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Abnormal dense and dilute nuclear systems

E. E. Kolomeitsev, D. N. Voskresensky

Abstract

Researchers have long been interested in exotic states of matter. In the early 1970s, Migdal proposed the existence of metastable or stable nuclei containing a pion condensate, and Bodmer posited the existence of collapsed nuclei with a quark core. Lee and Wick proposed that compressed nuclear matter could undergo a phase transition into a scalar condensate state with effectively very light baryons. In the mid-1980s, Witten pointed out that strange quark matter may be an absolutely stable form of matter that can exist in the form of quark strangelets. These hypotheses stimulated large experimental efforts to detect these states in heavy-ion collisions and in terrestrial samples. Additionally, the cosmos is the arena for a broad search for traces of exotic matter in compact objects and other energetic phenomena. We review various approaches and arguments for the possibility of abnormal states of matter, including metastable and stable dense objects with condensates, as well as dilute nuclear objects. Among these, we discuss scalar condensate and p-wave and s-wave pion condensations in dense nuclear systems and the formation of a $Δ$ resonance matter. Then we consider a scalar mode condensation triggered by the Pomeranchuk instability in dilute nuclear matter, and clustering. We also mention recent ideas that a relativistic rotation and a dark-matter component may stabilize abnormal nuclear systems. Finally, we list some observational anomalies that cannot yet be appropriately explained by conventional physics.

Abnormal dense and dilute nuclear systems

Abstract

Researchers have long been interested in exotic states of matter. In the early 1970s, Migdal proposed the existence of metastable or stable nuclei containing a pion condensate, and Bodmer posited the existence of collapsed nuclei with a quark core. Lee and Wick proposed that compressed nuclear matter could undergo a phase transition into a scalar condensate state with effectively very light baryons. In the mid-1980s, Witten pointed out that strange quark matter may be an absolutely stable form of matter that can exist in the form of quark strangelets. These hypotheses stimulated large experimental efforts to detect these states in heavy-ion collisions and in terrestrial samples. Additionally, the cosmos is the arena for a broad search for traces of exotic matter in compact objects and other energetic phenomena. We review various approaches and arguments for the possibility of abnormal states of matter, including metastable and stable dense objects with condensates, as well as dilute nuclear objects. Among these, we discuss scalar condensate and p-wave and s-wave pion condensations in dense nuclear systems and the formation of a resonance matter. Then we consider a scalar mode condensation triggered by the Pomeranchuk instability in dilute nuclear matter, and clustering. We also mention recent ideas that a relativistic rotation and a dark-matter component may stabilize abnormal nuclear systems. Finally, we list some observational anomalies that cannot yet be appropriately explained by conventional physics.

Paper Structure

This paper contains 24 sections, 74 equations, 11 figures.

Figures (11)

  • Figure 1: Potential (\ref{['Lee-U']}) for $\mu>0$, $\lambda>0$ and $0<\delta <1 - 2 \sqrt{2}/3$.
  • Figure 2: Difference in the energy density (\ref{['Lee-Edens']}) due to the development of the scalar field for ISM as function of $\phi$ for various nucleon densities calculated with the model parameters (\ref{['Lee-param']}).
  • Figure 3: Effective nucleon mass for ISM as a function of the nucleon density. Solid line is calculated for the Lee-Wick model with parameters (\ref{['Lee-param']}). Dashed line is drawn for $\delta=0.02$. Dash-dotted line corresponds to the RMF model (\ref{['Lee-W']}) with parameters (\ref{['Lee-W-param']}).
  • Figure 4: Binding energy per nucleon (\ref{['Ebind-def']}) for ISM as a function of nucleon density. Difference in the energy density (\ref{['Lee-Edens']}) due to the development of the scalar field is calculated for parameters (\ref{['Lee-param']}). Solid line shows the result of the Lee-Wick model. Dashed lines include nucleon-nucleon interaction term (\ref{['k-correl']}). The dash-dotted curve shows the RMF calculation with parameters (\ref{['Lee-W-param']}).
  • Figure 5: Potentials of the scalar field for the Lee-Wick model (\ref{['Lee-U']}) with parameters (\ref{['Lee-param']}) and for the RMF model with parameters (\ref{['Lee-W-param']}) as functions of the dimensionless scalar field. Dots show the values of the dimensionless magnitude of the scalar field for five values of the nucleon density from $1\,n_0$ till $5\,n_0$ with the step $1\,n_0$.
  • ...and 6 more figures