considering the Hawking and Ellis extended interpretation of the KN spacetime, it is shown that, similarly to the electron-positron system, this solution presents four inequivalent classical states. Making use of Wheeler's idea of charge without charge, the topological structure of the extended KN spatial section is found to be highly non-trivial, leading thus to the existence of gravitational states with half-integral angular momentum. This property is corroborated by the fact that, under a rotation of the space coordinates, those inequivalent states transform into themselves only after a 4π rotation. As a consequence, it becomes possible to naturally represent them in a Lorentz spinor basis. The state vector representing the whole KN solution is then constructed, and its evolution is shown to be governed by the Dirac equation. The KN solution can thus be consistently interpreted as a model for the electron-positron system, in which the concepts of mass, charge and spin become connected with the spacetime geometry. Some phenomenological consequences of the model are explored.

Partículas de spin 1/2 e o papel da torção na descrição da interação gravitacional

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

L'atmosfera termica e il suo ruolo nell'entropia dei buchi neri

Con il testo presente, si intende mostrare come i gradi di libertà associati all'entropia di un buco nero possano essere ricercati in parte fruttuosamente nell'interazione dei campi quantistici con la struttura causale e geometrica esibita da un buco nero. Nel Capitolo 1, si affrontano le principali caratteristiche dei buchi neri alla luce della teoria classica di Relatività Generale: sono analizzate la soluzione di Schwarzschild e la struttura causale nello spazio-tempo conseguente, discutendo le definizioni di orizzonte e di singolarità e il rapporto che le lega, con riferimento ai risultati di Penrose e Hawking. Introdotto, all'inizio del Capitolo 2, il concetto di gravità superficiale e la metrica di Kerr-Newman, si studia il significato delle Quattro Leggi dei buchi neri, valide per soluzioni stazionarie. Il Capitolo 3 espone quali motivazioni spingano a proporre una caratterizzazione termodinamica dei buchi neri, attribuendovi una temperatura e un'entropia (detta “di Bekenstein-Hawking”) di natura geometrica, dipendente dall'area dell'orizzonte; si trattano qui i problemi che si incontrano nel costruire una corrispondente Meccanica Statistica. Si descrive dunque in quali termini il processo di radiazione di Hawking riesca a dare una spiegazione fisica della temperatura, e si rileva la presenza, secondo osservatori statici, di un'atmosfera termica nei pressi dell’orizzonte. Infine, si esamina la possibilità di attribuire alla radiazione di Hawking i gradi di libertà relativi all'entropia di Bekenstein-Hawking. In particolare, si illustra il modello a muro di mattoni di 't Hooft, che lega i gradi di libertà all'atmosfera termica. Considerando infine la deformazione dell'orizzonte dovuta a fluttuazioni quantistiche, si giunge alla conclusione che l'entropia dell'atmosfera termica rappresenta non un'interpretazione dell'entropia di Bekenstein-Hawking, bensì una sua correzione al secondo ordine.

Virtual worlds in Australian and New Zealand higher education : remembering the past, understanding the present and imagining the future

3D virtual reality, including the current generation of multi-user virtual worlds, has had a long history of use in education and training, and it experienced a surge of renewed interest with the advent of Second Life in 2003. What followed shortly after were several years marked by considerable hype around the use of virtual worlds for teaching, learning and research in higher education. For the moment, uptake of the technology seems to have plateaued, with academics either maintaining the status quo and continuing to use virtual worlds as they have previously done or choosing to opt out altogether. This paper presents a brief review of the use of virtual worlds in the Australian and New Zealand higher education sector in the past and reports on its use in the sector at the present time, based on input from members of the Australian and New Zealand Virtual Worlds Working Group. It then adopts a forward-looking perspective amid the current climate of uncertainty, musing on future directions and offering suggestions for potential new applications in light of recent technological developments and innovations in the area.

Enhanced sensitivity in detection of Kerr rotation by double modulation and time averaging based on Allan variance

Experiments in spintronics necessarily involve the detection of spin polarization. The sensitivity of this detection becomes an important factor to consider when extending the low temperature studies on semiconductor spintronic devices to room temperature, where the spin signal is weaker. In pump-probe experiments, which optically inject and detect spins, the sensitivity is often improved by using a photoelastic modulator (PEM) for lock-in detection. However, spurious signals can arise if diode lasers are used as optical sources in such experiments, along with a PEM. In this work, we eliminated the spurious electromagnetic coupling of the PEM onto the probe diode laser, by the double modulation technique. We also developed a test for spurious modulated interference in the pump-probe signal, due to the PEM. Besides, an order of magnitude enhancement in the sensitivity of detection of spin polarization by Kerr rotation, to 3x10(-8) rad was obtained by using the concept of Allan variance to optimally average the time series data over a period of 416 s. With these improvements, we are able to experimentally demonstrate at room temperature, photoinduced steady-state spin polarization in bulk GaAs. Thus, the advances reported here facilitate the use of diode lasers with a PEM for sensitive pump-probe experiments. They also constitute a step toward detection of spin-injection in Si at room temperature.

Thriocerodes anthicides (newman), Comb. N. (Coleoptera: Cleridae): An australian, not South African, species

Corynetes compactus Westwood is recognised as a junior synonym (syn. n.) of Pylus anthicides Newman, which is transferred from the South African genus Thriocera Gorham to the endemic Australian genus Thriocerodes Wolcott & Dybas, resulting in the combination Thriocerodes anthicides (Newman), comb. n.

Creemos porque amamos : la estructura interna del acto de fe en John Henry Newman

El autor nos introduce en la cuestión de los motivos racionales de la fe. Las operaciones llevadas a cabo por la inteligencia y la voluntad en el acto de creer, constituyen el fundamento por el cual la Verdad revelada entabla históricamente el diálogo con el hombre. El tema se halla en el centro de la experiencia religiosa y de la reflexión teológica de Newman, y ha significado un aporte indiscutible a la teología contemporánea.

La “experiencia religiosa” forjadora de un lenguaje teológico significativo en John Henry Newman

El autor plantea la cuestión de lo significativo del lenguaje teológico a partir del concepto de experiencia en el pensamiento del cardenal Newman. Su itinerario de fe y conversión, enraizado en un diálogo personal con Dios, le ha dado tanto a su teología como a su predicación, un atractivo que trasciende su época y que puede servir de estímulo actualmente en la comunicación teológica.

Newman y “La idea de una universidad”

El papa Benedicto XVI beatificó el 19 de septiembre del año pasado a John Henry Newman, en la Misa final de su visita oficial al Reino Unido. En un pasaje de la homilía dijo así: “Me gustaría rendir especial homenaje a su visión de la educación, que ha hecho tanto por formar el ethos que es la fuerza motriz de las escuelas y facultades católicas actuales. Firmemente contrario a cualquier enfoque reductivo o utilitarista, buscó lograr unas condiciones educativas en las que se unificara el esfuerzo intelectual, la disciplina moral y el compromiso religioso. El proyecto de fundar una Universidad Católica en Irlanda le brindó la oportunidad de desarrollar sus ideas al respecto, y la colección de discursos que publicó con el título La Idea de una Universidad sostiene un ideal mediante el cual todos los que están inmersos en la formación académica pueden seguir aprendiendo”. Estas palabras por sí solas justifican que nos ocupemos aquí de Newman y la Universidad, recordando que el suyo no fue solo un pensamiento teórico sino fruto de su experiencia personal: anglicano en Oxford, como fellow y tutor en el Oriel College, y católico en Dublín, como fundador y rector de la Universidad Católica de Irlanda. Vivió entre 1801 y 1890, y se convirtió en 1845, y en su paso del anglicanismo al catolicismo mantuvo los mismos principios esenciales, a los cuales pretendo acercarme en esta exposición.

Enhancing Kerr nonlinearity in an asymmetric double quantum well via Fano interference

We investigate the enhancement of Kerr nonlinearity in an asymmetric GaAs double quantum well via Fano interference, which is caused by tunneling from the excited subband to the continuum. In our structure, owing to Fano interference, the Kerr nonlinearity can be enhanced by appropriately choosing the values of the detunings and the intensity of the pump field, while cancel the linear and nonlinear absorptions.