Renormalization group approach to neutron matter: quasiparticle interactions, superfluid gaps and the equation of state
arXiv:nucl-th/0207004 · doi:10.1016/S0375-9474(02)01290-3
Abstract
Renormalization group methods can be applied to the nuclear many-body problem using the approach proposed by Shankar. We start with the two-body low momentum interaction V_{low k} and use the RG flow from the particle-hole channels to calculate the full scattering amplitude in the vicinity of the Fermi surface. This is a new straightforward approach to the many-body problem which is applicable also to condensed matter systems without long-range interactions, such as liquid 3He. We derive the one-loop renormalization group equations for the quasiparticle interaction and the scattering amplitude at zero temperature. The RG presents an elegant method to maintain all momentum scales and preserve the antisymmetry of the scattering amplitude. As a first application we solve the RG equations for neutron matter. The resulting quasiparticle interaction includes effects due to the polarization of the medium, the so-called induced interaction of Babu and Brown. We present results for the Fermi liquid parameters, the equation of state of neutron matter and the 1S0 superfluid pairing gap.
31 pages, 9 figures, minor revisions, to appear in Nucl. Phys. A
Cited by in corpus (149)
- Physics of Neutron Star Crusts
- Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII: Stiffness and stability of neutron-star matter
- Minimal Cooling of Neutron Stars: A New Paradigm
- Neutron stars - cooling and transport
- Neutron Stars and the Nuclear Equation of State
- The BCS-BEC crossover: From ultra-cold Fermi gases to nuclear systems
- Strongly paired fermions: Cold atoms and neutron matter
- Low-density neutron matter
- Neutrino Emission from Cooper Pairs and Minimal Cooling of Neutron Stars
- Superfluidity in nuclear systems and neutron stars
- Long Type I X-ray Bursts and Neutron Star Interior Physics
- Spatial structure of neutron Cooper pair in low density uniform matter
- Equation of state sensitivities when inferring neutron star and dense matter properties
- Resonant Fermi gases with a large effective range
- Neutron Matter from Low to High Density
- Polarization contributions to the spin-dependence of the effective interaction in neutron matter
- Low-momentum interaction in few-nucleon systems
- Tests of the nuclear equation of state and superfluid and superconducting gaps using the Cassiopeia A neutron star
- Microscopic calculations and energy expansions for neutron-rich matter
- Upper Limit on the QCD Axion Mass from Isolated Neutron Star Cooling
- Induced P-wave Superfluidity in Asymmetric Fermi Gases
- Limit on the Axion Decay Constant from the Cooling Neutron Star in Cassiopeia A
- Equation of state of superfluid neutron matter and the calculation of pairing gap
- Nuclear chiral dynamics and thermodynamics
- The Virial Equation of State of Low-Density Neutron Matter
- Heavy Baryons in Compact Stars
- Constraints on Axion-like Particles and Nucleon Pairing in Dense Matter from the Hot Neutron Star in HESS J1731-347
- Spin and spin-isospin instabilities in asymmetric nuclear matter at zero and finite temperatures using Skyrme functionals
- Superfluidity and Superconductivity in Neutron Stars
- Magnetic, thermal and rotational evolution of isolated neutron stars
- BCS-BEC crossover of neutron pairs in symmetric and asymmetric nuclear matter
- Pinning down the superfluid and measuring masses using pulsar glitches
- Forecasting neutron star temperatures: predictability and variability
- Effective pairing interactions with isospin density dependence
- Pairing in high-density neutron matter including short- and long-range correlations
- Pairing in high-density neutron matter including short- and long-range correlations
- What is the nature of the HESS J1731-347 compact object?
- Reaction rates and transport in neutron stars
- Magnetic neutron star cooling and microphysics
- NS 1987A in SN 1987A
- The , interaction in finite volume and the nature of the resonance
- Axion Emission Can Explain a New Hard -ray Excess from Nearby Isolated Neutron Stars
- Equation of state of low--density neutron matter and the pairing gap
- Cooling of hypernuclear compact stars
- The entrainment matrix of a superfluid neutron-proton mixture at a finite temperature
- Superfluid Properties of the Inner Crust of Neutron Stars
- Quiescent thermal emission from neutron stars in LMXBs
- 1S0 Proton and Neutron Superfluidity in beta-stable Neutron Star Matter
- Non-empirical pairing energy functional in nuclear matter and finite nuclei
- Diffusive nuclear burning in cooling simulations and application to new temperature data of the Cassiopeia A neutron star
- Nuclear Superfluidity and Specific Heat in the Inner Crust of Neutron Stars
- Constraints on Skyrme Equations of State from Properties of Doubly Magic Nuclei and Ab-Initio Calculations of Low-Density Neutron Matter
- Goldstone Bosons in the 3P2 Superfluid Phase of Neutron Matter and Neutrino Emission
- The Neutrino Response of Low-Density Neutron Matter from the Virial Expansion
- Pairing in neutron matter: New uncertainty estimates and three-body forces
- Scattering of unstable particles in a finite volume: the case of pi rho scattering and the a1(1260) resonance
- Late time cooling of neutron star transients and the physics of the inner crust
- Superfluid Fermi atomic gas as a quantum simulator for the study of neutron-star equation of state
- Vertex renormalization in weak decays of Cooper pairs and cooling compact stars
- An effective field theory for coupled-channel scattering
- Spatial structure of a vortex in low density neutron matter
- Lattice Calculation of Thermal Properties of Low-Density Neutron Matter with Pionless NN Effective Field Theory
- Thermal evolution of relativistic hyperonic compact stars with calibrated equations of state
- Superfluid Response and the Neutrino Emissivity of Neutron Matter
- Cooling of Neutron Stars with Strong Toroidal Magnetic Fields
- Neutron matter at finite temperature
- Dependence of the BCS 1S0 superfluid pairing gap on nuclear interactions
- The structure of nuclear systems derived from low momentum nucleon-nucleon potentials
- Chiral effective field theory calculations of neutrino processes in dense matter
- In-medium enhancement of the modified Urca neutrino reaction rates
- Neutrino processes in partially degenerate neutron matter
- The thermal state of KS 1731-260 after 14.5 years in quiescence
- Effective density functionals beyond mean field
- Static response of Fermi liquids with tensor interactions
- Pairing Matrix Elements and Pairing Gaps with Bare, Effective and Induced Interactions
- Renormalization group approach to interacting fermion systems in the two-particle-irreducible formalism
- A cooling neutron star crust after recurrent outbursts: Modelling the accretion outburst history of Aql X-1
- Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
- On the superfluid properties of the inner crust of neutron stars
- Unified approach to structure factors and neutrino processes in nucleon matter
- Nuclear matter with Brown-Rho-scaled Fermi liquid interactions
- Cooling of young neutron stars and dark gauge bosons
- Effective Field Theory and Finite Density Systems
- Screening of nuclear pairing in nuclear and neutron matter
- Low-momentum NN interactions and all-order summation of ring diagrams of symmetric nuclear matter
- Neutrino Bremsstrahlung in Neutron Matter from Effective Nuclear Interactions
- Cooling of hypernuclear compact stars: Hartree-Fock models and high-density pairing
- Rapid neutron star cooling triggered by dark matter
- The neutron polaron as a constraint on nuclear density functionals
- Energy-density functionals inspired by effective-field theories: Applications to neutron drops
- Non-perturbative Extraction of the Effective Mass in Neutron Matter
- The role of mass, equation of state and superfluid reservoir in large pulsar glitches
- Weinberg Eigenvalues and Pairing with Low-Momentum Potentials
- Low-momentum Hyperon-Nucleon Interactions
- Cooling of neutron stars in soft X-ray transients
- Chiral three-nucleon forces and pairing in nuclei
- 3D code for MAgneto-Thermal evolution in Isolated Neutron Stars, MATINS: thermal evolution and lightcurves
- Impact of axions on the Cassiopea A neutron star cooling
- The impact of asymmetric dark matter on the thermal evolution of nucleonic and hyperonic compact stars
- Superfluid LDA (SLDA): Local Density Approximation for Systems with Superfluid Correlations
- Screening and anti-screening of the pairing interaction in low-density neutron matter
- Microscopic Study of Superfluidity in Dilute Neutron Matter
- Correlation functions for a di-neutron condensate in asymmetric nuclear matter
- Static response, collective frequencies and ground state thermodynamical properties of spin saturated two-component cold atoms and neutron matter
- Dispersion and decay of collective modes in neutron star cores
- Long-wavelength spin- and spin-isospin correlations in nucleon matter
- Linear Response Theory with finite-range interactions
- Mean Field Calculation of Thermal Properties of Simple Nucleon Matter on a Lattice
- Many-body approximations to the superfluid gap and critical temperature in pure neutron matter
- Skyrmion Stars: Astrophysical motivations and implications
- Finite-size effects and collective vibrations in the inner crust of neutron stars
- Landau-Migdal vs. Skyrme
- Equation of state of superfluid neutron matter with low-momentum interactions
- Gapless neutron superfluidity can explain the late time cooling of transiently accreting neutron stars
- Low-momentum interactions for nuclei
- Spin response of a normal Fermi liquid with noncentral interactions
- Long-term temperature evolution of neutron stars undergoing episodic accretion outbursts
- Lee-Yang-inspired energy-density functional including contributions from -wave scattering
- Off-shell pairing correlations from meson-exchange theory of nuclear forces
- Dineutron correlations and BCS-BEC crossover in nuclear matter with the Gogny pairing force
- Crust Cooling Models are Insensitive to the Crust-Core Transition Pressure for Realistic Equations of State
- Renormalization group and Fermi liquid theory for many-nucleon systems
- Deep crustal heating by neutrinos from the surface of accreting neutron stars
- Hybrid cooling of the Cassiopeia A neutron star
- Spin excitonic and diffusive modes in superfluid Fermi liquids
- Current Status of Nuclear Physics Research
- Variational and parquet-diagram calculations for neutron matter. III. S-wave pairing
- Isospin Dependence of 1S0 Proton and Neutron Superfluidity in Asymmetric Nuclear Matter
- Flux Relaxation after two outbursts of the magnetar SGR 162741 and possible hard X-ray emission
- Neutron localization induced by the pairing field in an inhomogeneous neutron matter
- Liquid-gas instability and superfluidity in nuclear matter
- Gapless neutron superfluidity in the crust of the accreting neutron stars KS 1731-260 and MXB 1659-29
- Foundations of Strangeness Nuclear Physics derived from chiral Effective Field Theory
- Superfluid neutron matter with a twist
- Finite-temperature infinite matter with effective-field-theory-inspired energy-density functionals
- Neutron star cooling within the equation of state with induced surface tension
- Probing Strong Field Gravity and Ultra-Dense Matter with the Structure and Thermal Evolution of Neutron Stars
- Novel effects of electromagnetic interaction on the correlation of nucleons in nuclear matter
- Neutrino emission in neutron matter from magnetic moment interactions
- Strong-coupling effects of pairing fluctuations, and Anderson-Bogoliubov mode in neutron S superfluids in neutron stars
- Pairing effects on neutron matter equation of state and symmetry energy at subsaturation densities
- Fast neutron star cooling in light of the PREX-2 experiment
- Cold atoms beyond atomic physics
- Neutron matter at the interface(s): static response and effective mass
- Nuclear interactions from the renormalization group
- Renormalization-group approach to the Kohn-Luttinger superconductivity: Amplification of the pairing gap from to
- First detection of X-ray pulsations and spectrum of the high Galactic latitude pulsar PSR J0837-2454 and direct Urca cooling implications
- Hartree shift and pairing gap in ultracold Fermi gases in the framework of low-momentum interactions
- A "Hyperburst" in the MAXI J0556-332 Neutron Star: Evidence for a New Type of Thermonuclear Explosion