{"id":195458,"date":"2025-10-01T19:47:15","date_gmt":"2025-10-01T19:47:15","guid":{"rendered":"https:\/\/www.newsbeep.com\/us\/195458\/"},"modified":"2025-10-01T19:47:15","modified_gmt":"2025-10-01T19:47:15","slug":"criticality-in-natures-strongest-force","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/us\/195458\/","title":{"rendered":"Criticality in Nature\u2019s Strongest Force"},"content":{"rendered":"<p>September 29, 2025&amp;bullet;  Physics 18, 164<\/p>\n<p>Experiments at the Relativistic Heavy Ion Collider give the first hints of a critical point in the hot quark\u2013gluon \u201csoup\u201d that is thought to have pervaded the infant Universe.<\/p>\n<p><a data-reveal-id=\"figure-modal-1\" href=\"https:\/\/www.newsbeep.com\/us\/wp-content\/uploads\/2025\/10\/e164_2.png\"><img decoding=\"async\" alt=\"Figure caption\" src=\"https:\/\/www.newsbeep.com\/us\/wp-content\/uploads\/2025\/10\/e164_2_medium.png\"\/><\/a><img decoding=\"async\" alt=\"expand figure\" class=\"figure-expander\" src=\"https:\/\/cdn.journals.aps.org\/development\/physics\/images\/icon-expand.svg\"\/><\/p>\n<p><a data-reveal-id=\"figure-modal-1\" href=\"https:\/\/www.newsbeep.com\/us\/wp-content\/uploads\/2025\/10\/e164_2.png\">Figure 1:<\/a> This schematic of the quantum chromodynamics phase diagram depicts how increasing the temperature can change a gas of bound quark particles (called hadrons) into a liquid-like quark\u2013gluon plasma (shown as an orange \u201csoup\u201d). Heavy-ion collision experiments in the relevant energy range have detected hints of a critical point (purple dot), which would mark the edge of a first-order phase transition (blue arc) that extends up from the high-density, low-temperature region of the diagram.<\/p>\n<p><img decoding=\"async\" alt=\"Figure caption\" src=\"https:\/\/www.newsbeep.com\/us\/wp-content\/uploads\/2025\/10\/e164_2.png\"\/><\/p>\n<p>Figure 1: This schematic of the quantum chromodynamics phase diagram depicts how increasing the temperature can change a gas of bound quark particles (called hadrons) into a liquid-like quark\u2013gluon plasma (shown as an orange \u201csoup\u201d). Heavy-ion collision experiments in the relevant energy range have detected hints of a critical point (purple dot), which would mark the edge of a first-order phase transition (blue arc) that extends up from the high-density, low-temperature region of the diagram.<a aria-label=\"Close\" class=\"close-reveal-modal\">\u00d7<\/a><\/p>\n<p id=\"d5e107\">The strongest force of nature\u2014the one holding nuclear matter together\u2014is described by the theory of quantum chromodynamics (QCD). The fundamental particles of QCD are quarks and gluons, which are normally bound within composite particles called hadrons\u2014the most well-known of which are protons and neutrons. Only at extreme temperatures around 1012 K (a million times hotter than the core of the Sun) can quarks and gluons become deconfined, leading to a new phase of matter called the quark\u2013gluon plasma. At vanishing densities, the transition between confined hadrons and the quark\u2013gluon plasma is known to be ill-defined\u2014happening across a wide range of temperatures rather than at a specific temperature. But theory predicts that at large densities and moderately high temperatures, a critical point exists, where the \u201cfuzziness\u201d disappears and a clear distinction can be made between the gas-like hadrons and the liquid-like quark\u2013gluon mix [<a href=\"#c1\" class=\"ref-target inline-ref-target\" data-ref-target=\"c1\">1<\/a>\u2013<a href=\"#c3\" class=\"ref-target inline-ref-target\" data-ref-target=\"c3\">3<\/a>]. New data from the STAR experiment at the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory in New York show what appears to be the first hints of this critical point (Fig. <a href=\"#f1\" class=\"ref-target inline-ref-target\" data-ref-target=\"f1\">1<\/a>) [<a href=\"#c4\" class=\"ref-target inline-ref-target\" data-ref-target=\"c4\">4<\/a>]. If confirmed, such a landmark detection would provide an anchoring point from which further explorations of the quark\u2013gluon plasma could venture, potentially offering insights into astrophysical phenomena like supernovae or binary neutron-star mergers.<\/p>\n<p id=\"d5e124\">The most familiar critical point is that of water. Under atmospheric pressure, water has three phases\u2014solid, liquid, and vapor\u2014which are separated by first-order phase transitions. However, if one heats and squeezes water to high-enough temperatures and pressures, it is no longer possible to easily distinguish the liquid and gas phases\u2014such melding of phases is called a crossover. The critical point marks the boundary between this crossover and the first-order phase transition at lower temperature and pressure.<\/p>\n<p id=\"d5e126\">Critical points were first identified over 200 years ago by physicist Charles Cagniard de la Tour, and their striking properties have fascinated physicists ever since. Near a critical point, particles become correlated with their distant neighbors, causing large fluctuations in observable properties. For example, a droplet of water turns white at its critical point (so-called critical opalescence) because the long-range correlated particles cause photons to scatter more often in the material. The modern theoretical understanding of critical points was established by Kenneth Wilson, who was awarded the 1982 Nobel Prize in Physics for his theory of critical phenomena in connection with phase transitions.<\/p>\n<p id=\"d5e128\">The QCD critical point is especially interesting because\u2014if observed\u2014it would be the first critical point in a fundamental force of nature. What\u2019s more, the observation of a sharp, nonambiguous transition between confined hadrons and deconfined quarks and gluons would help explain why quarks and gluons are never observed in isolation. This \u201cconfinement\u201d puzzle is one of the <a target=\"xrefwindow\" href=\"https:\/\/www.claymath.org\/millennium\/yang-mills-the-maths-gap\/\" id=\"d5e130\" rel=\"nofollow noopener\">Millennium Prize Problems<\/a> selected by the Clay Mathematics Institute.<\/p>\n<p id=\"d5e133\">Measuring the QCD critical point has been challenging. For water and other condensed-matter systems, one can simply tune the parameters to reach a specific point in the phase diagram. But that\u2019s not possible for quark\u2013gluon matter. Instead, researchers must smash together heavy ions in colliders, creating short-lived, highly dense concentrations of matter that traverse the phase diagram as they expand and cool. By varying the beam energies, one can explore different regions of the phase diagram: Higher beam energies correspond to lower baryon densities, while lower beam energies probe higher baryon densities.<\/p>\n<p id=\"d5e135\">The STAR experiment is designed to sort through the debris from collisions at RHIC. In particular, the experiment\u2019s detectors record the number of protons and the number of antiprotons that come out from each collision event. The net-proton yield, which is the difference between the proton and antiproton numbers, varies from event to event. The STAR Collaboration measures the net-proton distribution, whose \u201cshape,\u201d like that of other statistical distributions, is described by its mean, variance, and other so-called moments. The higher moments\u2014in particular the fourth moment, or kurtosis\u2014are sensitive to the growth of the correlation length at the critical point and are expected to show nonmonotonic behavior near a critical point [<a href=\"#c5\" class=\"ref-target inline-ref-target\" data-ref-target=\"c5\">5<\/a>].<\/p>\n<p id=\"d5e140\">In its hunt for the critical point, the STAR experiment performed a beam-energy scan to obtain data across a wide range of densities and then calculated the net-proton moments at each beam energy [<a href=\"#c4\" class=\"ref-target inline-ref-target\" data-ref-target=\"c4\">4<\/a>]. From the QCD equation of state (which describes the relationship between pressure and density), the moments are expected to remain constant or to monotonically decrease with increasing density. But if a critical point is present, the kurtosis could exhibit nonmonotonic behavior, including dips or peaks depending on the trajectory of the system in the phase diagram. The new STAR measurements revealed such a dip in the ratio of the fourth- to second-order moments (C4\/C2) near a collision energy of 19.6 GeV. The size of the dip relative to experimental noise corresponds to a significance between 2 and 5 sigma (where 5 sigma would signify a detection) [<a href=\"#c6\" class=\"ref-target inline-ref-target\" data-ref-target=\"c6\">6<\/a>].<\/p>\n<p id=\"d5e158\">The dip in the kurtosis is qualitatively consistent with expectations of critical phenomena. If indeed the QCD critical point has been observed, the location of the point (below 20 GeV) would imply that that a first-order phase transition (like that between water and steam) occurs at high densities, which might be relevant to supernovae, binary neutron-star mergers, and other astrophysical phenomena.<\/p>\n<p id=\"d5e160\">However, it\u2019s important to note that a dip is not a unique signature of the critical point: Dynamical effects such as baryon-number conservation [<a href=\"#c7\" class=\"ref-target inline-ref-target\" data-ref-target=\"c7\">7<\/a>] or nonequilibrium dynamics [<a href=\"#c8\" class=\"ref-target inline-ref-target\" data-ref-target=\"c8\">8<\/a>] can produce similar behavior. The observed minimum may also be sensitive to \u201cfreeze-out,\u201d which is the reduction in particle interactions as the system expands and the particles end up too far from each other. The location of the freeze-out condition in the phase diagram can affect the appearance of the dip [<a href=\"#c9\" class=\"ref-target inline-ref-target\" data-ref-target=\"c9\">9<\/a>].<\/p>\n<p id=\"d5e171\">Although the new STAR experimental data are extremely exciting, their interpretation will require further theoretical and experimental progress. The incorporation of critical fluctuations into dynamical models such as relativistic viscous hydrodynamics is an ongoing effort [<a href=\"#c10\" class=\"ref-target inline-ref-target\" data-ref-target=\"c10\">10<\/a>]. The STAR Collaboration is still analyzing data from the Beam Energy Scan program, including fixed-target measurements at lower collision energies (3.0\u20137.7 GeV), which will probe even higher baryon densities. These future experimental results, combined with novel theoretical modeling, will be crucial for determining whether the observed nonmonotonic behavior indeed signals the presence of the QCD critical point.<\/p>\n<p>ReferencesM. Stephanov et al., \u201cSignatures of the tricritical point in QCD,\u201d <a href=\"http:\/\/dx.doi.org\/10.1103\/PhysRevLett.81.4816\" rel=\"nofollow noopener\" target=\"_blank\">Phys. Rev. Lett. 81, 4816 (1998)<\/a>.V. A. Dexheimer and S. Schramm, \u201cNovel approach to modeling hybrid stars,\u201d <a href=\"http:\/\/dx.doi.org\/10.1103\/PhysRevC.81.045201\" rel=\"nofollow noopener\" target=\"_blank\">Phys. Rev. C 81, 045201 (2010)<\/a>.M. Hippert et al., \u201cBayesian location of the QCD critical point from a holographic perspective,\u201d <a href=\"http:\/\/dx.doi.org\/10.1103\/PhysRevD.110.094006\" rel=\"nofollow noopener\" target=\"_blank\">Phys. Rev. D 110, 094006 (2024)<\/a>.B. E. Aboona et al. (STAR Collaboration), \u201cPrecision measurement of net-proton-number fluctuations in Au + Au collisions at RHIC,\u201d <a href=\"http:\/\/dx.doi.org\/10.1103\/9l69-2d7p\" rel=\"nofollow noopener\" target=\"_blank\">Phys. Rev. Lett. 135, 142301 (2025)<\/a>.M. A. Stephanov, \u201cNon-Gaussian fluctuations near the QCD critical point,\u201d <a href=\"http:\/\/dx.doi.org\/10.1103\/PhysRevLett.102.032301\" rel=\"nofollow noopener\" target=\"_blank\">Phys. Rev. Lett. 102, 032301 (2009)<\/a>.V. Vovchenko et al., \u201cProton number cumulants and correlation functions in Au-Au collisions at sNN= 7.7\u2013200 GeV from hydrodynamics,\u201d <a href=\"http:\/\/dx.doi.org\/10.1103\/PhysRevC.105.014904\" rel=\"nofollow noopener\" target=\"_blank\">Phys. Rev. C 105, 014904 (2022)<\/a>.P. Braun-Munzinger et al., \u201cRelativistic nuclear collisions: Establishing a non-critical baseline for fluctuation measurements,\u201d <a href=\"http:\/\/dx.doi.org\/10.1016\/j.nuclphysa.2021.122141\" rel=\"nofollow noopener\" target=\"_blank\">Nucl. Phys. A 1008, 122141 (2021)<\/a>.T. Dore et al., \u201cCritical lensing and kurtosis near a critical point in the QCD phase diagram in and out of equilibrium,\u201d <a href=\"http:\/\/dx.doi.org\/10.1103\/PhysRevD.106.094024\" rel=\"nofollow noopener\" target=\"_blank\">Phys. Rev. D 106, 094024 (2022)<\/a>.D. Mroczek et al., \u201cQuartic cumulant of baryon number in the presence of a QCD critical point,\u201d <a href=\"http:\/\/dx.doi.org\/10.1103\/PhysRevC.103.034901\" rel=\"nofollow noopener\" target=\"_blank\">Phys. Rev. C 103, 034901 (2021)<\/a>.X. An et al., \u201cThe BEST framework for the search for the QCD critical point and the chiral magnetic effect,\u201d <a href=\"http:\/\/dx.doi.org\/10.1016\/j.nuclphysa.2021.122343\" rel=\"nofollow noopener\" target=\"_blank\">Nucl. Phys. A 1017, 122343 (2022)<\/a>.About the Author<img decoding=\"async\" alt=\"Image of Jacquelyn Noronha-Hostler\" src=\"https:\/\/www.newsbeep.com\/us\/wp-content\/uploads\/2025\/10\/e26c4f5d-e40a-4a9b-99fc-fc878decda05.png\" width=\"125\"\/><\/p>\n<p>Jacquelyn Noronha-Hostler is an associate professor in the Department of Physics at the University of Illinois Urbana-Champaign. She earned her PhD from Goethe University in Germany.\u00a0Her work explores the interface between the nearly perfect fluid obtained in heavy-ion collisions and the densest matter of the Universe found in the core of neutron stars. She received the 2018 Department of Energy Early Career Award and is an Alfred P. Sloan fellow. She was elected to the American Physical Society\u2019s Division of Nuclear Physics Executive Committee and is in the leadership of both the MUSES and SURGE Collaborations.<\/p>\n<p>Subject AreasRelated Articles<a href=\"https:\/\/physics.aps.org\/articles\/v18\/s73\" rel=\"nofollow noopener\" target=\"_blank\"><img decoding=\"async\" alt=\"Searching for a New Force\" src=\"https:\/\/www.newsbeep.com\/us\/wp-content\/uploads\/2025\/10\/large.png\"\/><\/a>Atomic and Molecular Physics<a href=\"https:\/\/physics.aps.org\/articles\/v18\/s73\" rel=\"nofollow noopener\" target=\"_blank\">Searching for a New Force<\/a>June 10, 2025<\/p>\n<p class=\"feed-item-deck\">A hypothetical fifth force could be detected by its effect on the optical transition frequencies of an element\u2019s different isotopes.<a href=\"https:\/\/physics.aps.org\/articles\/v18\/s73\" rel=\"nofollow noopener\" target=\"_blank\"> Read More \u00bb<\/a><\/p>\n<p><a href=\"https:\/\/physics.aps.org\/articles\/v18\/s61\" rel=\"nofollow noopener\" target=\"_blank\"><img decoding=\"async\" alt=\"Peering into Protons\" src=\"https:\/\/www.newsbeep.com\/us\/wp-content\/uploads\/2025\/10\/1759348035_377_large.png\"\/><\/a>Particles and Fields<a href=\"https:\/\/physics.aps.org\/articles\/v18\/s61\" rel=\"nofollow noopener\" target=\"_blank\">Peering into Protons<\/a>May 22, 2025<\/p>\n<p class=\"feed-item-deck\">The internal structure of protons bound in nuclei has been probed by studying short-lived particles created when high-energy photons strike nuclei.<a href=\"https:\/\/physics.aps.org\/articles\/v18\/s61\" rel=\"nofollow noopener\" target=\"_blank\"> Read More \u00bb<\/a><\/p>\n<p><a href=\"https:\/\/physics.aps.org\/articles\/v18\/s64\" rel=\"nofollow noopener\" target=\"_blank\"><img decoding=\"async\" alt=\"Lithium Cosmic Rays Are Not Primordial\" src=\"https:\/\/www.newsbeep.com\/us\/wp-content\/uploads\/2025\/10\/1759348035_232_large.png\"\/><\/a><a class=\"large button\" href=\"https:\/\/physics.aps.org\/browse\" rel=\"nofollow noopener\" target=\"_blank\"> More Articles<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"September 29, 2025&amp;bullet; Physics 18, 164 Experiments at the Relativistic Heavy Ion Collider give the first hints of&hellip;\n","protected":false},"author":2,"featured_media":195459,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[49],"tags":[199,79],"class_list":{"0":"post-195458","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-physics","8":"tag-physics","9":"tag-science"},"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/posts\/195458","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/comments?post=195458"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/posts\/195458\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/media\/195459"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/media?parent=195458"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/categories?post=195458"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/tags?post=195458"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}