4,510 research outputs found
Aplikasi Game Yang Menerapkan Metode Autonomous NPC Untuk Mengkoordinasi AI Dari Enemy
Dalam action game belakangan ini, biasanya player akan dihadapkan dengan banyak AI secara bersamaan. Agar dapat memberikan tantangan terhadap player akan dibutuhkan kelakuan yang kompleks. Untuk menciptakan kesan ini, AI tersebut harus dapat berkoordinasi dengan yang lain dalam menyerang player tanpa menghilangkan gameplay yang baik dan seimbang.Untuk dapat membuat AI tersebut, maka akan ditambahkan mekanisme attack slot, exclusion zone, trigger system, enemy event, player mutex, allowed zone, dan blackboard untuk membantu AI saling berkomunikasi dan mengatur sikap dari AI dalam menghadapi sebuah situasi.Dari hasil pengujian, bisa dilihat bahwa player dapat melawan sejumlah AI sekaligus dan memiliki kesempatan untuk menang. AI tersebut juga bisa terlihat berkoordinasi dalam perlawanan mereka terhadap player. Masalah yang dapat terjadi adalah dalam penggunaan attack slot dan exclusion zone harus memperhitungkan jumlah enemy yang bisa menempati slot yang sama karena bila terlalu banyak dapat megakibatkan enemy saling berebut tempat dan menghilangkan kesan berkoordinasi. Dalam penggunaan player mutex harus dipastikan pengembaliannya oleh enemy yang mengambil. Kegagalan dalam mengembalikan mutex tersebut akan membuat semua enemy lain tidak dapat menyerang
The Size and Origin of Metal-enriched Regions in the Intergalactic Medium from Spectra of Binary Quasars
We present tomography of the circum-galactic metal distribution at redshift 1.7-4.5 derived from echellete spectroscopy of binary quasars. We find C IV systems at similar redshifts in paired sightlines more often than expected for sightline-independent redshifts. As the separation of the sightlines increases from 36 kpc to 907 kpc, the amplitude of this clustering decreases. At the largest separations, the C IV systems cluster similar to the Lyman-break galaxies studied by Adelberger et al. in 2005. The C IV systems are significantly less correlated than these galaxies, however, at separations less than R_1 0.42 ± 0.15 h^( –1) comoving Mpc. Measured in real space, i.e., transverse to the sightlines, this length scale is significantly smaller than the break scale estimated previously from the line-of-sight correlation function in redshift space by Scannapieco et al. in 2006. Using a simple model, we interpret the new real-space measurement as an indication of the typical physical size of enriched regions. We adopt this size for enriched regions and fit the redshift-space distortion in the line-of-sight correlation function. The fitted velocity kick is consistent with the peculiar velocity of galaxies as determined by the underlying mass distribution and places an upper limit on the average outflow (or inflow) speed of metals. The implied timescale for dispersing metals is larger than the typical stellar ages of Lyman-break galaxies, and we argue that enrichment by galaxies at z > 4.3 played a greater role in dispersing metals. To further constrain the growth of enriched regions, we discuss empirical constraints on the evolution of the C IV correlation function with cosmic time. This study demonstrates the potential of tomography for measuring the metal enrichment history of the circum-galactic medium
The Role of Collective Neutrino Flavor Oscillations in Core-Collapse Supernova Shock Revival
We explore the effects of collective neutrino flavor oscillations due to
neutrino-neutrino interactions on the neutrino heating behind a stalled
core-collapse supernova shock. We carry out axisymmetric (2D)
radiation-hydrodynamic core-collapse supernova simulations, tracking the first
400 ms of the post-core-bounce evolution in 11.2 solar mass and 15 solar mass
progenitor stars. Using inputs from these 2D simulations, we perform neutrino
flavor oscillation calculations in multi-energy single-angle and multi-angle
single-energy approximations. Our results show that flavor conversions do not
set in until close to or outside the stalled shock, enhancing heating by not
more than a few percent in the most optimistic case. Consequently, we conclude
that the postbounce pre-explosion dynamics of standard core-collapse supernovae
remains unaffected by neutrino oscillations. Multi-angle effects in regions of
high electron density can further inhibit collective oscillations,
strengthening our conclusion.Comment: v2: Added multi-angle calculations. Conclusions unchanged. 16 pages,
7 figures. Accepted to Phys. Rev. D after revisions: 15 Sept 2011 (major), 24
Jan 2012 (minor
A New Waveform Consistency Test for Gravitational Wave Inspiral Searches
Searches for binary inspiral signals in data collected by interferometric
gravitational wave detectors utilize matched filtering techniques. Although
matched filtering is optimal in the case of stationary Gaussian noise, data
from real detectors often contains "glitches" and episodes of excess noise
which cause filter outputs to ring strongly. We review the standard \chi^2
statistic which is used to test whether the filter output has appropriate
contributions from several different frequency bands. We then propose a new
type of waveform consistency test which is based on the time history of the
filter output. We apply one such test to the data from the first LIGO science
run and show that it cleanly distinguishes between true inspiral waveforms and
large-amplitude false signals which managed to pass the standard \chi^2 test.Comment: 10 pages, 6 figures, submitted to Classical and Quantum Gravity for
the proceedings of the Eighth Gravitational Wave Data Analysis Workshop
(GWDAW-8
Multiple Chemodynamic Stellar Populations of the Ursa Minor Dwarf Spheroidal Galaxy
We present a Bayesian method to identify multiple (chemodynamic) stellar
populations in dwarf spheroidal galaxies (dSphs) using velocity, metallicity,
and positional stellar data without the assumption of spherical symmetry. We
apply this method to a new Keck/DEIMOS spectroscopic survey of the Ursa Minor
(UMi) dSph. We identify 892 likely members, making this the largest UMi sample
with line-of-sight velocity and metallicity measurements. Our Bayesian method
detects two distinct chemodynamic populations with high significance
(). The metal-rich () population is
kinematically colder (radial velocity dispersion of ) and more centrally concentrated than the metal-poor () and kinematically hotter population (). Furthermore, we apply the same analysis to
an independent MMT/Hectochelle data set and confirm the existence of two
chemodynamic populations in UMi. In both data sets, the metal-rich population
is significantly flattened () and the metal-poor
population is closer to spherical (). Despite
the presence of two populations, we are unable to robustly estimate the slope
of the dynamical mass profile. We found hints for prolate rotation of order
in the MMT data set, but further observations
are required to verify this. The flattened metal-rich population invalidates
assumptions built into simple dynamical mass estimators, so we computed new
astrophysical dark matter annihilation (J) and decay profiles based on the
rounder, hotter metal-poor population and inferred
for the Keck
data set. Our results paint a more complex picture of the evolution of Ursa
Minor than previously discussed.Comment: 20 pages, 11 figures, data included. Comments welcome. Accepted to
MNRA
Mechanical Instabilities of Biological Tubes
We study theoretically the shapes of biological tubes affected by various
pathologies. When epithelial cells grow at an uncontrolled rate, the negative
tension produced by their division provokes a buckling instability. Several
shapes are investigated : varicose, enlarged, sinusoidal or sausage-like, all
of which are found in pathologies of tracheal, renal tubes or arteries. The
final shape depends crucially on the mechanical parameters of the tissues :
Young modulus, wall-to-lumen ratio, homeostatic pressure. We argue that since
tissues must be in quasistatic mechanical equilibrium, abnormal shapes convey
information as to what causes the pathology. We calculate a phase diagram of
tubular instabilities which could be a helpful guide for investigating the
underlying genetic regulation
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