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  <channel rdf:about="http://biblioteca.universia.net/vernivel.do?nivel=2208">
    <title>Nomenclatura Unesco &gt; (22) Física &gt; (2208) Nucleónica</title>
    <link>http://biblioteca.universia.net/vernivel.do?nivel=2208</link>
    <description>Mostrando recursos 1 - 20 de 235</description>
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    <dc:language>es</dc:language>
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  <image>
    <title>Universia-Recursos de Aprendizaje</title>
    <url>http://biblioteca.universia.net/img/logotipo.jpg</url>
    <link>http://biblioteca.universia.net/</link>
  </image>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=41607611">
    <title>Diffractive Contribution to the Elasticity and the Nucleonic Flux in the Atmosphere</title>
    <link>http://biblioteca.universia.net/ficha.do?id=41607611</link>
    <description>We calculate the average elasticity considering non-diffractive and single diffractive
interactions and perform an analysis of the cosmic-ray flux by means of an
analytical solution for the nucleonic diffusion equation. We show that the diffractive
contribution is important for the adequate description of the nucleonic and
hadronic fluxes in the atmosphere.
It is well known that the evolution of the nucleonic cosmic ray component is controlled
by two physical quantities related to high energy...</description>
    <dc:creator>J. Bell,R. J. M. Covolan,A. L. Godoi,J. Montanha,Gleb Wataghin</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=41519976">
    <title>Consistent Effective Description Of Nucleonic Resonances In An Unitary Relativistic Field-Theoret...</title>
    <link>http://biblioteca.universia.net/ficha.do?id=41519976</link>
    <description>High energy strong interaction physics is successfully described by the local renormalizable
gauge theory called Quantum--Chromo--Dynamics (QCD) with quarks and
gluons as "elementary" degrees of freedom, while intermediate energy strong interaction
physics shows up to be determined by a non--local, non--renormalizable effective
field theory (EFT) of "effective" degrees of freedom like mesons, ground state
baryons and resonances. The connection between high and intermediate physics is
establis...</description>
    <dc:creator>F. Kleefeld</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=41839722">
    <title>Consistent Effective Description Of Nucleonic Resonances In An Unitary Relativistic Field--Theore...</title>
    <link>http://biblioteca.universia.net/ficha.do?id=41839722</link>
    <description>High energy strong interaction physics is successfully described by the local renormalizable
gauge theory called Quantum--Chromo--Dynamics (QCD) with quarks and
gluons as "elementary" degrees of freedom, while intermediate energy strong interaction
physics shows up to be determined by a non--local, non--renormalizable effective
field theory (EFT) of "effective" degrees of freedom like mesons, ground state
baryons and resonances. The connection between high and intermediate physics is
establis...</description>
    <dc:creator>F. Kleefeld</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=44377735">
    <title>Nucleonic coal detector with independent, hydropneumatic suspension</title>
    <link>http://biblioteca.universia.net/ficha.do?id=44377735</link>
    <description>The design of a nucleonic, coal interface detector which measures the depth of coal on the roof and floor of a coal mine is presented. The nucleonic source and the nucleonic detector are on independent hydropneumatic suspensions to reduce the measurement errors due to air gap.</description>
    <dc:creator>Jones, E. W.; Handy, K.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=42917727">
    <title>Optimal configuration for a zero-g nucleonic fuel gage.</title>
    <link>http://biblioteca.universia.net/ficha.do?id=42917727</link>
    <description>Optimal configuration for zero-g nucleonic fuel gage</description>
    <dc:creator>Pfeifer, R. J.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=42895696">
    <title>Nucleonic measurements of cryogenic densities and qualities.</title>
    <link>http://biblioteca.universia.net/ficha.do?id=42895696</link>
    <description>Liquid and slush hydrogen density data measured by fast response nucleonic densitometer, reviewing liquid-vapor quality data obtained from cryogenic meter</description>
    <dc:creator>Cho, B. Y.; Scheiwe, J. P.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=44282451">
    <title>Nucleonic lunar ranging and tracking system Final report</title>
    <link>http://biblioteca.universia.net/ficha.do?id=44282451</link>
    <description>Nucleonic lunar ranging and tracking system for altitude measurement in lunar landing vehicles</description>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=539733">
    <title>Construction of gauge invariant effective nucleonic theories: functional
  approach</title>
    <link>http://biblioteca.universia.net/ficha.do?id=539733</link>
    <description>Starting from relativistic quantum field theories, describing interacting
nucleons and pions coupled to the dynamical electromagnetic field, the pion
degrees of freedom are eliminated by means of functional integration. Apart
from taking into account some operators perturbatively in $e$, e.g. the vacuum
polarization, this procedure is exact, giving effective theories for nucleons
and photons. The subsequent nonrelativistic reduction yields the corresponding
nonrelativistic quantum field theor...</description>
    <dc:creator>Naus, H. W. L.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=542611">
    <title>Nucleonic resonance effects in the $\phi$ meson photoproduction</title>
    <link>http://biblioteca.universia.net/ficha.do?id=542611</link>
    <description>The process $\gamma p \to \phi p$ close to threshold is investigated focusing
on the role played by the {\it s}- and {\it u}-channel nucleonic resonances.
For this purpose, a recent quark model approach, based on the $SU(6)\otimes
O(3)$ symmetry with an effective Lagrangian, is extended to the $\phi$ meson
photoproduction. Another non-diffractive process, the {\it t}-channel $\pi^0$
exchange, is also included. The diffractive contribution is produced by the
{\it t}-channel Pomeron exchange. C...</description>
    <dc:creator>Zhao, Q.; Didelez, J. -P.; Guidal, M.; Saghai, B.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=20960682">
    <title>Pairing properties of nucleonic matter employing dressed nucleons</title>
    <link>http://biblioteca.universia.net/ficha.do?id=20960682</link>
    <description>A survey of pairing properties of nucleonic matter is presented that includes
the off-shell propagation associated with short-range and tensor correlations.
For this purpose, the gap equation has been solved in its most general form
employing the complete energy and momentum dependence of the normal self-energy
contributions. The latter correlations include the self-consistent calculation
of the nucleon self-energy that is generated by the summation of ladder
diagrams. This treatment preserve...</description>
    <dc:creator>Müther, H.; Dickhoff, W. H.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=295010">
    <title>Diffractive Contribution to the Elasticity and the Nucleonic Flux in the
  Atmosphere</title>
    <link>http://biblioteca.universia.net/ficha.do?id=295010</link>
    <description>We calculate the average elasticity considering non-diffractive and single
diffractive interactions and perform an analysis of the cosmic-ray flux by
means of an analytical solution for the nucleonic diffusion equation. We show
that the diffractive contribution is important for the adequate description of
the nucleonic and hadronic fluxes in the atmosphere.</description>
    <dc:creator>Bellandi, J.; Covolan, R. J. M.; Godoi, A. L.; Montanha, J.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=21796070">
    <title>Nucleonic gamma-ray production in Pulsar Wind Nebulae</title>
    <link>http://biblioteca.universia.net/ficha.do?id=21796070</link>
    <description>Observations of the inner radian of the Galactic disk at very high energy
(VHE) gamma-rays have revealed at least 16 new sources. Besides shell type
super-nova remnants, pulsar wind nebulae (PWN) appear to be a dominant source
population in the catalogue of VHE gamma-ray sources. Except for the Crab
nebula, the newly discovered PWN are resolved at VHE gamma-rays to be spatially
extended (5-20 pc). Currently, at least 3 middle aged ($t&gt;10$ kyrs) PWN (Vela
X, G18.0-0.7, and G313.3+0.6 in the ``...</description>
    <dc:creator>Horns, D.; Aharonian, F.; Hoffmann, A. I. D.; Santangelo, A.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=322454">
    <title>Complete Set of Splitting Functions Relevant in the Evolution of
  Nucleonic Helicity Distributions</title>
    <link>http://biblioteca.universia.net/ficha.do?id=322454</link>
    <description>In this work, we show how the complete set of splitting functions relevant
for the evolution of various distribution functions describing nucleonic
helicity structure can be obtained in the light front Hamiltonian perturbation
theory using completely fixed light front gauge, $A^+=0$.</description>
    <dc:creator>Kundu, Rajen</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=444621">
    <title>Has Nucleonic Matter at the Critical Point Been Produced in Recent
  Multifragmentation Experiments?</title>
    <link>http://biblioteca.universia.net/ficha.do?id=444621</link>
    <description>For nuclei in five different mass regions the critical temperatures, at which
the surface tension vanishes, are derived from information on the liquid branch
of the coexistence curve. These critical temperatures increase with increasing
mass and, for higher masses are well above recently reported critical
temperatures obtained from Fisher Droplet model and percolation model analyses.
However, for the lowest mass region nuclei, with 30&lt;A&lt;60, this analysis
indicates that nucleonic matter has be...</description>
    <dc:creator>Natowitz, J. B.; Hagel, K.; Ma, Y.; Murray, M.; Qin, L.; Shlomo, S.; Wada, R.; Wang, J.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=543005">
    <title>Nucleonic resonance excitations and "missing resonances" in the $\omega$
  meson photoproduction</title>
    <link>http://biblioteca.universia.net/ficha.do?id=543005</link>
    <description>In this work, an improved quark model approach to the $\omega$ meson
photoproduction with an effective Lagrangian is reported. The {\it t}-channel
{\it natural} parity exchange is consistently taken into account through the
Pomeron exchange, while the {\it unnatural} parity exchange is described by the
$\pi^0$ exchange. It shows that with very limited number of parameters, all the
available experimental data in the low energy regime can be consistently
accounted for in this framework. Effects...</description>
    <dc:creator>Zhao, Q.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=538169">
    <title>Is it Possible to Describe Short-range NN Correlations in Nuclei on the
  Basis of Nucleonic Degr...</title>
    <link>http://biblioteca.universia.net/ficha.do?id=538169</link>
    <description>Assuming that NN interaction is modified inside a nucleus by a specific way,
phenomenological effective broad core (BC) NN potential is constructed. It is
shown that increase in the width of repulsive core lets us describe the Coulomb
form factors of few-body nuclei on the basis of nucleonic degrees of freedom
only.</description>
    <dc:creator>Ryzhikh, G. G.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=43063387">
    <title>Solar-cycle dependence of galactic cosmic ray flux. II - The correlation between the nucleonic fl...</title>
    <link>http://biblioteca.universia.net/ficha.do?id=43063387</link>
    <description>To investigate the relationship between solar activity and cosmic-ray modulation, time series of the nucleonic flux and of solar plages, sunspots, centimeter radio noise, and the brightness of the white-light corona at 1.1 and 1.5 solar radii from the center of sun are cross-correlated. Data pertain to the years 1964-1967 during the ascending phase of the current solar cycle. The amplitudes and phases of correlation functions for filtered and unfiltered indices are discussed. The existence of...</description>
    <dc:creator>Parker, G. D.; Chasson, R. L.; Hansen, R. T.; Hansen, S. F.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=43183036">
    <title>Improved nucleonic coal-thickness monitor</title>
    <link>http://biblioteca.universia.net/ficha.do?id=43183036</link>
    <description>Design for coal-thickness-sensing instrument features independent hydropneumatic suspension of radiation source and detector. Monitor uses source and detector which are independently mounted, to follow contour of coal surface more closely and to eliminate errors caused by variations in airgap along radiation path. Device may help to bring fully-automated coal mining closer to reality.</description>
    <dc:creator>Crouch, C. E.; Rose, S. D.; Jones, E. W.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=40123610">
    <title>Nucleonic thickness gauges -- a SAPPHO pair</title>
    <link>http://biblioteca.universia.net/ficha.do?id=40123610</link>
    <dc:creator>Rothwell, R.</dc:creator>
  </item>
  <item rdf:about="http://biblioteca.universia.net/ficha.do?id=446369">
    <title>Equation of state of nucleonic matter</title>
    <link>http://biblioteca.universia.net/ficha.do?id=446369</link>
    <description>The nuclear equation of state (EoS) is investigated by flow phenomena in
relativistic heavy-ion collisions, both in transverse and radial direction, in
comparison to experimental data from 150 A MeV to 11 A GeV. To this aim the
collective dynamics of the nucleus-nucleus collision is described within a
transport model of the coupled channel RBUU type. There are two factors which
dominantly determine the baryon flow at these energies: the momentum dependence
of the scalar ($U_S$) and vector pot...</description>
    <dc:creator>Cassing, W.</dc:creator>
  </item>
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