Colóquios

Viscous hydrodynamics of strongly-interacting QCD medium, as probed by dileptons

Data: 
sexta-feira, 16 Fevereiro, 2018 - 11:00
Palestrante: 
Dr. Gojko Vujanovic (The Ohio State University)
Resumo: 

Recent viscous hydrodynamical studies [1,2] of the strongly-interacting medium created at the Relativistic Heavy-Ion Collider (RHIC) and the Large Hadron Collider (LHC), show that bulk viscosity plays an important role in their phenomenological description. A temperature-dependent bulk viscosity in the hydrodynamical evolution of the medium can modify the development of the hydrodynamic momentum anisotropy differently in the high- and low-temperature regions. Thus, anisotropic flow coefficients of various observables are affected differently depending where their surface of last scattering lies. For the case of hadronic observables, they are predominantly sensitive to low temperature regions, while electromagnetic radiation is emitted at all temperatures. Therefore, bulk viscosity should affect electromagnetic radiation differently than hadron emission. The effects of bulk viscosity on one of the electromagnetic probes, namely photons, has already been investigated [1]. The same statement holds true for hadrons [2]. The goal of this presentation is to study how thermal dilepton production, the other source of electromagnetic radiation, gets modified owing to the presence of bulk viscosity at RHIC and LHC energies. With calculations at different collision energies, comparisons in the dilepton signal can be made and more robust conclusions regarding the role of bulk viscosity in high energy heavy-ion collisions can be drawn. Dilepton radiation from the dilute hadronic phase of the medium will also be included to ascertain whether these modifications may be observable in experimental data.

[1] Jean-François Paquet et al., Phys. Rev. C 93 no. 4, 044906 (2016)
[2] S. Ryu et al., Phys. Rev. Lett. 115 no. 13, 132301 (2015)

 

(Local: Sala Jayme Tiomno)

Quantum Mechanics Without Wavefunctions

Data: 
terça-feira, 6 Fevereiro, 2018 - 11:00
Palestrante: 
Prof. Bill Poirier (Texas Tech University)
Resumo: 

This talk addresses a new formulation of quantum mechanics in which the wavefunction Ψ(t, x) is discarded entirely. Instead, the quantum state is represented as an ensemble of quantum trajectories x(t, C), or “worlds.” Each of these worlds has well-defined real- valued particle positions and momenta, and is thereby classical-like. Unlike a classical ensemble, however, nearby trajectories/worlds can interact with each other dynamically, giving rise to quantum effects. Moreover, x(t, C) satisfies a trajectory-based action principle, which allows quantum theory (via the Euler-Lagrange equation and Noether’s theorem) to be placed on the same footing as classical theories. In this manner, a straightforward relativistic generalization can be obtained. These and other developments, e.g. for many dimensions, multiple particles, and spin, may also be discussed.

(Local: Sala Jayme Tiomno)

Testando a isotropia do Universo com a estrutura em grande escala cosmológica

Data: 
terça-feira, 28 Novembro, 2017 - 11:00
Palestrante: 
Dr. Carlos Bengaly, University of Western Cape
Resumo: 

O modelo padrão atual da Cosmologia, ΛCDM, tem o Princípio Cosmológico (PC) como uma de suas hipóteses fundamentais, de modo que a métrica de fundo do Universo consiste na métrica Friedman-Lemaître-Robertson-Walker (FLRW). Assim, assume-se que o Universo é isotrópico e homogêneo em grandes escalas. Apesar do bom acordo entre o modelo ΛCDM (bem como demais modelos FLRW) e as observações cosmológicas, testes diretos do PC ainda precisam ser realizados para verificar se, de fato, o PC é uma hipótese válida ou tão apenas uma simplificação matemática.

Neste seminário, apresentarei um teste da isotropia cosmológica que fez uso da distribuição angular de galáxias da amostra WISE x SuperCOSMOS (WISC). Mais precisamente, verificamos se o dipolo desta distribuição está de acordo com análises anteriores na literatura, e de acordo com a amplitude típica de simulações baseadas no modelo ΛCDM. Além disto, discutirei brevemente sobre uma análise similar realizada recentemente com fontes em rádio, além das expectativas que surveys futuros, como o Square Kilometer Array (SKA), poderiam lançar sobre a isotropia cosmológica.

Referência dos trabalhos: https://arxiv.org/abs/1707.08091 e https://arxiv.org/abs/1710.08804Abstract: O modelo padrão atual da Cosmologia, ΛCDM, tem o Princípio Cosmológico (PC) como uma de suas hipóteses fundamentais, de modo que a métrica de fundo do Universo consiste na métrica Friedman-Lemaître-Robertson-Walker (FLRW). Assim, assume-se que o Universo é isotrópico e homogêneo em grandes escalas. Apesar do bom acordo entre o modelo ΛCDM (bem como demais modelos FLRW) e as observações cosmológicas, testes diretos do PC ainda precisam ser realizados para verificar se, de fato, o PC é uma hipótese válida ou tão apenas uma simplificação matemática.

Neste seminário, apresentarei um teste da isotropia cosmológica que fez uso da distribuição angular de galáxias da amostra WISE x SuperCOSMOS (WISC). Mais precisamente, verificamos se o dipolo desta distribuição está de acordo com análises anteriores na literatura, e de acordo com a amplitude típica de simulações baseadas no modelo ΛCDM. Além disto, discutirei brevemente sobre uma análise similar realizada recentemente com fontes em rádio, além das expectativas que surveys futuros, como o Square Kilometer Array (SKA), poderiam lançar sobre a isotropia cosmológica.

Referência dos trabalhos: https://arxiv.org/abs/1707.08091 e https://arxiv.org/abs/1710.08804

Wavepackets on de Sitter spacetime: first step towards a Haag-Ruelle scattering theory

Data: 
terça-feira, 21 Novembro, 2017 - 11:00
Palestrante: 
Dr. Marcus Brum, Instituto de Física da USP
Resumo: 

In this colloquium, we want to present the first steps of the formulation of a scattering theory on a curved spacetime, in the Haag-Ruelle approach. This approach determines the S-matrix without specifying a particular interaction, it is rather based on the asymptotic behaviour of massive solutions of the wave equation, which can be estimated with great generality. We will show the construction of wavepackets on de Sitter spacetime, whose masses are consistently defined from the structure of the Lorentz algebra, and estimate its asymptotic behaviour. Furthermore, we show that, in the limit as the de Sitter radius tends to infinity, the wavepackets tend to the wavepackets of Minkowski spacetime and the plane waves arising after contraction have support sharply located on the mass shell. We will also show how to construct (scalar) field operators from these wavepackets. Besides, we will argue that the equilibrium state is not a thermal state, thus avoiding known issues of scattering theory at finite temperatures, and we will discuss possible interpretations of the in- and out-states.

The phase diagram in T-muB-Nc space

Data: 
terça-feira, 27 Maio, 2014 - 11:00
Palestrante: 
Prof. Giorgio Torrieri (UNICAMP)
Resumo: 

I will discuss the phase structure of Yang-Mills matter at moderate temperature and chemical potential. Motivated by large Nc physics, I will argue that the non-perturbative structure of QCD can give rise to hitherto little explored phenomena, such as the coexistence of confinement with perturbative quark degrees of freedom. I will however show that this "quarkyonic phase" is defined by a percolation-type phase transition line which curves in "number of colors", as well as density and temperature. Given theoretical uncertainities in dealing with matter at this regime, therefore, a phenomenological and experimental investigation of matter at high chemical potential might be decisive to determine if the quarkyonic phase does in fact exist. I will conclude discussing possible experimental signatures of this new state of matter, concentrating on electromagnetic signals, as well as proposals for studying this matter using Gauge/Gravity duality.

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