[PDF] Top 20 El desarrollo de la identidad profesional en los estudiantes de Medicina: rol de los docentes

... in neutron stars, kaon-condensed phase in hyperon-mixed matter (abbreviated to Y +K phase) has been considered, and its implications for astrophysical phenomena such as structure and thermal evolution of ... See full document

... the hyperons with the residual ...the neutron stars, whose structure is strongly debated, following the measurement of two neutron stars exceeding 2M [26, ... See full document

... of hyperons and nucleon resonances have been dis- ...in neutron stars was presented by introducing a repulsive density depen- dence in the hyperon-vector meson ...in nuclei was derived by ... See full document

... the neutron and proton pair as valence particles, however due to rather different structure of these states with respect to the 10 B ground state, they are not expected to be populated strongly in this ... See full document

... of neutron stars where we have tried to present the most remarkable observational and theoretical aspects of this ...of neutron stars have been ...two neutron stars opens, as ... See full document

... Gravitational-wave chirp created from the collision of two neutron stars..[r] ... See full document

... MeV) this enhancement is relatively constant and can be considered geometric. Near and below the barrier how- ever, the enhancement increases rapidly with decreasing incident energy. In this energy domain the enhancement ... See full document

... The project B.6 has been funded over the second and third period of the SFB/TR 16. It grew out of the project B.3 from the first funding period, as explained in the corre- sponding contribution to that project. In the ... See full document

... light nuclei the number of protons and neutrons is the same ( N = Z ) but the number of neutrons increases fast as go up to balance the repulsive force between positively charges protons so that the nucleus ... See full document

... (i) Light ion reactions. These were used first, because of the 3 availability of suitable beams. For example, the (t,p) and (t, He) reactions change the isospin of the target nucleus by +1 (AT = +1). The reaction “* * * ... See full document

... We have studied a model that can explain the observations of large velocities found on neutron stars. Our model is based on the magnetic induced anisotropic emission of neutrinos as a mechanism of ... See full document

... The sporadic outbursts are thought to be triggered by thermal-viscous instabilities in the accretion disc that leads to an increased mass accretion rate onto the compact accretor (see e.g. Lasota 2001). Dynamical studies ... See full document

... QCD above the nuclear saturation density. We begin by examining what can be deduced about the M-R relation directly from these mass measurements, without employing a separate model for high- density matter. For lower ... See full document

... The next constraint I discuss here comes from the first observation of gravitational waves from a binary NS merger and its electromagnetic counterpart, GW170817 and AT2017gfo [27–29]. The observed gravitational wave ... See full document

... Abstract. In this work, we present a calculation of the non-Fermi liquid correction to the specific heat of magnetized degenerate quark matter present at the core of the neutron star. The role of non-Fermi liquid ... See full document

... At the heavy ion accelerator ATLAS at Argonne National Laboratory we have begun to study some of the reactions critical to our understanding of type I X-ray bursts and superbursts using beams on the proton-rich as well ... See full document

... Dynamical Stability of Nascent Neutron Stars Thesis by Yuk Tung Liu In Partial Fulfillment of the Requirements for the Degree of Doct or of Philosophy California Institute of Technology P asaden a, Ca[.] ... See full document

... the neutron radius of lead to about 1% accuracy (current accuracy is about 5%) using the parity violating asymmetry in elastic scattering due to the weak neutral ... See full document

... previous work [4], Lee et al. tried to explain this observation by introducing supercritical accretion in the evolution process of NS-NS binaries. In this work[4], they argued that the NS masses in NS-NS binaries cannot ... See full document

... Figure 1 shows, in the bottom, the γ-spectrum measured in coincidence with 49 Ca ions detected in PRISMA. All strong transitions correspond to decays from states identified as single particle excitations, besides the 660- ... See full document