322 research outputs found
A New Measurement of the Temperature Density Relation of the IGM From Voigt Profile Fitting
We decompose the Lyman-{\alpha} (Ly{\alpha}) forest of an extensive sample of
74 high signal-to-noise ratio and high-resolution quasar spectra into a
collection of Voigt profiles. Absorbers located near caustics in the peculiar
velocity field have the smallest Doppler parameters, resulting in a low-
cutoff in the - set by the thermal state of intergalactic
medium (IGM). We fit this cutoff as a function of redshift over the range
, which allows us to measure the evolution of the IGM
temperature-density () relation parameters
and . We calibrate our measurements against Ly forest
simulations, using 21 different thermal models of the IGM at each redshift,
also allowing for different values of the IGM pressure smoothing scale. We
adopt a forward-modeling approach and self-consistently apply the same
algorithms to both data and simulations, propagating both statistical and
modeling uncertainties via Monte Carlo. The redshift evolution of shows a
suggestive peak at , while our evolution of is consistent with
and disfavors inverted temperature-density relations. Our
measured evolution of and are generally in good agreement with
previous determinations in the literature. Both the peak in the evolution of
at , as well as the high temperatures K
that we observe at , strongly suggest that a significant episode
of heating occurred after the end of HI reionization, which was most likely the
cosmic reionization of HeII.Comment: Accepted for publication in ApJ, 23 pages, 26 figures, machine
readable tables available onlin
Electron-ion recombination of Si IV forming Si III: Storage-ring measurement and multiconfiguration Dirac-Fock calculations
The electron-ion recombination rate coefficient for Si IV forming Si III was
measured at the heavy-ion storage-ring TSR. The experimental electron-ion
collision energy range of 0-186 eV encompassed the 2p(6) nl n'l' dielectronic
recombination (DR) resonances associated with 3s to nl core excitations, 2s
2p(6) 3s nl n'l' resonances associated with 2s to nl (n=3,4) core excitations,
and 2p(5) 3s nl n'l' resonances associated with 2p to nl (n=3,...,infinity)
core excitations. The experimental DR results are compared with theoretical
calculations using the multiconfiguration Dirac-Fock (MCDF) method for DR via
the 3s to 3p n'l' and 3s to 3d n'l' (both n'=3,...,6) and 2p(5) 3s 3l n'l'
(n'=3,4) capture channels. Finally, the experimental and theoretical plasma DR
rate coefficients for Si IV forming Si III are derived and compared with
previously available results.Comment: 13 pages, 9 figures, 3 tables. Accepted for publication in Physical
Review
Experimental study of fragmentation products in the reactions 112Sn + 112Sn and 124Sn + 124Sn at 1 AGeV
Production cross-sections and longitudinal velocity distributions of the
projectile-like residues produced in the reactions 112Sn + 112Sn and 124Sn +
124Sn both at an incident beam energy of 1 AGeV were measured with the
high-resolution magnetic spectrometer, the Fragment Separator (FRS) of GSI. For
both reactions the characteristics of the velocity distributions and nuclide
production cross sections were determined for residues with atomic number Z
10. A comparison of the results of the two reactions is presented.Comment: 14 pages, 12 figure
Dielectronic Recombination of Fe XV forming Fe XIV: Laboratory Measurements and Theoretical Calculations
We have measured resonance strengths and energies for dielectronic
recombination (DR) of Mg-like Fe XV forming Al-like Fe XIV via N=3 -> N' = 3
core excitations in the electron-ion collision energy range 0-45 eV. All
measurements were carried out using the heavy-ion Test Storage Ring at the Max
Planck Institute for Nuclear Physics in Heidelberg, Germany. We have also
carried out new multiconfiguration Breit-Pauli (MCBP) calculations using the
AUTOSTRUCTURE code. For electron-ion collision energies < 25 eV we find poor
agreement between our experimental and theoretical resonance energies and
strengths. From 25 to 42 eV we find good agreement between the two for
resonance energies. But in this energy range the theoretical resonance
strengths are ~ 31% larger than the experimental results. This is larger than
our estimated total experimental uncertainty in this energy range of +/- 26%
(at a 90% confidence level). Above 42 eV the difference in the shape between
the calculated and measured 3s3p(^1P_1)nl DR series limit we attribute partly
to the nl dependence of the detection probabilities of high Rydberg states in
the experiment. We have used our measurements, supplemented by our
AUTOSTRUCTURE calculations, to produce a Maxwellian-averaged 3 -> 3 DR rate
coefficient for Fe XV forming Fe XIV. The resulting rate coefficient is
estimated to be accurate to better than +/- 29% (at a 90% confidence level) for
k_BT_e > 1 eV. At temperatures of k_BT_e ~ 2.5-15 eV, where Fe XV is predicted
to form in photoionized plasmas, significant discrepancies are found between
our experimentally-derived rate coefficient and previously published
theoretical results. Our new MCBP plasma rate coefficient is 19-28% smaller
than our experimental results over this temperature range
Effects of correlation between merging steps on the global halo formation
The excursion set theory of halo formation is modified by adopting the
fractional Brownian motion, to account for possible correlation between merging
steps. We worked out analytically the conditional mass function, halo merging
rate and formation time distribution in the spherical collapse model. We also
developed an approximation for the ellipsoidal collapse model and applied it to
the calculation of the conditional mass function and the halo formation time
distribution. For models in which the steps are positively correlated, the halo
merger rate is enhanced when the accreted mass is less than , while
for the negatively correlated case this rate is reduced. Compared with the
standard model in which the steps are uncorrelated, the models with positively
correlated steps produce more aged population in small mass halos and more
younger population in large mass halos, while for the models with negatively
correlated steps the opposite is true. An examination of simulation results
shows that a weakly positive correlation between successive merging steps
appears to fit best. We have also found a systematic effect in the measured
mass function due to the finite volume of simulations. In future work, this
will be included in the halo model to accurately predict the three point
correlation function estimated from simulations.Comment: 8 pages, submitted to MNRA
Social media and community policing implementation in South Eastern Europe : a question of trust
At the present time, social media are increasingly used within community policing as a tool of fostering communication, and improving trust between the police and communities. Community policing programmes implemented in post-communist countries in South Eastern Europe, as well as processes of building police legitimacy in general, have been facing challenges related to insufficient public confidence in the law enforcement, and a necessity to re-define police roles. This paper uses the results of empirical research to argue that the still ongoing processes of bridging gaps in police-community communication can be supported by the use of social media. Presented argumentation is based on the analysis of selected quantitative studies on police legitimacy, and chosen findings of qualitative field research which was conducted in 2016 in Bosnia and Herzegovina as a part of the project Community-Based Policing and Post-Conflict Police Reform (ICT4COP). An implication of presented study should be a more in-depth analysis of key factors influencing both the formation of police legitimacy, and ways in which the use of social media in police–community relations, especially, in post-communist societies, should be designed to serve the purpose of building trust in the police
Hydrogen storage in a layered flexible [Ni2(btc)(en)2]n coordination polymer
[Ni2(btc)(en)2]n coordination polymer exhibits a layered two-dimensional structure with weak interaction between the layers. Correlation of experimental measurements, DFT calculations and molecular simulations demonstrated that its structural features, primarily the inherent flexibility of the layered polymeric structure, lead to improved hydrogen storage performance at room temperature, due to significant enhancement in isosteric heats of hydrogen adsorption. Volumetric measurements of hydrogen adsorption at room temperature show up to 0.3 wt.% hydrogen absorbed at 303 K and 2.63 bar of hydrogen pressure, with isosteric heats of adsorption of about 12.5 kJ mol−1. Predicted performance at room temperature is 1.8 wt.% at 48 bar and 3.5 wt.% at 100 bar, better than both MOF-5 and NU-100, with calculated values of isosteric heats for adsorption of hydrogen in 8–13 kJ mol−1 range at both 77 K and 303 K. Grand canonical Monte Carlo calculations show that this material, at 77 K, exhibits gravimetric hydrogen densities of more than 10 wt.% (up to 8.3 wt.% excess) with the corresponding volumetric density of at least 66 gL−1, which is comparable to MOF-5, but achieved with considerably smaller surface area of about 2500 m2 g−1. This study shows that layered two-dimensional MOFs could be a step towards MOF systems with significantly higher isosteric heats of adsorption, which could provide better room temperature hydrogen storage capabilities.This is the peer reviewed version of the following article: Blagojević, V.A., Lukić, V., Begović, N.N., Maričić, A.M., Minić, D.M., 2016, “Hydrogen storage in a layered flexible [Ni2(btc)(en)2]n coordination polymer”, International Journal of Hydrogen Energy, http://dx.doi.org/10.1016/j.ijhydene.2016.08.20
A Numerical Model for Brownian Particles Fluctuating in Incompressible Fluids
We present a numerical method that consistently implements thermal
fluctuations and hydrodynamic interactions to the motion of Brownian particles
dispersed in incompressible host fluids. In this method, the thermal
fluctuations are introduced as random forces acting on the Brownian particles.
The hydrodynamic interactions are introduced by directly resolving the fluid
motions with the particle motion as a boundary condition to be satisfied. The
validity of the method has been examined carefully by comparing the present
numerical results with the fluctuation-dissipation theorem whose analytical
form is known for dispersions of a single spherical particle. Simulations are
then performed for more complicated systems, such as a dispersion composed of
many spherical particles and a single polymeric chain in a solvent.Comment: 6 pages, 8 figure
The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
The baryon content of high-density regions in the universe is relevant to two
critical unanswered questions: the workings of nurture effects on galaxies and
the whereabouts of the missing baryons. In this paper, we analyze the
distribution of dark matter and semianalytical galaxies in the Millennium
Simulation to investigate these problems. Applying the same density field
reconstruction schemes as used for the overall matter distribution to the
matter locked in halos we study the mass contribution of halos to the total
mass budget at various background field densities, i.e., the conditional halo
mass function. In this context, we present a simple fitting formula for the
cumulative mass function accurate to ~ 5% for halo masses between 10^{10} and
10^{15}Msol/h. We find that in dense environments the halo mass function
becomes top heavy and present corresponding fitting formulae for different
redshifts. We demonstrate that the major fraction of matter in high-density
fields is associated with galaxy groups. Since current X-ray surveys are able
to nearly recover the universal baryon fraction within groups, our results
indicate that the major part of the so-far undetected warm-hot intergalactic
medium resides in low-density regions at low temperatures. Similarly, we show
that the differences in galaxy mass functions with environment seen in observed
and simulated data stem predominantly from differences in the mass distribution
of halos. In particular, the hump in the galaxy mass function is associated
with the central group galaxies, and the bimodality observed in the galaxy mass
function is therefore interpreted as that of central galaxies versus
satellites.Comment: aligned with version published in Ap
Preliminary geosite assessment model (gam) and its application on Fruška gora mountain, potential geotourism destination of Serbia
This paper presents a preliminary geosite physical assessment model which has the potential to assist in the sustainable planning and management of natural heritage locations and their transformation into tourism destination. The methodology is based on several existing models and presented through two groups of values – main and additional, which are further divided into indicators and subindicators respectively. The resultant model is a graph that consists of nine fields, into which geosites can be classified as fitting into nine general areas of suitability for tourism in terms of their main (scientific/educational, aesthetic/scenic and protection as market appeal and conservation) and additional values (functional and tourism use as current stage of development). This could prove to be of great help to natural heritage protection and tourism managers, as they could assess the current state of a geosite and thence propose a future path for it
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