7,751 research outputs found
Energy-Efficient Multi-View Video Transmission with View Synthesis-Enabled Multicast
Multi-view videos (MVVs) provide immersive viewing experience, at the cost of
heavy load to wireless networks. Except for further improving viewing
experience, view synthesis can create multicast opportunities for efficient
transmission of MVVs in multiuser wireless networks, which has not been
recognized in existing literature. In this paper, we would like to exploit view
synthesis-enabled multicast opportunities for energy-efficient MVV transmission
in a multiuser wireless network. Specifically, we first establish a
mathematical model to characterize the impact of view synthesis on multicast
opportunities and energy consumption. Then, we consider the optimization of
view selection, transmission time and power allocation to minimize the weighted
sum energy consumption for view transmission and synthesis, which is a
challenging mixed discrete-continuous optimization problem. We propose an
algorithm to obtain an optimal solution with reduced computational complexity
by exploiting optimality properties. To further reduce computational
complexity, we also propose two low-complexity algorithms to obtain two
suboptimal solutions, based on continuous relaxation and Difference of Convex
(DC) programming, respectively. Finally, numerical results demonstrate the
advantage of the proposed solutions.Comment: 22 pages, 6 figures, to be published in GLOBECOM 201
The masses and axial currents of the doubly charmed baryons
The chiral dynamics of the doubly heavy baryons is solely governed by the
light quark. In this work, We have derived the chiral corrections to the mass
of the doubly heavy baryons up to NLO. The mass splitting of and
at the NLO depends on one unknown low energy constant .
With the experimental mass of as the input, we estimate the
mass of to be around 3.678 GeV. Moreover, we have also performed
a systematical analysis of the chiral corrections to the axial currents and
axial charges of the doubly heavy baryons. The chiral structure and analytical
expressions will be very useful to the chiral extrapolations of the future
lattice QCD simulations of the doubly heavy baryons.Comment: 10 pages, 2 tables, 3 figure. Accepted by Phys. Rev.
Applicability of Relativistic Point-Coupling Models to Neutron Star Physics
Comparing with a wide range of covariant energy density functional models
based on the finite-range meson-exchange representation, the relativistic
mean-field models with the zero-range contact interaction, namely the
relativistic point-coupling models, are still infrequent to be utilized in
establishing nuclear equation of state (EoS) and investigating neutron star
properties, although comprehensive applications and achievements of them in
describing many nuclear properties both in ground and exited states are mature.
In this work, the EoS of neutron star matter is established constructively in
the framework of the relativistic point-coupling models to study neutron star
physics. Taking two selected functionals DD-PC1 and PC-PK1 as examples, nuclear
symmetry energies and several neutron star properties including proton
fractions, mass-radius relations, the core-crust transition density, the
fraction of crustal moment of inertia and dimensionless tidal deformabilities
are discussed. A suppression of pressure of neutron star matter found in the
functional PC-PK1 at high densities results in the difficulty of its prediction
when approaching to the maximum mass of neutron stars. In addition, the
divergences between two selected functionals in describing neutron star
quantities mentioned above are still large, ascribing to the less constrained
behavior of these functionals at high densities. Then it is expected that the
constraints on the dense matter EoS from precise and massive modern
astronomical observations, such as the tidal-deformabilities taken from
gravitational-wave events, would be essential to improve the parameterizing of
the relativistic point-coupling models.Comment: To appear in the AIP Proceedings of the Xiamen-CUSTIPEN Workshop on
the EOS of Dense Neutron-Rich Matter in the Era of Gravitational Wave
Astronomy, Jan. 3-7, Xiamen, Chin
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