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image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Physical Review Carrow_drop_down
image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao
Physical Review C
Article . 1992 . Peer-reviewed
License: APS Licenses for Journal Article Re-use
Data sources: Crossref
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Nucleon in nuclear matter

Authors: , Banerjee;

Nucleon in nuclear matter

Abstract

We use the toy model of baryon bag formation to study the changes in the structure of a nucleon when it is placed in nuclear matter. Several interesting qualitative results have been found. We find that ${\mathit{M}}^{\mathrm{*}}$, the nucleon mass in nuclear matter, does not scale with ${\mathit{F}}_{\mathrm{\ensuremath{\pi}}}^{\mathrm{*}}$, the latter being the value of the \ensuremath{\sigma} field in nuclear matter. The product ${\mathit{M}}^{\mathrm{*}}$〈${\mathit{r}}^{2}$${\mathrm{〉}}^{1/2\mathrm{*}}$ is nearly independent of nuclear density. The coupling constant ${\mathit{g}}_{\mathrm{\ensuremath{\sigma}}\mathit{N}\mathit{N}}^{\mathrm{*}}$ decreases with density. The coupling constant ${\mathit{g}}_{\mathrm{\ensuremath{\pi}}\mathit{N}\mathit{N}}^{\mathrm{*}}$/2${\mathit{M}}^{\mathrm{*}}$ and the rho-nucleon tensor coupling constant, ${\mathit{f}}_{\mathrm{\ensuremath{\rho}}\mathit{N}\mathit{N}}^{\mathrm{*}}$/2${\mathit{M}}^{\mathrm{*}}$, increase with density at the same rate. The coupling constants ${\mathit{g}}_{\mathrm{\ensuremath{\omega}}\mathit{N}\mathit{N}}^{\mathrm{*}}$ and ${\mathit{g}}_{\mathrm{\ensuremath{\rho}}}^{\mathrm{*}}$ also increase at the same rate, but the rate itself is low. We find that ${\mathit{M}}^{\mathrm{*}}$+${\mathit{g}}_{\mathrm{\ensuremath{\sigma}}\mathit{N}\mathit{N}}^{\mathrm{*}}$(${\mathit{F}}_{\mathrm{\ensuremath{\pi}}}$-${\mathit{F}}_{\mathrm{\ensuremath{\pi}}}^{\mathrm{*}}$) is approximately independent of the nuclear density. The magnetic moments increase, while ${\mathit{g}}_{\mathit{A}}^{\mathrm{*}}$(0) decreases. At half the normal density these changes are in the range 3--7 % depending on the parameters used. We discuss briefly the implications of these results on the properties of nuclear matter.

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    influence
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
31
Average
Top 10%
Top 10%
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