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Exotic Phases of Hadronic Matter and their Astrophysical Application
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
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“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]
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“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).”
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Evaporation of strange matter (and similar condensed phases) at high temperatures
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Self-citationGravitational Waves from Phase‐Transition‐Induced Collapse of Neutron Stars
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“Nevertheless, the inclusion of the s-quark mass would decrease the pressure by only a few percent (Alcock & Olinto 1988).”
BackgroundAstrophysics probes of particle physics
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The phase transition from nuclear matter to quark matter during proto-neutron star evolution
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Buchdahl quark stars within f(Q) theory
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“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]).”
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JEM-EUSO: Meteor and nuclearite observations
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“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].”
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“The confined hadrons can exist in their true ground state in a hypothetical quark star [16,17].”
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“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).”
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Differences in the Cooling Behavior of Strange Quark Matter Stars and Neutron Stars
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Relativistic strange quark stars in Lovelock gravity
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Charged strange stellar model describing by Tolman V metric
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An Exact Family of Einstein–Maxwell Wyman–Adler Solution in General Relativity
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Is the sub-millisecond pulsar strange?
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Electrically charged strange quark stars with a non-linear equation-of-state
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Static solutions of Einstein's field equations for compact stellar objects
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Radial oscillations and tidal Love numbers of dark energy stars
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Strange stars in f(ℛ) gravity palatini formalism and gravitational wave echoes from them
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Strangelets and the TeV–PeV cosmic-ray anisotropies
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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
Electrically charged strange stars with an interacting quark matter equation of state
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Properties of strangelets at finite temperature in the liquid drop model
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Search for Strange Matter by Heavy Ion Activation
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FROM CRUST TO CORE: A BRIEF REVIEW OF QUARK MATTER IN NEUTRON STARS
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THE PROPERTIES OF STRANGE STARS IN THE QUARK MASS– DENSITY–DEPENDENT MODEL
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Radial oscillations and gravitational wave echoes of strange stars for various equations of state
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The first second of the Universe
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Converting neutron stars into strange stars
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Self-citationNeutron stars: Observing the properties of high-density nuclear matter
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Search for exotic strange quark matter in high energy nuclear reactions
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Absorption features caused by oscillations of electrons on the surface of a quark star
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Strange stars with a mirror-dark-matter core confronting with the observations of compact stars
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“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].”
BackgroundThe 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
Search for strange quark matter produced in relativistic heavy ion collisions
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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
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Charged anisotropic strange stars in Finslerian geometry
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Propagation of Strange Quark Matter in the atmosphere
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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
Self-citationStudy 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
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 23
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“…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
Metadata
- Authors
- 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
- 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 ›
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