Hyperon ordering in neutron star matter

We explore the possible formation of ordered phases in neutron star matter. In the framework of a quantum hadrodynamics model where neutrons, protons and Lambda hyperons interact via the exchange of mesons, we compare the energy of the usually assumed uniform, liquid phase, to that of a configuration in which di-lambda pairs immersed in an uniform nucleon fluid are localized on the nodes of a regular lattice. The confining potential is calculated self-consistently as resulting from the combined action of the nucleon fluid and the other hyperons, under the condition of beta equilibrium. We are able to obtain stable ordered phases for some reasonable sets of values of the model parameters. This could have important consequences on the structure and cooling of neutron stars.Comment: 6 pages, 2 figures. To appear in the proceedings of the 4th Catania Relativistic Ion Studies: Exotic Clustering (CRIS 2002), Catania, Italy, 10-14 Jun 200

Majorana vs Pseudo-Dirac Neutrinos at the ILC

Neutrino masses could originate in seesaw models testable at colliders, with light mediators and an approximate lepton number symmetry. The minimal model of this type contains two quasi-degenerate Majorana fermions forming a pseudo-Dirac pair. An important question is to what extent future colliders will have sensitivity to the splitting between the Majorana components, since this quantity signals the breaking of lepton number and is connected to the light neutrino masses. We consider the production of these neutral heavy leptons at the ILC, where their displaced decays provide a golden signal: a forward-backward charge asymmetry, which depends crucially on the mass splitting between the two Majorana components. We show that this observable can constrain the mass splitting to values much lower than current bounds from neutrinoless double beta decay and natural loop corrections.Comment: 16 pages, 5 figures; v2: Minor changes, version accepted for publication in EPJ

Hyperonic crystallization in hadronic matter

Published in Hadrons, Nuclei and Applications, World Scientific, Singapore, Proc.of the Conference Bologna2000. Structure of the Nucleus at the Dawn of the Century, G. Bonsignori, M. Bruno, A. Ventura, D. Vretenar Editors, pag. 319.Comment: 4 pages, 2figure

Ultrafast relaxation rates and reversal time in disordered ferrimagnets

In response to ultrafast laser pulses, single-phase metals have been classified as “fast” (with magnetization quenching on the time scale of the order of 100 fs and recovery in the time scale of several picoseconds and below) and “slow” (with longer characteristic time scales). Disordered ferrimagnetic alloys consisting of a combination of “fast” transition (TM) and “slow” rare-earth (RE) metals have been shown to exhibit an ultrafast all-optical switching mediated by the heat mechanism. The behavior of the characteristic time scales of coupled alloys is more complicated and is influenced by many parameters such as the intersublattice exchange, doping (RE) concentration, and the temperature. Here, the longitudinal relaxation times of each sublattice are analyzed within the Landau-Lifshitz-Bloch framework. We show that for moderate intersublattice coupling strength both materials slow down as a function of slow (RE) material concentration. For larger coupling, the fast (TM) material may become faster, while the slow (RE) one is still slower. These conclusions may have important implications in the switching time of disordered ferrimagnets such as GdFeCo with partial clustering. Using atomistic modeling, we show that in the moderately coupled case, the reversal would start in the Gd-rich region, while the situation may be reversed if the coupling strength is larger

Recent high resolution laboratory determinations of line broadening and intensity parameters: PH3, CH3D, and CO2

Recent unpublished laboratory work on rovibrational line strengths and broadening coefficients which is of interest in the study of planetary atmospheres was reviewed. The molecules discussed are PH3, CH3D and CO2

Insurance-related instruments for disaster risk reduction (2011 Global Assessment Report on Disaster Risk Reduction)

Strategies and measures for disaster risk reduction (DRR) are not being implemented at the scale called for by the Hyogo Framework of Action. Part of the problem is that, from the perspective of decision makers with resource constraints, it is risky to invest in something that reaps benefits only in the case of a relatively unlikely event (such as a hurricane or a drought). People and institutions are understandably prone to invest in choices that yield less uncertain benefits. DRR, in itself, can be perceived as a risky endeavor - especially from the financial perspective. One way to circumvent this problem is by promoting DRR through incentives and other features embedded in market-based financial instruments, which offer financial stability or reliable access to funds to help cope with the consequences of extreme events. Since not all risks can be cost-effectively reduced, especially those that occur only very rarely, forward-thinking DRR stakeholders tend to seek options for financing the remaining or residual risks. Insurance and other disaster risk sharing approaches can serve households, national governments and humanitarian or development organizations, not only to complement ex ante DRR by ensuring or accelerating financing for post-disaster activities (like relief, recovery and reconstruction), but also as a conduit for ex ante DRR, guiding investment decisions that would result in fewer losses if a disaster materializes in the future. The objective of this paper is to assist disaster risk reduction stakeholders analyze whether - and how - insurance and other market-based risk transfer instruments can help increase resilience to disasters