310 research outputs found
Subset Sampling and Its Extensions
This paper studies the \emph{subset sampling} problem. The input is a set
of records together with a function that assigns
each record a probability . A query returns a
random subset of , where each record is
sampled into independently with probability . The goal is to
store in a data structure to answer queries efficiently. If
fits in memory, the problem is interesting when is
dynamic. We develop a dynamic data structure with
expected \emph{query} time,
space and amortized expected \emph{update}, \emph{insert} and
\emph{delete} time, where
. The query time and
space are optimal. If does not fit in memory, the problem is
difficult even if is static. Under this scenario, we present an
I/O-efficient algorithm that answers a \emph{query} in
amortized expected I/Os using space, where is the memory
size, is the block size and is the number of iterative
operations we need to perform on before going below . In
addition, when each record is associated with a real-valued key, we extend the
\emph{subset sampling} problem to the \emph{range subset sampling} problem, in
which we require that the keys of the sampled records fall within a specified
input range . For this extension, we provide a solution under the
dynamic setting, with expected
\emph{query} time, space and amortized
expected \emph{update}, \emph{insert} and \emph{delete} time.Comment: 17 page
Nuclear Matter and Neutron Stars from Relativistic Brueckner-Hartree-Fock Theory
The momentum and isospin dependence of the single-particle potential for the
in-medium nucleon are the key quantities in the Relativistic
Brueckner-Hartree-Fock (RBHF) theory. It depends on how to extract the scalar
and the vector components of the single-particle potential inside nuclear
matter. In contrast to the RBHF calculations in the Dirac space with the
positive-energy states (PESs) only, the single-particle potential can be
determined in a unique way by the RBHF theory together with the negative-energy
states (NESs), i.e., the RBHF theory in the full Dirac space. The saturation
properties of symmetric and asymmetric nuclear matter in the full Dirac space
are systematically investigated based on the realistic Bonn nucleon-nucleon
potentials. In order to further specify the importance of the calculations in
the full Dirac space, the neutron star properties are investigated. The direct
URCA process in neutron star cooling will happen at density
fm with the proton fractions
. The radii of a neutron star are
predicated as km, and their tidal
deformabilities are for potential Bonn A,
B, C. Comparing with the results obtained in the Dirac space with PESs only,
full-Dirac-space RBHF calculation predicts the softest symmetry energy which
would be more favored by the gravitational waves (GW) detection from GW170817.
Furthermore, the results from full-Dirac-space RBHF theory are consistent with
the recent astronomical observations of massive neutron stars and simultaneous
mass-radius measurement
TrafficPredict: Trajectory Prediction for Heterogeneous Traffic-Agents
To safely and efficiently navigate in complex urban traffic, autonomous
vehicles must make responsible predictions in relation to surrounding
traffic-agents (vehicles, bicycles, pedestrians, etc.). A challenging and
critical task is to explore the movement patterns of different traffic-agents
and predict their future trajectories accurately to help the autonomous vehicle
make reasonable navigation decision. To solve this problem, we propose a long
short-term memory-based (LSTM-based) realtime traffic prediction algorithm,
TrafficPredict. Our approach uses an instance layer to learn instances'
movements and interactions and has a category layer to learn the similarities
of instances belonging to the same type to refine the prediction. In order to
evaluate its performance, we collected trajectory datasets in a large city
consisting of varying conditions and traffic densities. The dataset includes
many challenging scenarios where vehicles, bicycles, and pedestrians move among
one another. We evaluate the performance of TrafficPredict on our new dataset
and highlight its higher accuracy for trajectory prediction by comparing with
prior prediction methods.Comment: Accepted by AAAI(Oral) 201
Offline Experience Replay for Continual Offline Reinforcement Learning
The capability of continuously learning new skills via a sequence of
pre-collected offline datasets is desired for an agent. However, consecutively
learning a sequence of offline tasks likely leads to the catastrophic
forgetting issue under resource-limited scenarios. In this paper, we formulate
a new setting, continual offline reinforcement learning (CORL), where an agent
learns a sequence of offline reinforcement learning tasks and pursues good
performance on all learned tasks with a small replay buffer without exploring
any of the environments of all the sequential tasks. For consistently learning
on all sequential tasks, an agent requires acquiring new knowledge and
meanwhile preserving old knowledge in an offline manner. To this end, we
introduced continual learning algorithms and experimentally found experience
replay (ER) to be the most suitable algorithm for the CORL problem. However, we
observe that introducing ER into CORL encounters a new distribution shift
problem: the mismatch between the experiences in the replay buffer and
trajectories from the learned policy. To address such an issue, we propose a
new model-based experience selection (MBES) scheme to build the replay buffer,
where a transition model is learned to approximate the state distribution. This
model is used to bridge the distribution bias between the replay buffer and the
learned model by filtering the data from offline data that most closely
resembles the learned model for storage. Moreover, in order to enhance the
ability on learning new tasks, we retrofit the experience replay method with a
new dual behavior cloning (DBC) architecture to avoid the disturbance of
behavior-cloning loss on the Q-learning process. In general, we call our
algorithm offline experience replay (OER). Extensive experiments demonstrate
that our OER method outperforms SOTA baselines in widely-used Mujoco
environments.Comment: 9 pages, 4 figure
Properties of Pb predicted from the relativistic equation of state in the full Dirac space
Relativistic Brueckner-Hartree-Fock (RBHF) theory in the full Dirac space
allows one to determine uniquely the momentum dependence of scalar and vector
components of the single-particle potentials. In order to extend this new
method from nuclear matter to finite nuclei, as a first step, properties of
Pb are explored by using the microscopic equation of state for
asymmetric nuclear matter and a liquid droplet model. The neutron and proton
density distributions, the binding energies, the neutron and proton radii, and
the neutron skin thickness in Pb are calculated. In order to further
compare the charge densities predicted from the RBHF theory in the full Dirac
space with the experimental charge densities, the differential cross sections
and the electric charge form factors in the elastic electron-nucleus scattering
are obtained by using the phase-shift analysis method. The results from the
RBHF theory are in good agreement with the experimental data. In addition, the
uncertainty arising from variations of the surface term parameter in the
liquid droplet model is also discussed
Rayleigh Quotient Graph Neural Networks for Graph-level Anomaly Detection
Graph-level anomaly detection has gained significant attention as it finds
applications in various domains, such as cancer diagnosis and enzyme
prediction. However, existing methods fail to capture the spectral properties
of graph anomalies, resulting in unexplainable framework design and
unsatisfying performance. In this paper, we re-investigate the spectral
differences between anomalous and normal graphs. Our main observation shows a
significant disparity in the accumulated spectral energy between these two
classes. Moreover, we prove that the accumulated spectral energy of the graph
signal can be represented by its Rayleigh Quotient, indicating that the
Rayleigh Quotient is a driving factor behind the anomalous properties of
graphs. Motivated by this, we propose Rayleigh Quotient Graph Neural Network
(RQGNN), the first spectral GNN that explores the inherent spectral features of
anomalous graphs for graph-level anomaly detection. Specifically, we introduce
a novel framework with two components: the Rayleigh Quotient learning component
(RQL) and Chebyshev Wavelet GNN with RQ-pooling (CWGNN-RQ). RQL explicitly
captures the Rayleigh Quotient of graphs and CWGNN-RQ implicitly explores the
spectral space of graphs. Extensive experiments on 10 real-world datasets show
that RQGNN outperforms the best rival by 6.74% in Macro-F1 score and 1.44% in
AUC, demonstrating the effectiveness of our framework. Our code is available at
https://github.com/xydong127/RQGNN
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