1,399 research outputs found
Due questioni di legittimità costituzionale relative alla disciplina dell’omicidio e delle lesioni stradali : deroga al giudizio di bilanciamento e automatismo della revoca della patente
Acoustic analysis of cement composites with lignocellulosic residues
Received: January 19th, 2021 ; Accepted: May 20th, 2021 ; Published: October 5th, 2021 ; Correspondence: [email protected] concept of environmental sustainability has been seeking a way to develop projects
that reduce the impacts provided by agricultural development and the excessive consumption of
natural resources. However, there is still little knowledge about the acoustic insulation/absorption
behaviour of lignocellulosic materials. Hence, this study aimed to evaluate the acoustic properties
of five cement panels reinforced with the following lignocellulosic materials: eucalyptus,
sugarcane bagasse, coconut shell, coffee husk, and banana pseudostem, which ones have as a
reference a commercial plaster used as sealing in civil constructions. The proposed panels were
produced with each lignocellulosic material residue. It was produced three replicates for each
type including plaster (being 18 panels in total). The sound insertion loss (SIL) measurement of
the above-mentioned panels have been performed using an acoustical treated inexpensive facility
developed based on the literature. The characterization of the acoustic behaviour of the studied
materials were analysed according to the IEC (61260-1). The acoustic measurements have been
done in the range of 20 Hz to 20 kHz and the analysis in octave bands have been performed. To
make the analysis easier, the overall range of frequencies mentioned above was divided as ‘low’,
‘middle’ and ‘high’ ranges. Additionally, the measurement of thickness, density and porosity
structure parameters of the lignocellulosic samples have been performed. According to the results
and doing a trade-off analysis, the eucalyptus presented the overall best performance considering
the overall range of analysis, being the banana pseudostem and sugarcane bagasse materials as
good competitors
MADES FP7 EU project: Effective high level SysML/MARTE methodology for real-time and embedded avionics systems
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High-precision determination of the critical exponents for the lambda-transition of 4He by improved high-temperature expansion
We determine the critical exponents for the XY universality class in three
dimensions, which is expected to describe the -transition in He.
They are obtained from the analysis of high-temperature series computed for a
two-component model. The parameter is fixed such that
the leading corrections to scaling vanish. We obtain ,
, . These estimates improve previous
theoretical determinations and agree with the more precise experimental results
for liquid Helium.Comment: 8 pages, revte
Gravitational radiation from gamma-ray bursts as observational opportunities for LIGO and VIRGO
Gamma-ray bursts are believed to originate in core-collapse of massive stars.
This produces an active nucleus containing a rapidly rotating Kerr black hole
surrounded by a uniformly magnetized torus represented by two counter-oriented
current rings. We quantify black hole spin-interactions with the torus and
charged particles along open magnetic flux-tubes subtended by the event
horizon. A major output of Egw=4e53 erg is radiated in gravitational waves of
frequency fgw=500 Hz by a quadrupole mass-moment in the torus. Consistent with
GRB-SNe, we find (i) Ts=90s (tens of s, Kouveliotou et al. 1993), (ii)
aspherical SNe of kinetic energy Esn=2e51 erg (2e51 erg in SN1998bw, Hoeflich
et al. 1999) and (iii) GRB-energies Egamma=2e50 erg (3e50erg in Frail et al.
2001). GRB-SNe occur perhaps about once a year within D=100Mpc. Correlating
LIGO/Virgo detectors enables searches for nearby events and their spectral
closure density 6e-9 around 250Hz in the stochastic background radiation in
gravitational waves. At current sensitivity, LIGO-Hanford may place an upper
bound around 150MSolar in GRB030329. Detection of Egw thus provides a method
for identifying Kerr black holes by calorimetry.Comment: to appear in PRD, 49
Pion emission from the T2K replica target: method, results and application
The T2K long-baseline neutrino oscillation experiment in Japan needs precise
predictions of the initial neutrino flux. The highest precision can be reached
based on detailed measurements of hadron emission from the same target as used
by T2K exposed to a proton beam of the same kinetic energy of 30 GeV. The
corresponding data were recorded in 2007-2010 by the NA61/SHINE experiment at
the CERN SPS using a replica of the T2K graphite target. In this paper details
of the experiment, data taking, data analysis method and results from the 2007
pilot run are presented. Furthermore, the application of the NA61/SHINE
measurements to the predictions of the T2K initial neutrino flux is described
and discussed.Comment: updated version as published by NIM
Kaon Production and Kaon to Pion Ratio in Au+Au Collisions at \snn=130 GeV
Mid-rapidity transverse mass spectra and multiplicity densities of charged
and neutral kaons are reported for Au+Au collisions at \snn=130 GeV at RHIC.
The spectra are exponential in transverse mass, with an inverse slope of about
280 MeV in central collisions. The multiplicity densities for these particles
scale with the negative hadron pseudo-rapidity density. The charged kaon to
pion ratios are and
for the most central collisions. The ratio is lower than the same
ratio observed at the SPS while the is higher than the SPS result.
Both ratios are enhanced by about 50% relative to p+p and +p
collision data at similar energies.Comment: 6 pages, 3 figures, 1 tabl
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