$w_d=-1$ in interacting quintessence model

$XMM-Newton$ $Ω$ project: III. Gas mass fraction shape in high redshift clusters

$\bar{SL}(4,R)$ Embedding for a 3D World Spinor Equation

$\hat{Q}$ operator for canonical quantum gravity

$\hbar$ as parameter of Minkowski metric in effective theory

$\La \to 0$ limit of 2+1 Quantum Gravity for arbitrary genus

$\mathcal{N}=1$ SUGRA Noether Charges

$\rm Ψ= W e^{\pm Φ}$ quantum cosmological solutions for Class A Bianchi Models

$^1$S$_0$ Neutron Pairing vs Observations of Cooling Neutron Stars

$^3$He experimentum crucis for Dark Matter puzzles

$^6$Li Production by the Radiative Decay of Long-Lived Particles

$^7$Li Abundances in Halo Stars: Testing Stellar Evolution Models and the Primordial $^7$Li Abundance

$^{12}$C/$^{13}$C ratio in planetary nebulae from the IUE archives

$^{13}CO(J = 1 -- 0)$ Depression in Luminous Starburst Mergers

$^{180}$Ta production in the classical s-process

$^{187}$Re(\gamm,n) cross section close to and above the neutron threshold

$^{26}$Al production from magnetically induced extramixing in AGB Stars

$^{92}$Mo($α,α$)$^{92}$Mo scattering,the $^{92}$Mo--$α$ optical potential, and the $^{96}$Ru($γ,α$)$^{92}$Mo reaction rate at astrophysically relevant energies

$β$--Radioactive Cosmic Rays in a diffusion model: test for a local bubble?

$β$-exponential inflation