Cited by 211Quantum Chromodynamics and Particle InteractionsHigh-Energy Particle Collisions ResearchPulsars and Gravitational Waves Research

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

Exotic Phases of Hadronic Matter and their Astrophysical Application

Alcock, C, Olinto, A·1988·Annual Review of Nuclear and Particle Science

DOI 10.1146/annurev.ns.38.120188.001113

Open this paper in CoChat — free account

Abstract

Following a major shortage of 99Mo in the 2009–2010 period, concern grew that the aging reactor production facilities needed to be replaced. Most producers were using highly enriched 235U (HEU) as the target material. The Organisation for Economic Co-...Read More

Integrity signals

Registry

Crossref · 10.1146/annurev.ns.38.120188.001113

Cites

1 of 1 references verified0 citation errors · 0 not checkable

Statistics

Recomputing p-values needs the paper’s full text.

Claims the paper makes

This paper’s full text isn’t openly available, so its claims and self-check weren’t run. The registry and citation checks still apply.

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

The Origin and Evolution of Neutron Stars
(1987) · Springer eBooks · doi:10.1007/978-94-009-3913-4 · Cited by 221

Show all 1 references

Sorted by citations

Items 101–200 of 210

Properties of strange quark matter under strong rotation
Sun, F., & Huang, A. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.106.076007 · Cited by 15
Quark stars with isotropic matter in Hořava gravity and Einstein–æther theory
Panotopoulos, G., Vernieri, D., & Lopes, I. P. (2020) · The European Physical Journal C · doi:10.1140/epjc/s10052-020-8105-5 · Cited by 14
Dynamical effects of quantum chromodynamics on the surface tension of a cold strange quark nugget
Parija, B. C. (1993) · Physical Review C · doi:10.1103/physrevc.48.2483 · Cited by 14
Structure of Quark Stars
Weber, F., Orsaria, M. G., Rodrigues, H., & Yang, S. H. (2012) · LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) · Cited by 13
Cooling of a rotating strange star in the color superconducting phase with a crust
Yu, Y.-W., & Zheng, X. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20054184 · Cited by 13
Anisotropy in cosmic rays from internal transitions in neutron stars
Pérez-García, M. Á., Kotera, K., & Silk, J. I. (2013) · Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · doi:10.1016/j.nima.2013.11.007 · Cited by 12
Prospects for macroscopic dark matter detection at space-based and suborbital experiments
Anchordoqui, L. A., Bertaina, M. E., Casolino, M., Eser, J., Krizmanic, J. F., Olinto, A. V., Otte, A. N., Paul, T. C., Piotrowski, L. W., Reno, M. H., et al. (2021) · Europhysics Letters (EPL) · doi:10.1209/0295-5075/ac115f · Cited by 12
Self-citation
Search for neutral strange quark matter in high energy heavy ion collisions
Armstrong, T. A., Barish, K. N., Bennett, S. J., Chikanian, A., Coe, S. D., Cormier, T. M., de Cataldo, G., Davies, R., Dee, P. R., Diebold, G. E., et al. (1999) · Physical Review C · doi:10.1103/physrevc.59.r1829 · Cited by 12
Cosmic technicolor nuggets
Frieman, J. A., & Giudice, G. F. (1991) · Nuclear Physics B · doi:10.1016/0550-3213(91)90308-k · Cited by 12
Strangeness in stellar matter
Prakash, M., & Lattimer, J. M. (1998) · Nuclear Physics A · doi:10.1016/s0375-9474(98)00309-1 · Cited by 12
Strange stars
Alcock, C. R. (1991) · Nuclear Physics B - Proceedings Supplements · doi:10.1016/0920-5632(91)90305-x · Cited by 12
Self-citation
Thermal relaxation and cooling of quark stars with a strangelet crust
Campos, J. J. Z., Sales, T., Jaikumar, P., & Negreiros, R. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202243148 · Cited by 11
Color-flavor locked strange stars admixed with mirror dark matter and the observations of compact stars
Yang, S., & Pi, C. (2024) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2024/09/052 · Cited by 12
Impact of strange quark matter nuggets on pycnonuclear reaction rates in the crusts of neutron stars
Golf, B., Hellmers, J., & Weber, F. (2009) · Physical Review C · doi:10.1103/physrevc.80.015804 · Cited by 11
Strange stars at finite magnetic field
Phukon, T. C. (2000) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.62.023002 · Cited by 11
Axions and the QCD phase transition
Hindmarsh, M. B. (1992) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.45.1130 · Cited by 11
A family of well behaved charge analogues of Durgapal’s perfect fluid exact solution in general relativity II
Murad, M. H., & Fatema, S. (2012) · Astrophysics and Space Science · doi:10.1007/s10509-012-1320-2 · Cited by 10
Mergers of binary stars: the ultimate heavy-ion experience
Prakash, M., Ratkovi, S. A., & Lattimer, J. M. (2004) · Journal of Physics G Nuclear and Particle Physics · doi:10.1088/0954-3899/30/8/108 · Cited by 10
Exploring the structural properties of anisotropic dark matter-admixed quark stars
Panotopoulos, G. P., Rincón, Á., & Lopes, I. P. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101972 · Cited by 9
Implications of f ( R , T ) gravity on the complexity factor of a physically consistent charged anisotropic stellar model
Zubair, M., Azmat, H., Güdekli, E., Alhowaity, A., & Hamam, H. (2022) · New Astronomy · doi:10.1016/j.newast.2022.101996 · Cited by 9
Baryon number transport in a cosmic QCD-phase transition
Jedarnzik, K., & Fuller, G. M. (1995) · Nuclear Physics B · doi:10.1016/0550-3213(95)00097-c · Cited by 9
Deconfinement of nonstrange hadronic matter with nucleons and Δ baryons to quark matter in neutron stars
Sen, D., & Jha, T. K. (2018) · International Journal of Modern Physics D · doi:10.1142/s0218271819500408 · Cited by 9
The High Density Interiors of Neutron Stars
Baym, G. (1991) · Springer eBooks · doi:10.1007/978-94-011-3536-8_2 · Cited by 9
Radial Oscillations of Dark Matter Stars Admixed with Dark Energy
Sepúlveda, C., & Panotopoulos, G. (2024) · Universe · doi:10.3390/universe10010041 · Cited by 8
Unmasking strange dwarfs with gravitational-wave observations
Perot, L., Nicolas Chamel, A., & Vallet, P. (2023) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.107.103004 · Cited by 7
STRANGENESS IN NEUTRON STARS
Weber, F., HO, A., Negreiros, R., & Rosenfield, P. A. (2007) · International Journal of Modern Physics D · doi:10.1142/s0218271807009966 · Cited by 7
Non-Newtonian gravity in strange stars and constraints from the observations of compact stars
Pi, C., & Yang, S. (2021) · New Astronomy · doi:10.1016/j.newast.2021.101670 · Cited by 7
A Cluster-Theoretical Approach to Saturation Property of Strange Quark Systems in Constituent Quark Model
Ishii, M., & Tamagaki, R. (1992) · Progress of Theoretical Physics · doi:10.1143/ptp.87.969 · Cited by 7
EUSO-SPB2 sensitivity to macroscopic dark matter
Paul, T. C., Reese, S. T., Anchordoqui, L. A., & Olinto, A. V. (2021) · International Cosmic Ray Conference · doi:10.22323/1.395.0519 · Cited by 7
“Among the most appealing macro candidates is Witten’s proposal [12] wherein the QCD phase transition in the early universe resulted in an abundance of baryons alongside macroscopically sized nuggets of strange quark matter [13, 14], with a density ρs ∼ 3.”
Self-citation
Color-singlet strangelets at finite temperature
Mustafa, M. G., & Ansari, A. (1997) · Physical Review C · doi:10.1103/physrevc.55.2005 · Cited by 7
Quark matter and cosmology
Schramm, D. N., Fields, B. D., & Thomas, D. (1992) · Nuclear Physics A · doi:10.1016/0375-9474(92)90579-9 · Cited by 7
Cooling of strange stars in the color-flavor locked phase with a rotating crust Cooling of strange stars in the color-flavor locked phase with a rotating crustPreprint
Yu, Y.-W., Yunwei, Z. X. Y., & Xiaoping, Z. (2004) · arXiv (Cornell University) · doi:10.48550/arxiv.astro-ph/0411023 · Cited by 7
Tidal Love numbers of anisotropic stars within the complexity factor formalism
Rincón, Á., Panotopoulos, G., & Lopes, I. P. (2024) · Chinese Journal of Physics · doi:10.1016/j.cjph.2024.10.034 · Cited by 6
Dependence of maximum mass of strange star on finite strange quark mass (m s ≠ 0)
Goswami, K. B., Saha, A., & Chattopadhyay, P. K. (2022) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ac7f78 · Cited by 6
Could strange stars be in the color-flavor-locked phase: Tested by their thermal evolutions
Cheng, Q., Yu, Y.-W., & Zheng, X. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.87.063009 · Cited by 6
The microsecond old universe — Relics of QCD phase transition
Sinha, B. (2014) · International Journal of Modern Physics A · doi:10.1142/s0217751x14300245 · Cited by 6
Density dependence of quark masses and stability of color-flavor locked phases
Zhang, X., & Li, X. (2005) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.72.054021 · Cited by 6
Neutron star interiors and the equation of state of ultra-dense matter
Weber, F., Negreiros, R., Rosenfield, P., & Cuadrat, A. T. (2006) · CERN Document Server (European Organization for Nuclear Research) · Cited by 6
Luminosity evolution of strange dwarf stars
Benvenuto, O. G., & Althaus, L. G. (1996) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.53.635 · Cited by 6
A study on anisotropic compact stellar model under color-flavor locked equation of state
Das, S., Ray, S., Khlopov, M., Parida, B. K., Chakraborty, K., & Pal, S. K. (2024) · Chinese Journal of Physics · doi:10.1016/j.cjph.2024.04.001 · Cited by 5
DARK MATTER: An Introduction
Schramm, D. N. (1997) · Springer eBooks · doi:10.1007/978-94-009-0053-0_6 · Cited by 5
Electrically charged strange quark stars with anisotropic matter: exact analytical solution
Panotopoulos, G., & Lopes, I. P. (2020) · General Relativity and Gravitation · doi:10.1007/s10714-020-02701-2 · Cited by 5
On Exotic Objects Made of Dark Energy and Dark Matter: Mass-to-Radius Profiles and Tidal Love Numbers
Sepúlveda, C., & Panotopoulos, G. (2023) · Galaxies · doi:10.3390/galaxies11050101 · Cited by 5
Neutrino sparking and the neutron→strange stars conversion
Horvath, J. E., & Vucetich, H. (1998) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.59.023003 · Cited by 5
New window on strange quark matter as the ground state of strongly interacting matter
Soni, V., & Bhattacharya, D. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.69.074001 · Cited by 5
Maximum Mass of Strange Stars and Pulsars with the Most Accurately Measured Masses
Vartanyan, Y. L., Grigoryan, A. K., & Shahinyan, H. A. (2015) · Astrophysics · doi:10.1007/s10511-015-9382-9 · Cited by 5
Anisotropic quark stars within 4D Einstein–Gauss–Bonnet gravity
Tangphati, T., Panotopoulos, G., Banerjee, A., & Pradhan, A. (2023) · International Journal of Geometric Methods in Modern Physics · doi:10.1142/s0219887824500117 · Cited by 4
Constraining mass–radius limit of gravitationally decoupled binary compact star mergers PSR J0952-0607 and GW200210 generated by dual matter density profiles
Maurya, S. K., Jasim, M. K., Errehymy, A., Channuie, P., Mustafa, G., & Dönmez, O. (2025) · The European Physical Journal C · doi:10.1140/epjc/s10052-025-13917-4 · Cited by 4
Role of Quark Matter and Color Superconductivity in the Structure and Tidal Deformability of Strange Dwarfs
Perot, L., & Nicolas Chamel, A. (2023) · Universe · doi:10.3390/universe9090382 · Cited by 4
Is EG 50 a White or Strange Dwarf?
Hajyan, G. S., & Vartanyan, Y. L. (2017) · Astrophysics · doi:10.1007/s10511-017-9506-5 · Cited by 4
Structural properties of charged compact stars with color-flavor-locked quarks matter
Jasim, M. K., Pradhan, A., Banerjee, A., Tangphati, T., & Panotopoulos, G. (2021) · Modern Physics Letters A · doi:10.1142/s0217732321502278 · Cited by 4
Solutions of Einstein's field equation modified for the cosmological constant
Zubairi, O., & Weber, F. (2014) · Astronomische Nachrichten · doi:10.1002/asna.201412078 · Cited by 4
White dwarf stars as strange quark matter detectors
Benvenuto, O. G. (2005) · Journal of Physics G Nuclear and Particle Physics · doi:10.1088/0954-3899/31/11/l01 · Cited by 4
First order quark-gluon/hadron transition may affect cosmological nucleosynthesis
Burakovsky, L. (1996) · Physics Letters B · doi:10.1016/0370-2693(96)00517-5 · Cited by 4
Comment on “Bare Quark Matter Surfaces of Strange Stars and e+e− Emission”
Mitra, A. (1998) · Physical Review Letters · doi:10.1103/physrevlett.81.4774 · Cited by 4
Technological implications of stable strange quark matter
Desai, M. S., & Shaw, G. L. (1991) · Nuclear Physics B - Proceedings Supplements · doi:10.1016/0920-5632(91)90326-a · Cited by 4
A Way to Quark Matter: Possible Intermediate Stages
Tamagaki, R., & Tatsumi, T. (2013) · Progress of Theoretical Physics Supplement · doi:10.1143/ptp.112.277 · Cited by 4
Impact of non-zero strange quark mass (m s ≠ 0) on the properties of strange stars in f(R, T) gravity admitting observational results
Bhattacharjee, D., & Chattopadhyay, P. K. (2025) · Physica Scripta · doi:10.1088/1402-4896/adcaf4 · Cited by 3
Strange Quark Stars with Kuchowicz Metric Function in Modified Gravitational Theory
Sinha, M., & Singh, S. S. (2025) · International Journal of Theoretical Physics · doi:10.1007/s10773-025-06069-4 · Cited by 3
“The model is based on the assumption that the asymptotically free quarks are confined within a region of finite volume which is called bag ( from the observational constraints, MIT bag constant has the bounds of (41 MeV/fm 3 B 75 MeV/fm 3 ) [84, 85] ).”
Fundamental and higher-order excited modes of radial oscillation of neutron stars for various types of cold nucleonic and hyperonic matter
Barta, D. (2021) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ac12e2 · Cited by 3
“[69] C.”
Background
Neutron stars, strange pulsars and strange dwarfs
Weber, F., Weigel, M. K., & Glendenning, N. K. (1997) · Nuclear Physics A · doi:10.1016/s0375-9474(97)00276-5 · Cited by 3
Puzzle of muons in extensive air showers
Rybczyński, M., & Włodarczyk, Z. (2019) · International Journal of Modern Physics D · doi:10.1142/s0218271819500974 · Cited by 3
Engineering with quark matter
Alcock, C. R. (1989) · Nature · doi:10.1038/337405a0 · Cited by 3
Self-citation
Rotational properties of strange-pulsar models
Benvenuto, O. G., Horvath, J. E., & Vucetich, H. (1991) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.44.1321 · Cited by 3
First Order Quark-Gluon/Hadron Transition May Affect Cosmological NucleosynthesisPreprint
Burakovsky, L. (1996) · Cited by 3
The Effect of a Self-bound Equation of State on the Structure of Rotating Compact Stars
Konstantinou, A. (2026) · The Astrophysical Journal · doi:10.3847/1538-4357/ae2f62 · Cited by 2
“6 and m s = 100 MeV we have (145 MeV ) 4 B (160 MeV ) 4 , while for a c = 0 and m s = 200 MeV we have (130 MeV ) 4 B (145 MeV ) 4 (Alcock & Olinto 1988).”
Constraints on color-flavored locked quark matter in view of the HESS J1731-347 measurement
Kourmpetis, K., Laskos-Patkos, P., & Moustakidis, C. C. (2025) · HNPS Advances in Nuclear Physics · doi:10.12681/hnpsanp.8013 · Cited by 2
White dwarf stars as strange quark matter detectors �� III
Benvenuto, O. G. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.10755.x · Cited by 2
Strange quark star in dilaton gravity
Peivand, A., Naficy, K., & Bordbar, G. H. (2019) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/19/6/78 · Cited by 2
“…matter (Witten 1984; Farhi & Jaffe 1984), it has been shown that a new class of compact object may exist that have been composed from strange quark matter, known as strange quark stars(SQS) or strange stars(SS) (Haensel et al. 1986; Alcock et al. 1986b,a; Alcock & Olinto 1988; Glendenning 1990).”
Background
The Astrophysics and Cosmology of Quark—Gluon Plasma
Alcock, C. R. (1990) · Research reports in physics · doi:10.1007/978-3-642-75289-6_6 · Cited by 2
Self-citation
Neutrinos and cosmology
Schramm, D. N. (1995) · Nuclear Physics B - Proceedings Supplements · doi:10.1016/0920-5632(94)00769-r · Cited by 2
The physics potential of the RICH
Treille, D. (1996) · Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · doi:10.1016/0168-9002(95)01183-8 · Cited by 2
Electrically charged compact stars with an interacting quark equation of state
Panotopoulos, G., Tangphati, T., & Banerjee, A. (2021) · Chinese Journal of Physics · doi:10.1016/j.cjph.2021.10.027 · Cited by 1
Orbital Properties and Gravitational-wave Signatures of Strangelet Crystal Planets
Zapata, J., & Negreiros, R. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab77b7 · Cited by 1
Pulsars with the masses 2.14M⊙ and 2.27M⊙ as strange star candidates
Shahinyan, H. A., Sargsyan, T., & Babajanyan, A. (2024) · Journal of High Energy Astrophysics · doi:10.1016/j.jheap.2024.06.010 · Cited by 1
Isotropic charged compact stars in $$f(R,\mathcal T\mkern1.5mu)$$ gravity: A conformal Killing vector approach to stability, exact solutions, and strange star candidates
Salako, I. G., Ahouannou, H. S., Mavoa, F., & Monwanou, A. V. (2025) · Theoretical and Mathematical Physics · doi:10.1134/s0040577925110121 · Cited by 1
Maximal mass strange quark stars based on the modified MIT model with variable vacuum pressure
Shahinyan, H. A., Sargsyan, T., & Babajanyan, A. (2025) · Nuclear Physics B · doi:10.1016/j.nuclphysb.2025.117277 · Cited by 1
The pulsar PSR J0348-0432 and strange stars
Vartanyan, Y. L., Grigoryan, A. K., & Shaginyan, A. A. (2015) · Astronomy Letters · doi:10.1134/s1063773715070051 · Cited by 1
Converting neutron stars into strange stars: Instanton model
Gurovich, V. T., & Fel, L. G. (2014) · International Journal of Modern Physics D · doi:10.1142/s0218271814500783 · Cited by 1
EQUATION OF STATE OF NEUTRON STAR MATTER
Weber, F. (2004) · International Journal of Modern Physics D · doi:10.1142/s0218271804005420 · Cited by 1
Non-Newtonian gravity in color-flavor locked strange stars and the 2.6M⊙ component in GW190814
Pi, C., & Yang, S. (2024) · New Astronomy · doi:10.1016/j.newast.2024.102347 · Cited by 1
Role of finite value of strange quark mass ( m s ≠ 0 ) and baryon number density ( n ) on the structure of strange stars
Chattopadhyay, P. K., & Bhattacharjee, D. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101927 · Cited by 1
Can strangelets solve the muon puzzle?
Rybczyński, M., & Włodarczyk, Z. (2019) · EPJ Web of Conferences · doi:10.1051/epjconf/201920804004 · Cited by 1
Strange Quark Matter Inside Neutron Stars
Weber, F. (2016) · Springer eBooks · doi:10.1007/978-3-319-20794-0_71-1 · Cited by 1
Primordial Nucleosynthesis and Light Element Abundances
Schramm, D. N. (1995) · ESO astrophysics symposia · doi:10.1007/978-3-540-49169-9_9 · Cited by 1
Non-Baryonic Dark Matter
Sarkar, S. (1991) · Springer eBooks · doi:10.1007/978-94-011-3510-8_9 · Cited by 1
Production of drops of strange matter in fixed-target heavy-ion collisions
Crawford, H. J., Desai, M. S., & Shaw, G. L. (1991) · Nuclear Physics B - Proceedings Supplements · doi:10.1016/0920-5632(91)90325-9 · Cited by 1
Cosmology and unstable nuclei
Schramm, D. N. (1995) · Nuclear Physics A · doi:10.1016/0375-9474(95)00152-q · Cited by 1
The Role of Quarks in Astrophysics
Alcock, C. R. (1990) · NATO ASI series. Series B : Physics · doi:10.1007/978-1-4684-1336-6_7
Self-citation
The Equation of State of Dense Matter
Vautherin, D. (1995) · Springer eBooks · doi:10.1007/978-94-011-0067-0_14
Fast Pulsars, Strange Stars, and Strange Dwarfs†
Weber, F., & Glendenning, N. K. (1995) · Annals of the New York Academy of Sciences · doi:10.1111/j.1749-6632.1995.tb17550.x
AN UPPER LIMIT ON MASS DENSITY OF QUARK NUGGETS FROM THE MICROLENSING EVENT STATISTICS
Yoon, S. U., Lee, C. H., & Yang, J. (1998) · Modern Physics Letters A · doi:10.1142/s0217732398001625
Modern cosmology and physics beyond the standard model
Dolgov, A. D. (1991) · Surveys In High Energy Physics · doi:10.1080/01422419108242498
The Particle-Cosmology Connection: Neutrino Counting, Dark Matter and Large-Scale Structure
Schramm, D. N. (1991) · NATO ASI series. Series B : Physics · doi:10.1007/978-1-4899-3547-2_15
Effects of Density-Dependent Quark Mass on Phase Diagram of Color-Flavor-Locked Quark Matter
Xiao-Bing, Z., & Li, X. (2006) · Communications in Theoretical Physics · doi:10.1088/0253-6102/45/4/024
Ultrarelativistic Heavy-Ion Collisions: Present and Future
Baym, G. (1992) · Research reports in physics · doi:10.1007/978-3-642-84708-0_10
Strange Quark Matter Inside Neutron Stars
Weber, F. (2017) · Springer eBooks · doi:10.1007/978-3-319-21846-5_71
Topics in the Physics and Astrophysics of Neutron Stars
Postnikov, S. (2010) · OhioLink ETD Center (Ohio Library and Information Network)
The puzzle of muons: novel particles or novel properties
Rybczyński, M., & Włodarczyk, Z. (2019) · Journal of Physics Conference Series · doi:10.1088/1742-6596/1181/1/012051
Charged charm stars
Gonçalves, V. P., & Lazzari, L. (2020) · Nuclear Physics A · doi:10.1016/j.nuclphysa.2020.122043

Authors: Alcock, C., & Olinto, A.
ORCID: Alcock, C
Olinto, A
Venue: Annual Review of Nuclear and Particle Science
Publisher: Annual Reviews
Published: 1988-12
Volume: 38
Issue: 1
Pages: 161-184
ISSN: 0163-8998 (ISSN-L)
1545-4134
DOI: 10.1146/annurev.ns.38.120188.001113
OpenAlex: W2122622871
Cited by: 211
References: 1
Citations by year: 2026: 5 · 2025: 11 · 2024: 9 · 2023: 9 · 2022: 9 · 2021: 12 · 2020: 12 · 2019: 8 · 2018: 4 · 2017: 3 · 2016: 1 · 2015: 5 · 2014: 4 · 2013: 6 · 2012: 4
FWCI: 8.18
Type: journal article
Language: en
Open access: closed
Locations: Annual Review of Nuclear and Particle Science (publishedVersion)
Topics: Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Quantum Chromodynamics and Particle Interactions
Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › High-Energy Particle Collisions Research
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
Keywords: dense matter, nuclear equation of state, neutron stars, compact stars, astrophysical applications

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

Exotic Phases of Hadronic Matter and their Astrophysical Application

Abstract

Overview

Integrity signals

Verification

Claims the paper makes

Claims other papers make about this one

Citations

Cites

Cited by

Related

Metadata

Record

About these checks