1,975 research outputs found
Recharging of Flying Base Stations using Airborne RF Energy Sources
This paper presents a new method for recharging flying base stations, carried
by Unmanned Aerial Vehicles (UAVs), using wireless power transfer from
dedicated, airborne, Radio Frequency (RF) energy sources. In particular, we
study a system in which UAVs receive wireless power without being disrupted
from their regular trajectory. The optimal placement of the energy sources are
studied so as to maximize received power from the energy sources by the
receiver UAVs flying with a linear trajectory over a square area. We find that
for our studied scenario of two UAVs, if an even number of energy sources are
used, placing them in the optimal locations maximizes the total received power,
while achieving fairness among the UAVs. However, in the case of using an odd
number of energy sources, we can either maximize the total received power, or
achieve fairness, but not both at the same time. Numerical results show that
placing the energy sources at the suggested optimal locations results in
significant power gain compared to nonoptimal placements.Comment: 6 pages, 5 figures, conference pape
Thermodynamic analysis of gravitational field equations in Lyra manifold
Considering the Einstein field equations in Lyra manifold, and applying the
unified first law of thermodynamics as well as the Clausius relation to the
apparent horizon of FRW universe, we find the entropy of apparent horizon in
Lyra manifold. In addition, the validity of second law of thermodynamics and
its generalized form are also studied. Finally, we use the first law of
thermodynamics in order to find the horizon entropy of static spherically
symmetric spacetimes. Some results of considering (anti)de-Sitter and
Schwarzschild metrics have also been addressed.Comment: Accepted by AHE
Side effects of phenobarbital and carbamazepine in childhood epilepsy: randomised controlled trial
Objective: To compare the behavioural side effects associated with two commonly used antiepilepsy drugs--phenobarbital and carbamazepine--in children in Bangladesh. Design: Prospective randomised controlled single centre trial. Setting: Specialist children's hospital in Dhaka, Bangladesh. Participants: 108 children aged 2-15 with generalised tonic-clonic (n=51) or partial and secondary generalised seizures (n=57). Main outcome measures: Seizure control and behavioural side effects. Results: 91 children were followed up for 12 months. Six required a change of antiepilepsy drug. Side effects were compared in 85 children. In the last quarter of the 12 month follow-up, 71 children were seizure free after one year's treatment. Thirty two in the phenobarbital group and 39 in the carbamazepine group had no seizures in 74 and 102 days after randomisation, respectively. Ten children had increased behavioural problems, which were unacceptable in four (one in the phenobarbital group and three in the carbamazepine group). Independent t tests, however, showed no difference between the two trial drugs. Conclusion: There was no excess in behavioural side effects with phenobarbital in children with epilepsy in a country with limited resources
Flux Expulsion - Field Evolution in Neutron Stars
Models for the evolution of magnetic fields of neutron stars are constructed,
assuming the field is embedded in the proton superconducting core of the star.
The rate of expulsion of the magnetic flux out of the core, or equivalently the
velocity of outward motion of flux-carrying proton-vortices is determined from
a solution of the Magnus equation of motion for these vortices. A force due to
the pinning interaction between the proton-vortices and the neutron-superfluid
vortices is also taken into account in addition to the other more conventional
forces acting on the proton-vortices. Alternative models for the field
evolution are considered based on the different possibilities discussed for the
effective values of the various forces. The coupled spin and magnetic evolution
of single pulsars as well as those processed in low-mass binary systems are
computed, for each of the models. The predicted lifetimes of active pulsars,
field strengths of the very old neutron stars, and distribution of the magnetic
fields versus orbital periods in low-mass binary pulsars are used to test the
adopted field decay models. Contrary to the earlier claims, the buoyancy is
argued to be the dominant driving cause of the flux expulsion, for the single
as well as the binary neutron stars. However, the pinning is also found to play
a crucial role which is necessary to account for the observed low field binary
and millisecond pulsars.Comment: 23 pages, + 7 figures, accepted for publication in Ap
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