Exotic Phases of Hadronic Matter and their Astrophysical Application

Alcock, C; Olinto, A

doi:10.1146/annurev.ns.38.120188.001113

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

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?

Although values for η dramatically different from those in the standard BBN are excluded both from measurements of the light element abundances and from the CMB, it might be possible to alter the primordial abundance of heavy elements (A > 7) in inhomogeneous scenarios.
“Although values for η dramatically different from those in the standard BBN are excluded both from measurements of the light element abundances and from the CMB, it might be possible to alter the primordial abundance of heavy elements ( A > 7) in inhomogeneous scenarios [104].”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [104]

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

Flagged first, then by citations

Sorted by citations

Neutron Star Structure and the Equation of State
Lattimer, J. M., & Prakash, M. (2001) · The Astrophysical Journal · doi:10.1086/319702 · Cited by 1,668 · see citing works
“The best-known example of self-bound stars results from WittenÏs (1984) conjecture (also see Fahri & Ja†e 1984 ; Haensel, Zdunik, & Schae†er 1986 ; Alcock & Olinto 1988 ; Prakash et al. 1990) that strange quark matter is the ultimate ground state of matter.”
Background
Color superconductivity in dense quark matter
Alford, M., Schmitt, A., Rajagopal, K., & Schäfer, T. (2008) · Reviews of Modern Physics · doi:10.1103/revmodphys.80.1455 · Cited by 1,447 · see citing works
The Physics of Neutron Stars
Lattimer, J. M., & Prakash, M. (2004) · Science · doi:10.1126/science.1090720 · Cited by 1,403 · see citing works
Strange quark matter and compact stars
Weber, F. (2004) · Progress in Particle and Nuclear Physics · doi:10.1016/j.ppnp.2004.07.001 · Cited by 870 · see citing works
Particle physics from stars
Raffelt, G. (2003) · Annual Review of Nuclear and Particle Science · doi:10.1146/annurev.nucl.49.1.163 · Cited by 266 · see citing works
Physics and astrophysics of strange quark matter
Madsen, J. (2007) · Springer eBooks · doi:10.1007/bfb0107314 · Cited by 218 · see citing works
Structure and stability of strange and charm stars at finite temperatures
Kettner, C., Weber, F., Weigel, M. K., & Glendenning, N. K. (1995) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.51.1440 · Cited by 210 · see citing works
STRANGE STARS AND RELATED ASTROPHYSICAL PHENOMENA
Cheng, K. S., Dai, Z.-G., & Tan, L. (1998) · International Journal of Modern Physics D · doi:10.1142/s0218271898000139 · Cited by 174 · see citing works
Electrically charged strange quark stars
Negreiros, R., Weber, F., Malheiro, M. M., & Usov, V. V. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.083006 · Cited by 170 · see citing works
The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) Observatory
Krizmanic, J. F., & Al., E. (2020) · Institutional Research Information System University of Turin (University of Turin) · doi:10.13016/m2mrqv-xkk6 · Cited by 160 · see citing works
Phase Transitions in the Early and Present Universe
Boyanovsky, D., de Vega, H. J., & Schwarz, D. J. (2006) · Annual Review of Nuclear and Particle Science · doi:10.1146/annurev.nucl.56.080805.140539 · Cited by 146 · see citing works
Strange matter equation of state in the quark mass-density-dependent model
Benvenuto, O. G., & Lugones, G. (1995) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.51.1989 · Cited by 138 · see citing works
Anisotropic strange stars in Tolman–Kuchowicz spacetime
Jasim, M. K., Deb, D., Ray, S., Gupta, Y. K., & Chowdhury, S. R. (2018) · The European Physical Journal C · doi:10.1140/epjc/s10052-018-6072-x · Cited by 97 · see citing works
Search for supermassive relics with a 2000- m2 array of plastic track detectors
Orito, S., Ichinose, H., Nakamura, S., Kuwahara, K., Doke, T., Ogura, K., Tawara, H., Imori, M., Yamamoto, K., Yamakawa, H., et al. (1991) · Physical Review Letters · doi:10.1103/physrevlett.66.1951 · Cited by 95 · see citing works
Effects of Anisotropy on Strongly Magnetized Neutron and Strange Quark Stars in General Relativity
Deb, D., Mukhopadhyay, B. N., & Weber, F. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac222a · Cited by 88 · see citing works
Equilibrium and stability of charged strange quark stars
Arbañil, J. D. V., & Malheiro, M. M. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.92.084009 · Cited by 81 · see citing works
Decoupling gravitational sources in f ( R , T ) gravity under class I spacetime
Maurya, S. K., Tello‐Ortiz, F., & Ray, S. (2020) · Physics of the Dark Universe · doi:10.1016/j.dark.2020.100753 · Cited by 78 · see citing works
Modified gravity with logarithmic curvature corrections and the structure of relativistic stars
Alavirad, H., & Weller, J. M. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.124034 · Cited by 78 · see citing works
Combustion of nuclear matter into strange matter
Lugones, G., Benvenuto, O. G., & Vucetich, H. (1994) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.50.6100 · Cited by 70 · see citing works
MAXIMUM MASS OF A CLASS OF COLD COMPACT STARS
Sharma, R., Karmakar, S., & Mukherjee, S. (2006) · International Journal of Modern Physics D · doi:10.1142/s0218271806008012 · Cited by 69 · see citing works
Evolution of a Neutron Star from Its Birth to Old Age
Prakash, M., Lattimer, J. M., PONS, J. A., Steiner, A. W., & Reddy, S. K. (2001) · Lecture notes in physics · doi:10.1007/3-540-44578-1_14 · Cited by 69 · see citing works
Anisotropic strange stars in the Einstein–Maxwell spacetime
Deb, D., Khlopov, M., Farook Rahaman, A., Ray, S., & Guha, B. K. (2018) · The European Physical Journal C · doi:10.1140/epjc/s10052-018-5930-x · Cited by 66 · see citing works
Relativistic simulations of the phase-transition-induced collapse of neutron stars
Abdikamalov, E. B., Dimmelmeier, H., Rezzolla, L., & Miller, J. C. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.14056.x · Cited by 63 · see citing works
“Nevertheless, including this mass for the s quark, rather than taking it to be massless, would decrease the pressure by only a few percent (Alcock & Olinto 1988).”
Background
Strange baryon matter
Lynn, B. W., Nelson, A. E., & Tetradis, N. (1990) · Nuclear Physics B · doi:10.1016/0550-3213(90)90614-j · Cited by 62 · see citing works
Evaporation of strange matter (and similar condensed phases) at high temperatures
Alcock, C. R., & Olinto, A. V. (1989) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.39.1233 · Cited by 60 · see citing works
Self-citation
Gravitational Waves from Phase‐Transition‐Induced Collapse of Neutron Stars
Lin, L.-M., Cheng, K. S., Chu, M. C., & Suen, W.-M. (2006) · The Astrophysical Journal · doi:10.1086/499202 · Cited by 58 · see citing works
“Nevertheless, the inclusion of the s-quark mass would decrease the pressure by only a few percent (Alcock & Olinto 1988).”
Background
Astrophysics probes of particle physics
Raffelt, G. G. (2000) · Physics Reports · doi:10.1016/s0370-1573(00)00039-9 · Cited by 57 · see citing works
The phase transition from nuclear matter to quark matter during proto-neutron star evolution
Benvenuto, O. G., & Lugones, G. (1999) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1999.02458.x · Cited by 50 · see citing works
Strange Quark Matter in Physics and Astrophysics
Madsen, J. (1991) · Astrophysics and space science library · doi:10.1007/978-94-011-3410-1_11 · Cited by 50 · see citing works
Buchdahl quark stars within f(Q) theory
Sokoliuk, O., Pradhan, S., Sahoo, P. K., & Baransky, A. (2022) · The European Physical Journal Plus · doi:10.1140/epjp/s13360-022-03273-7 · Cited by 48 · see citing works
“This model is based on an assumption that the asymptotically free quarks are trapped in a region with finite volume, which is called bag (from the observational constraints, MIT bag constant has the bounds 41MeV/fm3 < B < 75MeV/fm3 [22, 23]).”
Anisotropic strange quark stars with a non-linear equation-of-state
Lopes, I. P., Panotopoulos, G., & Rincón, Á. (2019) · The European Physical Journal Plus · doi:10.1140/epjp/i2019-12842-4 · Cited by 47 · see citing works
JEM-EUSO: Meteor and nuclearite observations
Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L. A., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave, M., et al. (2014) · Experimental Astronomy · doi:10.1007/s10686-014-9375-4 · Cited by 46 · see citing works
“Nuggets of Strange Quark Matter (SQM), composed of approximately the same numbers of up, down and strange quarks could be the true ground state of quantum chromodynamics [2, 41].”
Nucleation of strange matter in dense stellar cores
Horvath, J. E., Benvenuto, O. G., & Vucetich, H. (1992) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.45.3865 · Cited by 46 · see citing works
Rotation of stars containing strange quark matter
Prakash, M., Baron, E., & Prakash, M. (1990) · Physics Letters B · doi:10.1016/0370-2693(90)90835-t · Cited by 46 · see citing works
Boiling of strange-quark matter
Madsen, J., & Olesen, M. L. (1991) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.43.1069 · Cited by 46 · see citing works
Anisotropic charged strange stars in Krori-Barua spacetime under f(R,T) gravity
Biswas, S., Deb, D., Ray, S., & Guha, B. K. (2021) · Annals of Physics · doi:10.1016/j.aop.2021.168429 · Cited by 45 · see citing works
Six flavor quark matter
Yang Bai, A., & Long, A. J. (2018) · Journal of High Energy Physics · doi:10.1007/jhep06(2018)072 · Cited by 43 · see citing works
Quark Stars in Massive Brans–Dicke Gravity with Tolman–Kuchowicz Spacetime
Majid, A., & Sharif, M. (2020) · Universe · doi:10.3390/universe6080124 · Cited by 43 · see citing works
“The confined hadrons can exist in their true ground state in a hypothetical quark star [16,17].”
Background
Charged quark stars in f(R,T) gravity*
Pretel, J. M. Z., Tangphati, T., Banerjee, A., & Pradhan, A. (2022) · Chinese Physics C · doi:10.1088/1674-1137/ac84cb · Cited by 43 · see citing works
Properties of bare strange stars associated with surface electric fields
Negreiros, R., Mishustin, I. N., Schramm, S., & Weber, F. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.82.103010 · Cited by 42 · see citing works
Production and detection of drops of strange matter
Crawford, H. J., Desai, M. S., & Shaw, G. L. (1992) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.45.857 · Cited by 42 · see citing works
Differences in the Cooling Behavior of Strange Quark Matter Stars and Neutron Stars
Schaab, C., Hermann, B., Weber, F., & Weigel, M. K. (1997) · The Astrophysical Journal · doi:10.1086/310626 · Cited by 41 · see citing works
“There have been investigations on this topic prior to this one (e.g., see Alcock & Olinto 1988, Pizzochero 1991, Page 1992, Schaab et al. 1996b).”
Background
Survivability of cosmological quark nuggets in the chromoelectric flux-tube fission model of baryon evaporation
Bhattacharjee, P., Alam, J., Sinha, B., & Sibaji Raha, A. (1993) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.48.4630 · Cited by 39 · see citing works
Strange quark matter searches
Klingenberg, R. (1999) · Journal of Physics G Nuclear and Particle Physics · doi:10.1088/0954-3899/25/11/201 · Cited by 39 · see citing works
Differences in the Cooling Behavior of Strange Quark Matter Stars and Neutron Stars
Schaab, C., Hermann, B., Weber, F., & Weigel, M. K. (1997) · CERN Document Server (European Organization for Nuclear Research) · Cited by 39 · see citing works
Relativistic strange quark stars in Lovelock gravity
Panotopoulos, G., & Rincón, Á. (2019) · The European Physical Journal Plus · doi:10.1140/epjp/i2019-12853-1 · Cited by 38 · see citing works
Quark stars with 2.6 $$M_\odot $$ in a non-minimal geometry-matter coupling theory of gravity
Carvalho, G. A., Lobato, R. V., Deb, D., Moraes, P. H. R. S., & Malheiro, M. M. (2022) · The European Physical Journal C · doi:10.1140/epjc/s10052-022-11058-6 · Cited by 38 · see citing works
Charged strange stellar model describing by Tolman V metric
Jasim, M. K., Maurya, S. K., Ray, S., Shee, D., Deb, D., & Farook Rahaman, A. (2020) · Results in Physics · doi:10.1016/j.rinp.2020.103648 · Cited by 37 · see citing works
Neutron Star Interiors and the Equation of State of Superdense Matter
Weber, F., Negreiros, R., & Rosenfield, P. A. (2009) · Astrophysics and space science library · doi:10.1007/978-3-540-76965-1_0 · Cited by 37 · see citing works
Evolution of baryon number density during the cosmic quark-hadron phase transition
Sumiyoshi, K., Kajino, T., Alcock, C. R., & Mathews, G. J. (1990) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.42.3963 · Cited by 37 · see citing works
Self-citation
A tale of two mergers: searching for strangeness in compact stars
Prakash, M., & Lattimer, J. M. (2003) · Journal of Physics G Nuclear and Particle Physics · doi:10.1088/0954-3899/30/1/053 · Cited by 36 · see citing works
An Exact Family of Einstein–Maxwell Wyman–Adler Solution in General Relativity
Fatema, S., & Murad, M. H. (2013) · International Journal of Theoretical Physics · doi:10.1007/s10773-013-1538-y · Cited by 36 · see citing works
ULTRA-DENSE NEUTRON STAR MATTER, STRANGE QUARK STARS, AND THE NUCLEAR EQUATION OF STATE
Weber, F., Meixner, M., Negreiros, R., & Malheiro, M. M. (2007) · International Journal of Modern Physics E · doi:10.1142/s0218301307006599 · Cited by 36 · see citing works
Burning of strange quark matter and transport properties of QCD plasmas
Heiselberg, H., Baym, G., & Pethick, C. J. (1991) · Nuclear Physics B - Proceedings Supplements · doi:10.1016/0920-5632(91)90313-4 · Cited by 36 · see citing works
Six flavor quark matter
Yang Bai, A. (2023) · OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) · doi:10.1007/jhep06%282018%29072 · Cited by 35 · see citing works
Relativistic simulations of the phase-transition-induced collapse of neutron stars
Abdikamalov, E. B., Dimmelmeier, H., Rezzolla, L., & Miller, J. C. (2009) · MPG.PuRe (Max Planck Society) · Cited by 35 · see citing works
Bremsstrahlung photons from the bare surface of a strange quark star
Jaikumar, P., Gale, C., Page, D. P., & Prakash, M. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.70.023004 · Cited by 35 · see citing works
Brown Dwarfs, Quark Stars, and Quark-Hadron Phase Transition
Cottingham, W. N., Kalafatis, D., & Mau, R. V. (1994) · Physical Review Letters · doi:10.1103/physrevlett.73.1328 · Cited by 35 · see citing works
Is the sub-millisecond pulsar strange?
Frieman, J. A., & Olinto, A. V. (1989) · Nature · doi:10.1038/341633a0 · Cited by 34 · see citing works
Self-citation
Equation of state, neutron stars and exotic phases
Lattimer, J. M., & Prakash, M. (2005) · Nuclear Physics A · doi:10.1016/j.nuclphysa.2005.01.014 · Cited by 32 · see citing works
Strange-pulsar model
Benvenuto, O. G., Horvath, J. E., & Vucetich, H. (1990) · Physical Review Letters · doi:10.1103/physrevlett.64.713 · Cited by 32 · see citing works
Electrically charged strange quark stars with a non-linear equation-of-state
Panotopoulos, G., & Rincón, Á. (2019) · The European Physical Journal C · doi:10.1140/epjc/s10052-019-7042-7 · Cited by 30 · see citing works
Static solutions of Einstein's field equations for compact stellar objects
Zubairi, O., Romero, A., & Weber, F. (2015) · Journal of Physics Conference Series · doi:10.1088/1742-6596/615/1/012003 · Cited by 29 · see citing works
Accelerator mass spectrometry: A versatile tool for research
Kutschera, W. (1990) · Nuclear Instruments and Methods in Physics Research Section B Beam Interactions with Materials and Atoms · doi:10.1016/0168-583x(90)90364-z · Cited by 29 · see citing works
Big Bang nucleosynthesis: the Standard Model and alternatives
Schramm, D. N. (1991) · Physica Scripta · doi:10.1088/0031-8949/1991/t36/003 · Cited by 28 · see citing works
Confronting Strange Stars with Compact-Star Observations and New Physics
Yang, S., Pi, C., Zheng, X., & Weber, F. (2023) · Universe · doi:10.3390/universe9050202 · Cited by 28 · see citing works
Modeling Compact Object Mergers GW190814 and GW200210 and Other Self-bound Compact Stars with Dark Matter Induced by Gravitational Decoupling and Its Significance to the Mass Gap
Maurya, S. K., Errehymy, A., Singh, K. N., Aziz, A., Hansraj, S., & Ray, S. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad5cf1 · Cited by 27 · see citing works
Radial oscillations and tidal Love numbers of dark energy stars
Panotopoulos, G., Rincón, Á., & Lopes, I. P. (2020) · The European Physical Journal Plus · doi:10.1140/epjp/s13360-020-00867-x · Cited by 27 · see citing works
Strange stars in f(ℛ) gravity palatini formalism and gravitational wave echoes from them
Bora, J., Gogoi, D. J., & Goswami, U. D. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/09/057 · Cited by 27 · see citing works
Strangelets and the TeV–PeV cosmic-ray anisotropies
Kotera, K., Pérez-García, M. Á., & Silk, J. I. (2013) · Physics Letters B · doi:10.1016/j.physletb.2013.07.010 · Cited by 27 · see citing works
Anisotropic strange stars through embedding technique in massive Brans–Dicke gravity
Sharif, M., & Majid, A. (2020) · The European Physical Journal Plus · doi:10.1140/epjp/s13360-020-00574-7 · Cited by 23 · see citing works
Electrically charged strange stars with an interacting quark matter equation of state
Gonçalves, V. P., & Lazzari, L. (2020) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.102.034031 · Cited by 25 · see citing works
Anisotropic Quark Stars with an Interacting Quark Equation of State within the Complexity Factor Formalism
Rincón, Á., Panotopoulos, G., & Lopes, I. P. (2023) · Universe · doi:10.3390/universe9020072 · Cited by 25 · see citing works
Properties of strangelets at finite temperature in the liquid drop model
He, Y., Gao, C. S., Li, X. Q., & Chao, W. Q. (1996) · Physical Review C · doi:10.1103/physrevc.53.1903 · Cited by 25 · see citing works
Search for Strange Matter by Heavy Ion Activation
Isaac, M. C. P., Chan, Y.-D., Clark, R. M., Deleplanque, M. A., Dragowsky, M. R., Fallon, P., Goldman, I. D., Larimer, R. M., Lee, I. Y., Macchiavelli, A. O., et al. (1998) · Physical Review Letters · doi:10.1103/physrevlett.81.2416 · Cited by 25 · see citing works
Neutron star properties and the relativistic equation of state of asymmetric nuclear matter
Huber, H., Weber, F., & Weigel, M. K. (1994) · Physical Review C · doi:10.1103/physrevc.50.r1287 · Cited by 25 · see citing works
Magnetized strange quark matter in a mass-density-dependent model
Hou, J.-X., Peng, G.-X., Xia, C.-J., & Xu, J.-F. (2015) · Chinese Physics C · doi:10.1088/1674-1137/39/1/015101 · Cited by 24 · see citing works
FROM CRUST TO CORE: A BRIEF REVIEW OF QUARK MATTER IN NEUTRON STARS
Weber, F., Hamil, O., Mimura, K., & Negreiros, R. (2010) · International Journal of Modern Physics D · doi:10.1142/s0218271810017329 · Cited by 24 · see citing works
THE PROPERTIES OF STRANGE STARS IN THE QUARK MASS– DENSITY–DEPENDENT MODEL
Benvenuto, O. G., & Lugones, G. (1998) · International Journal of Modern Physics D · doi:10.1142/s0218271898000048 · Cited by 24 · see citing works
Radial oscillations and gravitational wave echoes of strange stars for various equations of state
Bora, J., & Goswami, U. D. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab050 · Cited by 23 · see citing works
Non-Newtonian Gravity in Strange Quark Stars and Constraints from the Observations of PSR J0740+6620 and GW170817
Yang, S.-H., Pi, C.-M., Zheng, X.-P., & Weber, F. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abb365 · Cited by 23 · see citing works
The first second of the Universe
Schwarz, D. J. (2003) · Annalen der Physik · doi:10.1002/andp.20035150402 · Cited by 23 · see citing works
Converting neutron stars into strange stars
Olinto, A. V. (1991) · Nuclear Physics B - Proceedings Supplements · doi:10.1016/0920-5632(91)90306-y · Cited by 23 · see citing works
Self-citation
Neutron stars: Observing the properties of high-density nuclear matter
Baym, G. (1995) · Nuclear Physics A · doi:10.1016/0375-9474(95)00238-v · Cited by 22 · see citing works
Search for exotic strange quark matter in high energy nuclear reactions
Armstrong, T. A., Barish, K. N., Bennett, S. J., Chikanian, A., Coe, S. D., Cormier, T. M., Davies, R., De Cataldo, G., Dee, P., Diebold, G. E., et al. (1997) · Nuclear Physics A · doi:10.1016/s0375-9474(97)00399-0 · Cited by 21 · see citing works
Anisotropic dark energy stars within vanishing complexity factor formalism: Hydrostatic equilibrium, radial oscillations, and observational implications
Panotopoulos, G., Rincón, Á., & Lopes, I. P. (2024) · Physics Letters B · doi:10.1016/j.physletb.2024.138901 · Cited by 21 · see citing works
Absorption features caused by oscillations of electrons on the surface of a quark star
Xu, R., Баструков, С. И., Weber, F., Yu, J., & Molodtsova, I. V. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.85.023008 · Cited by 21 · see citing works
A new limit on the flux of strange matter
Nakamura, S., Orito, S., Suzuki, T., Doke, T., Ichinose, H., Kuwahara, K., & Ogura, K. (1991) · Physics Letters B · doi:10.1016/0370-2693(91)90500-p · Cited by 21 · see citing works
Strange stars with a mirror-dark-matter core confronting with the observations of compact stars
Yang, S., Pi, C.-M., & Zheng, X. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.083016 · Cited by 20 · see citing works
“According to this hypothesis, compact stars made entirely of SQM, referred to as SSs, ought to exist in the universe [5, 6, 7, 8, 9, 10].”
Background
The Effects of Charge On The Structure of Strange Stars
Malheiro, M. M., Negreiros, R., Weber, F., & Usov, V. V. (2011) · Journal of Physics Conference Series · doi:10.1088/1742-6596/312/4/042018 · Cited by 20 · see citing works
Search for strange quark matter produced in relativistic heavy ion collisions
Armstrong, T. A., Barish, K. N., Batsouli, S., Bennett, S. J., Bertaina, M. E., Chikanian, A., Coe, S. D., Cormier, T. M., Davies, R., DeCataldo, G., et al. (2001) · Physical Review C · doi:10.1103/physrevc.63.054903 · Cited by 20 · see citing works
Constraints from compact star observations on non-Newtonian gravity in strange stars based on a density dependent quark mass model
Yang, S., Pi, C., Zheng, X., & Weber, F. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.103.043012 · Cited by 19 · see citing works
Charged compact stars with color–flavor-locked strange quark matter in f(R,T) gravity
Tangphati, T., Panotopoulos, G., Banerjee, A., & Pradhan, A. (2023) · Chinese Journal of Physics · doi:10.1016/j.cjph.2022.12.014 · Cited by 19 · see citing works
Strange quark matter
Kumar, B. S. (1995) · Nuclear Physics A · doi:10.1016/0375-9474(95)00223-n · Cited by 19 · see citing works
Charged anisotropic strange stars in Finslerian geometry
Chowdhury, S. R., Deb, D., Ray, S., Rahaman, F., & Guha, B. K. (2019) · The European Physical Journal C · doi:10.1140/epjc/s10052-019-7054-3 · Cited by 17 · see citing works
Propagation of Strange Quark Matter in the atmosphere
Wilk, G. A., & Włodarczyk, Z. (1996) · Acta Physica Hungarica A) Heavy Ion Physics · doi:10.1007/bf03155636 · Cited by 17 · see citing works
The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) observatory
Olinto, A. V., Krizmanic, J. F., Adams, J. H., Aloisio, R., Anchordoqui, L. A., Anzalone, A., Bagheri, M., Barghini, D., Battisti, M., Bergman, D. R., et al. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/06/007 · Cited by 16 · see citing works
Self-citation
Study of physical properties of charged compact star model in f(T) gravity
Bhar, P. (2023) · Chinese Journal of Physics · doi:10.1016/j.cjph.2023.08.005 · Cited by 16 · see citing works
Strange stars admixed with mirror dark matter: Confronting observations of XTE J1814-338
Yang, S., Pi, C.-M., & Weber, F. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.043037 · Cited by 16 · see citing works
Structure of Quark Stars
Weber, F., Orsaria, M., Rodrigues, H., & Yang, S.-H. (2012) · Proceedings of the International Astronomical Union · doi:10.1017/s1743921312023174 · Cited by 16 · see citing works
“…early universe, its evolution to the present day, and astrophysical compact objects such as neutron stars and white dwarfs (see Alcock & Farhi 1986, Alcock & Olinto 1988, Aarhus 1991, Weber 1999, Madsen 1999, Glendenning 2000, Weber 2005, Page & Reddy 2006, Sagert et al. 2006, and references…”
Background

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

Integrity signals

Claims the paper makes

Claims other papers make about this one

Cites

Cited by

Related

Record

About these checks