The DOI matches its Crossref record; 15 of the 15 references it cites were found in a registry or an index.
Neutrino-“pasta” scattering: The opacity of nonuniform neutron-rich matter
Open accessAbstract
Neutron-rich matter at subnuclear densities may involve complex structures displaying a variety of shapes, such as spherical, slablike, and∕or rodlike shapes. These phases of the nuclear pasta are expected to exist in the crust of neutron stars and in core-collapse supernovae. The dynamics of core-collapse supernovae is very sensitive to the interactions between neutrinos and nucleons∕nuclei. Indeed, neutrino excitation of the low-energy modes of the pasta may allow for a significant energy transfer to the nuclear medium, thereby reviving the stalled supernovae shock. The linear response of the nuclear pasta to neutrinos is modeled via a simple semiclassical simulation. The transport mean free path for $\ensuremath{\mu}$ and $\ensuremath{\tau}$ neutrinos (and antineutrinos) is expressed in terms of the static structure factor of the pasta, which is evaluated using Metropolis Monte Carlo simulations.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Equation of State Calculations by Fast Computing Machines
Metropolis, N., Rosenbluth, A. W., Rosenbluth, M. N., Teller, A. H., & Teller, E. (1953) · The Journal of Chemical Physics · doi:10.1063/1.1699114 · Cited by 37,192
Combinatorial Optimization: Algorithms and Complexity.
Johnson, D. S., Papadimitriou, C. H., & Steiglitz, K. (1984) · The American Mathematical Monthly · doi:10.2307/2322374 · Cited by 5,942
Quantum theory of many-particle systems
Fetter, A. L., & Walecka, J. D. (1971) · Cited by 5,252
Combinatorial optimization:Algorithms and complexity
Rabiner, L. (1984) · IEEE Transactions on Acoustics, Speech, and Signal Processing · doi:10.1109/tassp.1984.1164450 · Cited by 3,576
Quantum Theory of Many Particle Systems
Fetter, A. L., Walecka, J. D., & Kadanoff, L. P. (1972) · Physics Today · doi:10.1063/1.3071096 · Cited by 2,652
Antiferromagnetism. The Triangular Ising Net
Wannier, G. H. (1950) · Physical Review · doi:10.1103/physrev.79.357 · Cited by 1,426
A generalized equation of state for hot, dense matter
Lattimer, J. M., & Douglas Swesty, F. (1991) · Nuclear Physics A · doi:10.1016/0375-9474(91)90452-c · Cited by 1,368
Infinite-ranged models of spin-glasses
Kirkpatrick, S., & Sherrington, D. (1978) · Physical Review B · doi:10.1103/physrevb.17.4384 · Cited by 1,006
A relativistic many-body theory of high density matter
Chin, S. A. (1977) · Annals of Physics · doi:10.1016/0003-4916(77)90016-1 · Cited by 565
Spin glass with non-random interactions
Villain, J. (1977) · Journal of Physics C Solid State Physics · doi:10.1088/0022-3719/10/10/014 · Cited by 420
The Weak Neutral Current and its Effects in Stellar Collapse
Freedman, D. Z., Schramm, D. N., & Tubbs, D. L. (1977) · Annual Review of Nuclear Science · doi:10.1146/annurev.ns.27.120177.001123 · Cited by 294
Quantum molecular dynamics approach to the nuclear matter below the saturation density
Maruyama, T., Niita, K., Oyamatsu, K., Maruyama, T., Chiba, S., & Iwamoto, A. (1998) · Physical Review C · doi:10.1103/physrevc.57.655 · Cited by 110
Clustering in nuclear matter at subsaturation densities
Peilert, G., Randrup, J., Horst Stöcker, B., & Greiner, W. (1991) · Physics Letters B · doi:10.1016/0370-2693(91)91611-x · Cited by 68
Classical simulations of heavy-ion collisions
Schlagel, T. J., & Pandharipande, V. R. (1987) · Physical Review C · doi:10.1103/physrevc.36.162 · Cited by 61
Classical-equations-of-motion calculations of high-energy heavy-ion collisions
Bodmer, A. R., Panos, C. N., & MacKellar, A. D. (1980) · Physical Review C · doi:10.1103/physrevc.22.1025 · Cited by 57
Cited by
Complexity in Strongly Correlated Electronic Systems
Dagotto, E. (2005) · Science · doi:10.1126/science.1107559 · Cited by 2,046
A statistical model for a complete supernova equation of state
Hempel, M., & Schaffner-Bielich, J. (2010) · Nuclear Physics A · doi:10.1016/j.nuclphysa.2010.02.010 · Cited by 638
Metadata
- Authors
- Horowitz, C. J., Pérez-García, M. A., & Piekarewicz, J.
- Venue
- Physical Review C
- Publisher
- American Physical Society (APS)
- Published
- 2004-04-27
- Volume
- 69
- Issue
- 4
- ISSN
- 0556-2813 (ISSN-L)
- 1089-490X
- OpenAlex
- W1990059845
- Cited by
- 259
- References
- 15
- FWCI
- 6.77
- Type
- journal article
- Language
- en
- Open access
- green
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
