{"id":3970,"date":"2016-08-25T03:11:50","date_gmt":"2016-08-25T03:11:50","guid":{"rendered":"http:\/\/www.particlebites.com\/?p=3970"},"modified":"2017-02-19T02:10:40","modified_gmt":"2017-02-19T02:10:40","slug":"the-delirium-over-beryllium","status":"publish","type":"post","link":"https:\/\/www.particlebites.com\/?p=3970","title":{"rendered":"The Delirium over Beryllium"},"content":{"rendered":"<div class=\"intro\"><strong>Article: <\/strong>Particle Physics Models for the 17 MeV Anomaly in Beryllium Nuclear Decays<br \/>\n<strong>Authors:<\/strong> J.L. Feng, B. Fornal, I.\u00a0Galon, S. Gardner, J. Smolinsky, T. M. P. Tait, F.\u00a0Tanedo<br \/>\n<strong>Reference:<\/strong>\u00a0<a href=\"http:\/\/arxiv.org\/abs\/1608.03591\">arXiv:1608.03591<\/a> (Submitted to Phys. Rev. D)<br \/>\nSee also this <a href=\"http:\/\/Latin American Webinars on Physics\">Latin American Webinar on Physics<\/a>\u00a0recorded talk.<\/div>\n<div class=\"intro\"><strong>Also featuring the results from:<\/strong><br \/>\n&#8212; Guly\u00e1s et al., &#8220;A pair spectrometer for measuring multipolarities of energetic nuclear transitions&#8221; (description of detector;\u00a0<a href=\"https:\/\/arxiv.org\/abs\/1504.00489\">1504.00489<\/a>;\u00a0<a href=\"http:\/\/linkinghub.elsevier.com\/retrieve\/pii\/S0168900215013716\">NIM<\/a>)<br \/>\n&#8212; Krasznahorkay et al., &#8220;Observation of Anomalous Internal Pair Creation in 8Be: A Possible Indication of a Light, Neutral Boson&#8221; \u00a0(experimental result;\u00a0<a href=\"https:\/\/arxiv.org\/abs\/1504.01527\">1504.01527<\/a>;\u00a0<a href=\"http:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.116.042501\">PRL version<\/a>; note PRL version differs from arXiv)<br \/>\n&#8212; Feng et al., &#8220;Protophobic Fifth-Force Interpretation of the Observed Anomaly in <sup>8<\/sup>Be Nuclear Transitions&#8221; (phenomenology;\u00a0<a href=\"http:\/\/arxiv.org\/abs\/1604.07411\">1604.07411<\/a>; <a href=\"http:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.117.071803\">PRL<\/a>)<\/div>\n<p><em>Editor&#8217;s note: the author is a co-author of the paper being highlighted.\u00a0<\/em><\/p>\n<p>Recently there&#8217;s some\u00a0press (see links below)\u00a0regarding\u00a0early hints\u00a0of a new particle\u00a0observed in a nuclear physics experiment.\u00a0In this bite,\u00a0we&#8217;ll\u00a0summarize the result that\u00a0has raised the eyebrows of some physicists,\u00a0and the hackles of others.<\/p>\n<h2>A crash course on nuclear physics<\/h2>\n<p>Nuclei are bound states of protons and neutrons. They can have excited states analogous to the excited states of at lowoms, which are bound states of nuclei and electrons.\u00a0The particular nucleus of interest is beryllium-8, which has four neutrons and four protons, which you may know from\u00a0the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Triple-alpha_process\">triple alpha process<\/a>. There are three\u00a0nuclear states\u00a0to be aware of: the ground state, the 18.15 MeV excited state, and the 17.64 MeV excited state.<\/p>\n<figure id=\"attachment_4133\" aria-describedby=\"caption-attachment-4133\" style=\"width: 751px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/particlebites.aas.org\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-21-at-8.19.26-AM-1.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4133 size-full\" src=\"https:\/\/particlebites.aas.org\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-21-at-8.19.26-AM-1.png\" width=\"751\" height=\"474\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-21-at-8.19.26-AM-1.png 751w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-21-at-8.19.26-AM-1-300x189.png 300w\" sizes=\"auto, (max-width: 706px) 89vw, (max-width: 767px) 82vw, 740px\" \/><\/a><figcaption id=\"caption-attachment-4133\" class=\"wp-caption-text\">Beryllium-8 excited nuclear states. The 18.15 MeV state (red) exhibits an anomaly. Both the 18.15 MeV and 17.64 states decay to the ground through a magnetic, p-wave transition. Image adapted from Savage et al. (1987).<\/figcaption><\/figure>\n<p>Most of the time the\u00a0excited states fall apart into a lithium-7 nucleus and a proton.\u00a0But sometimes, these excited states decay\u00a0into the beryllium-8 ground state\u00a0by emitting a photon (\u03b3-ray). Even more\u00a0rarely, these states can decay to the ground state by emitting an electron&#8211;positron pair from a virtual photon: this is called\u00a0<strong>internal pair creation <\/strong>and\u00a0it is these events\u00a0that\u00a0exhibit an anomaly.<\/p>\n<h2>The beryllium-8 anomaly<\/h2>\n<p>Physicists\u00a0at the\u00a0<a href=\"http:\/\/w3.atomki.hu\/index_en.html\">Atomki nuclear physics institute<\/a> in Hungary\u00a0were\u00a0studying the nuclear decays of\u00a0excited\u00a0beryllium-8 nuclei. The team,\u00a0led by Attila J. Krasznahorkay,\u00a0produced\u00a0beryllium\u00a0excited states by bombarding a lithium-7 nucleus with protons.<\/p>\n<figure id=\"attachment_4005\" aria-describedby=\"caption-attachment-4005\" style=\"width: 325px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-20-at-2.21.47-PM.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4005\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-20-at-2.21.47-PM.png\" alt=\"Preparation of beryllium-8 excited state\" width=\"325\" height=\"214\" \/><\/a><figcaption id=\"caption-attachment-4005\" class=\"wp-caption-text\">Beryllium-8 excited states are prepare by\u00a0bombarding\u00a0lithium-7 with protons.<\/figcaption><\/figure>\n<p>The proton beam is tuned to very specific energies\u00a0so that one can &#8216;tickle&#8217; specific beryllium excited states.\u00a0When the protons have around 1.03 MeV of kinetic\u00a0energy, they excite lithium into the 18.15 MeV beryllium\u00a0state. This has two important features:<\/p>\n<ol>\n<li>Picking the proton energy allows one to only produce a specific excited state\u00a0so one doesn&#8217;t have to worry about contamination from decays of other excited states.<\/li>\n<li>Because\u00a0the 18.15 MeV beryllium\u00a0nucleus is produced at <em>resonance<\/em>, one has a very high yield of these excited states. This is very good when looking for\u00a0very rare\u00a0decay processes like internal pair creation.<\/li>\n<\/ol>\n<p>What one\u00a0<em>expects<\/em> is that\u00a0most of the electron&#8211;positron pairs have small opening angle with\u00a0a\u00a0smoothly decreasing number as with larger opening angles.<\/p>\n<figure id=\"attachment_4024\" aria-describedby=\"caption-attachment-4024\" style=\"width: 600px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4024\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-22-at-9.18.11-AM.png\" alt=\"Screen Shot 2016-08-22 at 9.18.11 AM\" width=\"600\" height=\"364\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-22-at-9.18.11-AM.png 751w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-22-at-9.18.11-AM-300x182.png 300w\" sizes=\"auto, (max-width: 600px) 100vw, 600px\" \/><figcaption id=\"caption-attachment-4024\" class=\"wp-caption-text\">Expected distribution of opening angles for ordinary internal pair creation events.\u00a0Each line corresponds to\u00a0nuclear transition that is\u00a0electric (E) or magenetic (M) with a given orbital quantum number,\u00a0<em>l<\/em>.\u00a0The beryllium\u00a0transitionsthat we&#8217;re interested in are mostly M1. Adapted from Guly\u00e1s et al. (<a href=\"https:\/\/arxiv.org\/abs\/1504.00489\">1504.00489<\/a>).<\/figcaption><\/figure>\n<p>Instead, the Atomki\u00a0team found an excess of events\u00a0with large electron&#8211;positron opening angle. In fact,\u00a0even more intriguing: the excess occurs around a particular opening angle (140 degrees) and forms a bump.<\/p>\n<figure id=\"attachment_4004\" aria-describedby=\"caption-attachment-4004\" style=\"width: 400px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-20-at-2.22.05-PM.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4004\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-20-at-2.22.05-PM.png\" alt=\"Adapted from Krasznahorkay et al. \" width=\"400\" height=\"312\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-20-at-2.22.05-PM.png 642w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-20-at-2.22.05-PM-300x234.png 300w\" sizes=\"auto, (max-width: 400px) 100vw, 400px\" \/><\/a><figcaption id=\"caption-attachment-4004\" class=\"wp-caption-text\">Number of events (<em>dN\/d\u03b8<\/em>) for different electron&#8211;positron opening angles and plotted for different excitation energies (<em>E<sub>p<\/sub><\/em>). For <em>E<sub>p<\/sub>=<\/em>1.10 MeV, there is a pronounced bump at 140 degrees which does not appear to be explainable\u00a0from the ordinary internal pair conversion. This may be suggestive of a new particle.\u00a0Adapted from Krasznahorkay et al., <a href=\"http:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.116.042501\">PRL 116, 042501<\/a>.<\/figcaption><\/figure>\n<p>Here&#8217;s why\u00a0a bump is particularly interesting:<\/p>\n<ol>\n<li>The distribution of ordinary internal pair creation events is smoothly decreasing and so this is\u00a0very unlikely to produce a bump.<\/li>\n<li>Bumps can be signs of new particles: if there is a new, light particle\u00a0that can facilitate the decay, one would expect a bump at an opening angle that depends on the new particle mass.<\/li>\n<\/ol>\n<p>Schematically, the\u00a0new particle interpretation\u00a0looks like this:<\/p>\n<figure id=\"attachment_3971\" aria-describedby=\"caption-attachment-3971\" style=\"width: 600px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/TanedoIPC.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-3971\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/TanedoIPC.png\" alt=\"Schematic of the Atomki experiment.\" width=\"600\" height=\"235\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/TanedoIPC.png 2716w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/TanedoIPC-300x117.png 300w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/TanedoIPC-768x300.png 768w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/TanedoIPC-1024x400.png 1024w\" sizes=\"auto, (max-width: 600px) 100vw, 600px\" \/><\/a><figcaption id=\"caption-attachment-3971\" class=\"wp-caption-text\">Schematic of the Atomki experiment and new particle (<em>X<\/em>) interpretation of the anomalous events. In summary: protons of a specific energy bombard stationary lithium-7 nuclei and excite them to the 18.15 MeV beryllium-8 state. These decay into the beryllium-8 ground state. Some of these decays are mediated by the new\u00a0<em>X<\/em> particle, which then decays in to electron&#8211;positron pairs of a certain opening angle that are detected in the Atomki pair spectrometer detector. Image from <a href=\"http:\/\/arxiv.org\/abs\/1608.03591\">1608.03591<\/a>.<\/figcaption><\/figure>\n<p>As an exercise for those with a background in special relativity, one can use the relation $latex (p_{e^+} + p_{e^-})^2 = m_X^2$ to prove the result:<\/p>\n<p style=\"text-align: center;\">$latex m_{X}^2 = \\left(1-\\left(\\frac{E_{e^+}-E_{e^-}}{E_{e^+}+E_{e^-}}\\right)^2\\right) (E_{e^+}+E_{e^-})^2 \\sin^2 \\frac{\\theta}{2}+\\mathcal{O}(m_e^2)$<\/p>\n<p>This relates the mass of the proposed new particle,\u00a0<em>X<\/em>, to the opening angle \u03b8 and the energies\u00a0<em>E<\/em> of the electron and positron. The opening angle bump\u00a0would then be interpreted as a new particle with <strong>mass of roughly 17 MeV<\/strong>.\u00a0To match the observed number of anomalous events, the rate at which the excited beryllium decays via\u00a0the\u00a0<em>X<\/em> boson must be 6\u00d710<sup>-6<\/sup> times the rate at which\u00a0it goes into a \u03b3-ray.<\/p>\n<p>The anomaly has a significance of\u00a06.8\u03c3. This means that it&#8217;s highly unlikely to be a statistical fluctuation, as the <a href=\"http:\/\/www.particlebites.com\/?p=3904\">750 GeV diphoton bump<\/a> appears to have been. Indeed, the conservative bet would\u00a0be some not-understood systematic effect, akin to the <a href=\"http:\/\/arxiv.org\/abs\/1305.5597\">130 GeV Fermi \u03b3-ray line<\/a>.<\/p>\n<h2>The beryllium that cried wolf?<\/h2>\n<p>Some physicists are concerned that\u00a0beryllium may be the &#8216;<a href=\"https:\/\/en.wikipedia.org\/wiki\/The_Boy_Who_Cried_Wolf\">boy that cried wolf<\/a>,&#8217; and point to\u00a0papers by the late Fokke de Boer as early as\u00a0<a href=\"http:\/\/www.sciencedirect.com\/science\/article\/pii\/S0370269396013111\">1996<\/a>\u00a0and\u00a0all the way to <a href=\"http:\/\/arxiv.org\/abs\/hep-ph\/0101298\">2001<\/a>. de Boer\u00a0made strong claims about\u00a0evidence for a new 10 MeV particle in the internal pair creation decays of the\u00a017.64 MeV beryllium-8\u00a0excited state. These claims didn&#8217;t pan out, and in fact\u00a0the <a href=\"https:\/\/arxiv.org\/abs\/1504.00489\">instrumentation paper<\/a> by the Atomki\u00a0experiment rules out\u00a0that original anomaly.<\/p>\n<p>The proposed\u00a0evidence for\u00a0&#8220;de Boeron&#8221; is shown below:<\/p>\n<figure id=\"attachment_4118\" aria-describedby=\"caption-attachment-4118\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-22-at-10.40.29-AM.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4118\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-22-at-10.40.29-AM.png\" alt=\"Beryllium\" width=\"650\" height=\"367\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-22-at-10.40.29-AM.png 726w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-22-at-10.40.29-AM-300x169.png 300w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><\/a><figcaption id=\"caption-attachment-4118\" class=\"wp-caption-text\">The de Boer claim for a 10 MeV\u00a0new particle.\u00a0Left: distribution of opening angles\u00a0for internal pair creation events in an E1 transition of carbon-12. This transition\u00a0has similar\u00a0energy splitting to the beryllium-8 17.64 MeV transition and shows good agreement with the\u00a0expectations; as shown by the flat &#8220;signal &#8211; background&#8221; on the bottom panel. Right: the same analysis for the M1 internal pair creation events from the\u00a017.64 MeV beryllium-8 states.\u00a0The &#8220;signal &#8211; background&#8221; now shows a broad excess across all opening angles. Adapted from <a href=\"http:\/\/www.sciencedirect.com\/science\/article\/pii\/S0370269396013111\">de Boer et al. PLB 368, 235 (1996)<\/a>.<\/figcaption><\/figure>\n<p>When the\u00a0Atomki group\u00a0studied the same 17.64 MeV transition, they found that a\u00a0key\u00a0background component&#8212;subdominant E1 decays from nearby excited states&#8212;dramatically improved the fit and were not included in the original de Boer analysis. This\u00a0is\u00a0the last nail in the coffin for the proposed 10 MeV &#8220;de Boeron.&#8221;<\/p>\n<p>However, the Atomki group also\u00a0highlight how their new anomaly in the 18.15 MeV state behaves differently. Unlike the\u00a0broad excess in the de Boer result, the\u00a0new excess is concentrated in a bump.\u00a0There is no known way in which additional internal pair creation backgrounds can contribute to add a bump in\u00a0the opening angle distribution; as noted above: all of these distributions are smoothly falling.<\/p>\n<p>The Atomki group goes\u00a0on to suggest that\u00a0the new particle appears to fit the bill for a <a href=\"http:\/\/www.particlebites.com\/?p=3370\">dark photon<\/a>, a reasonably\u00a0well-motivated copy of the ordinary photon that differs in\u00a0its overall strength and having a non-zero (17 MeV?) mass.<\/p>\n<h2>Theory part 1:\u00a0Not a dark photon<\/h2>\n<p>With\u00a0the Atomki result was published and peer reviewed in Physics Review Letters, the game was afoot for theorists to\u00a0understand\u00a0how it would fit into a theoretical framework like the dark photon. A group from UC Irvine, University of Kentucky, and UC Riverside found that actually, <a href=\"http:\/\/arxiv.org\/abs\/1604.07411\">dark photons have a hard time fitting the anomaly<\/a> simultaneously with other experimental constraints. In the visual language of\u00a0<a href=\"http:\/\/www.particlebites.com\/?p=3980\">this recent ParticleBite<\/a>, the situation was this:<\/p>\n<figure id=\"attachment_4120\" aria-describedby=\"caption-attachment-4120\" style=\"width: 400px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_sideways_Be.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4120\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_sideways_Be.png\" alt=\"Beryllium-8\" width=\"400\" height=\"320\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_sideways_Be.png 600w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_sideways_Be-300x240.png 300w\" sizes=\"auto, (max-width: 400px) 100vw, 400px\" \/><\/a><figcaption id=\"caption-attachment-4120\" class=\"wp-caption-text\">It turns out that the minimal model of a dark photon cannot\u00a0simultaneously explain the Atomki beryllium-8 anomaly without\u00a0running afoul of other experimental constraints. Image adapted from <a href=\"http:\/\/www.particlebites.com\/?p=3980\">this ParticleBite<\/a>.<\/figcaption><\/figure>\n<p>The main reason for this is that a dark photon with mass and interaction strength to fit the beryllium anomaly would necessarily have\u00a0been seen by <a href=\"http:\/\/na48.web.cern.ch\/NA48\/NA48-2\/NA48_2.html\">the NA48\/2 experiment<\/a>. This experiment looks for dark photons in the decay of neutral pions (\u03c0<sup>0<\/sup>). These pions typically decay into two photons, but if there&#8217;s a 17 MeV dark photon around, some fraction of those decays would go into dark-photon &#8212; ordinary-photon pairs. The non-observation of these\u00a0unique decays\u00a0rules out the dark photon\u00a0interpretation.<\/p>\n<p>The theorists\u00a0then decided to &#8220;break&#8221; the dark photon theory\u00a0in order to try to make it fit. They generalized the types of interactions\u00a0that a\u00a0new photon-like particle, <em>X<\/em>,\u00a0could have, allowing protons, for example,\u00a0to have completely different charges than electrons rather than\u00a0having exactly opposite charges. Doing this does gross violence to the theoretical consistency of\u00a0a theory&#8212;but they goal was just to\u00a0see\u00a0what a new particle interpretation\u00a0would have to look like. They found that if a new photon-like particle\u00a0talked to neutrons but not protons&#8212;that is, the new force were <em>protophobic<\/em>&#8212;then\u00a0a theory might hold together.<\/p>\n<figure id=\"attachment_4124\" aria-describedby=\"caption-attachment-4124\" style=\"width: 400px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_sideways_Be2c.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4124\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_sideways_Be2c.png\" width=\"400\" height=\"320\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_sideways_Be2c.png 600w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_sideways_Be2c-300x240.png 300w\" sizes=\"auto, (max-width: 400px) 100vw, 400px\" \/><\/a><figcaption id=\"caption-attachment-4124\" class=\"wp-caption-text\">Schematic description of how model-builders &#8220;hacked&#8221; the dark photon theory to fit both the beryllium anomaly\u00a0while being\u00a0consistent with other experiments. This hack isn&#8217;t pretty&#8212;and indeed, comes at the cost of potentially invalidating the\u00a0mathematical\u00a0consistency of the theory&#8212;but the exercise demonstrates\u00a0the target for how to a complete theory might have to behave. Image adapted from <a href=\"http:\/\/www.particlebites.com\/?p=3980\">this ParticleBite<\/a>.<\/figcaption><\/figure>\n<h2>Theory appendix:\u00a0pion-phobia is protophobia<\/h2>\n<p><em>Editor&#8217;s note: what follows is for readers with some physics background interested in a technical detail; others\u00a0may skip this section.<\/em><\/p>\n<p>How does a new\u00a0particle that is allergic to protons avoid the\u00a0neutral pion decay bounds from NA48\/2?\u00a0Pions decay into pairs of photons through the well-known triangle-diagrams of the <a href=\"http:\/\/arxiv.org\/abs\/hep-th\/0509097v1\">axial\u00a0anomaly<\/a>. The decay into photon&#8211;dark-photon pairs proceed through similar diagrams.\u00a0The goal is then to make sure that these diagrams cancel.<\/p>\n<p>A cute way to look at this is to assume that at low energies, the relevant particles running in the loop aren&#8217;t quarks, but rather nucleons (protons \u00a0and neutrons). In fact,\u00a0since only the proton can talk to the photon, one only needs to consider proton loops. Thus if the new photon-like particle,\u00a0<em>X<\/em>, doesn&#8217;t talk to protons, then\u00a0there&#8217;s no diagram for the pion to decay into <em>\u03b3X<\/em>. This would be great if the story weren&#8217;t completely wrong.<\/p>\n<figure id=\"attachment_4122\" aria-describedby=\"caption-attachment-4122\" style=\"width: 550px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-3.06.05-PM.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4122\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-3.06.05-PM.png\" alt=\"Avoiding NA48\" width=\"550\" height=\"355\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-3.06.05-PM.png 757w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-3.06.05-PM-300x193.png 300w\" sizes=\"auto, (max-width: 550px) 100vw, 550px\" \/><\/a><figcaption id=\"caption-attachment-4122\" class=\"wp-caption-text\">Avoiding NA48\/2 bounds requires that\u00a0the new particle,\u00a0<em>X,\u00a0<\/em>is pion-phobic. It turns out that\u00a0this is equivalent to\u00a0<em>X<\/em> being protophobic. The\u00a0correct way to see this is on the left, making sure that the contribution of up-quark loops cancels the contribution from down-quark loops.\u00a0A slick (but naively\u00a0completely wrong) calculation is on the right,\u00a0arguing that effectively only protons\u00a0run in the loop.<\/figcaption><\/figure>\n<p>The correct way of seeing this is to treat the pion as a quantum superposition of an up&#8211;anti-up and down&#8211;anti-down bound state, and then make sure that the <em>X<\/em> charges are such that the\u00a0contributions of the two\u00a0states cancel. The resulting charges turn out to be protophobic.<\/p>\n<p>The fact that the &#8220;proton-in-the-loop&#8221; picture gives the correct charges, however, is no coincidence. Indeed, this\u00a0was\u00a0precisely how Jack Steinberger calculated the correct pion decay rate.\u00a0The key here is whether one\u00a0treats the\u00a0quarks\/nucleons linearly or non-linearly in\u00a0chiral perturbation theory. The relation to the Wess-Zumino-Witten term&#8212;which is what really encodes the low-energy interaction&#8212;is carefully\u00a0explained in chapter 6a.2 of Georgi&#8217;s revised\u00a0<a href=\"http:\/\/www.people.fas.harvard.edu\/~hgeorgi\/weak.pdf\"><em>Weak Interactions<\/em><\/a>.<\/p>\n<h2>Theory part 2: Not\u00a0a\u00a0spin-0 particle<\/h2>\n<p>The above considerations focus on a new particle with\u00a0the same spin and parity as a photon (spin-1, parity odd).\u00a0Another result of the UCI study was a systematic exploration of other possibilities. They found\u00a0that the beryllium anomaly could not be consistent with spin-0 particles.\u00a0For a\u00a0parity-odd, spin-0 particle, one cannot simultaneously conserve angular momentum and parity in the decay of the excited beryllium-8 state. (Parity violating effects are\u00a0negligible at these energies.)<\/p>\n<figure id=\"attachment_4129\" aria-describedby=\"caption-attachment-4129\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-3.49.42-PM.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4129\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-3.49.42-PM.png\" alt=\"Parity\" width=\"500\" height=\"311\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-3.49.42-PM.png 702w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-3.49.42-PM-300x187.png 300w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-4129\" class=\"wp-caption-text\">Parity and angular momentum conservation prohibit a &#8220;dark Higgs&#8221; (parity even scalar) from mediating the anomaly.<\/figcaption><\/figure>\n<p>For a parity-odd\u00a0pseudoscalar,\u00a0the\u00a0bounds on axion-like particles\u00a0at 20 MeV suffocate any reasonable\u00a0coupling. Measured in terms of the pseudoscalar&#8211;photon&#8211;photon coupling (which has dimensions of inverse GeV), this interaction is ruled out down to the inverse Planck scale.<\/p>\n<figure id=\"attachment_4131\" aria-describedby=\"caption-attachment-4131\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-4.01.07-PM.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4131\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-4.01.07-PM.png\" alt=\"Screen Shot 2016-08-24 at 4.01.07 PM\" width=\"500\" height=\"431\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-4.01.07-PM.png 609w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-4.01.07-PM-300x259.png 300w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-4131\" class=\"wp-caption-text\">Bounds on axion-like particles exclude a 20 MeV\u00a0pseudoscalar with couplings to photons stronger than the inverse Planck scale. Adapted from <a href=\"https:\/\/arxiv.org\/abs\/1205.2671\">1205.2671<\/a> and <a href=\"https:\/\/arxiv.org\/abs\/1512.03069\">1512.03069<\/a>.<\/figcaption><\/figure>\n<p>Additional possibilities include:<\/p>\n<ul>\n<li>Dark\u00a0<em>Z<\/em> bosons,\u00a0cousins of the dark photon with spin-1 but indeterminate parity.\u00a0This\u00a0is very constrained by <a href=\"http:\/\/arxiv.org\/abs\/1205.2709\">atomic parity violation<\/a>.<\/li>\n<li>Axial vectors, spin-1\u00a0bosons with positive parity. These remain a theoretical possibility, though their unknown nuclear matrix elements make it difficult to\u00a0write\u00a0a predictive model. (See section II.D of\u00a0<a href=\"https:\/\/arxiv.org\/abs\/1608.03591\">1608.03591<\/a>.)<\/li>\n<\/ul>\n<h2>Theory part 3:\u00a0Nuclear\u00a0input<\/h2>\n<p>The plot thickens when once also includes results from nuclear theory.\u00a0<a href=\"http:\/\/arxiv.org\/abs\/1406.2343\">Recent results<\/a> from Saori Pastore, Bob Wiringa, and collaborators\u00a0point out a very important fact: the 18.15 MeV beryllium-8 state that exhibits the anomaly and the 17.64 MeV state\u00a0which does not are actually closely related.<\/p>\n<p>Recall (e.g. from the first figure at the top) that both the 18.15 MeV and 17.64 MeV states are both spin-1 and parity-even. They differ in\u00a0mass and in one other key aspect: the 17.64 MeV state carries isospin charge, while the 18.15 MeV state and ground state do not.<\/p>\n<p>Isospin is the nuclear symmetry that relates\u00a0protons to\u00a0neutrons and is tied\u00a0to electroweak symmetry in the full\u00a0Standard Model. At\u00a0nuclear energies,\u00a0isospin charge is approximately conserved. This brings us to the following puzzle:<\/p>\n<p><em>If the new particle has mass around 17 MeV, why do we see its effects in the 18.15 MeV state but not the 17.64 MeV state?<\/em><\/p>\n<p>Naively, if the new particle emitted,\u00a0<em>X,\u00a0<\/em>carries no isospin charge, then isospin conservation prohibits the decay of the 17.64 MeV state through emission of an\u00a0<em>X<\/em> boson. However, <a href=\"http:\/\/arxiv.org\/abs\/1406.2343\">the Pastore et al. result<\/a>\u00a0tells us that actually, the isospin-neutral and isospin-charged states mix quantum mechanically so that the observed\u00a018.15\u00a0and 17.64 MeV states are mixtures of iso-neutral and iso-charged states. In fact,\u00a0this mixing is actually rather large, with mixing angle of around 10 degrees!<\/p>\n<p>The result of this is\u00a0that one cannot invoke isospin conservation to explain the non-observation of\u00a0an anomaly in the 17.64 MeV state. In fact, the only way to\u00a0avoid this is to assume that the mass of the\u00a0<em>X<\/em> particle is\u00a0on the heavier side of the experimentally allowed range. The rate for\u00a0<em>X\u00a0<\/em>emission goes like the 3-momentum cubed (see section II.E of <a href=\"http:\/\/arxiv.org\/abs\/1608.03591\">1608.03591<\/a>), so a small\u00a0increase in the mass can suppresses the rate of <em>X\u00a0<\/em>emission by the lighter state by a lot.<\/p>\n<p>The UCI collaboration of theorists went further and extended the Pastore et al. analysis to include a phenomenological parameterization of explicit isospin violation.\u00a0Independent of the Atomki\u00a0anomaly, they found that\u00a0including\u00a0isospin violation improved the fit for the 18.15 MeV and 17.64 MeV electromagnetic decay widths within the Pastore et al. formalism.\u00a0The results of including all of the isospin effects end up changing the particle physics story of the Atomki anomaly significantly:<\/p>\n<figure id=\"attachment_4136\" aria-describedby=\"caption-attachment-4136\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-4.27.41-PM.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4136\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-4.27.41-PM.png\" alt=\"Parameter fits\" width=\"650\" height=\"281\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-4.27.41-PM.png 660w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-4.27.41-PM-300x130.png 300w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><\/a><figcaption id=\"caption-attachment-4136\" class=\"wp-caption-text\">The rate of\u00a0<em>X<\/em> emission (colored contours) as a function of the\u00a0<em>X<\/em> particle&#8217;s couplings to protons (horizontal axis) versus neutrons (vertical axis). The best fit for a 16.7 MeV new particle is the dashed line in the teal region. The vertical band is the region allowed by the NA48\/2 experiment. Solid lines show the dark photon and protophobic limits. Left: the case for perfect (unrealistic) isospin. Right: the case when isospin mixing and explicit violation are included. Observe that incorporating realistic isospin happens to have only a modest effect in the protophobic region.\u00a0Figure from <a href=\"http:\/\/arxiv.org\/abs\/1608.03591\">1608.03591<\/a>.<\/figcaption><\/figure>\n<p>The results of\u00a0the nuclear analysis are thus that:<\/p>\n<ol>\n<li>An interpretation of the Atomki anomaly in terms of a new particle\u00a0tends to push for a slightly heavier\u00a0<em>X<\/em> mass than the reported best fit. (<em>Remark: the Atomki paper\u00a0does not do a combined fit for the mass and coupling\u00a0nor does it report the difficult-to-quantify systematic errors \u00a0associated with the fit. This information is important for understanding the extent to which the\u00a0X mass can be pushed to be heavier.)<\/em><\/li>\n<li>The effects of isospin mixing and violation\u00a0are important to include; especially as one drifts away from the purely\u00a0protophobic limit.<\/li>\n<\/ol>\n<h2>Theory part 4: towards a complete\u00a0theory<\/h2>\n<p>The theoretical\u00a0structure presented above gives a framework to do <a href=\"http:\/\/www.particlebites.com\/?p=3980\">phenomenology<\/a>: fitting the observed anomaly\u00a0to a particle physics model and then comparing that model to other experiments.\u00a0This, however, doesn&#8217;t guarantee that\u00a0a nice&#8212;or even self-consistent&#8212;theory exists that\u00a0can stretch over the scaffolding.<\/p>\n<p>Indeed, a few challenges\u00a0appear:<\/p>\n<ul>\n<li>The isospin mixing discussed above means the\u00a0<em>X<\/em> mass must be pushed to the heavier values allowed by the Atomki observation.<\/li>\n<li>The &#8220;protophobic&#8221; limit is not obviously anomaly-free: simply asserting that known particles have arbitrary charges\u00a0does not generically produce a mathematically self-consistent theory.<\/li>\n<li>Atomic parity violation constraints require that the\u00a0<em>X<\/em> couple in the same way to <a href=\"http:\/\/www.quantumdiaries.org\/2011\/06\/19\/helicity-chirality-mass-and-the-higgs\/\">left-handed and right-handed matter.<\/a>\u00a0The left-handed coupling implies that\u00a0<em>X<\/em> must also talk to neutrinos: these open up new experimental constraints.<\/li>\n<\/ul>\n<p>The Irvine\/Kentucky\/Riverside collaboration\u00a0first note the need for a\u00a0careful experimental analysis of the actual mass ranges allowed by the Atomki observation, treating the new particle mass and coupling as simultaneously free parameters in the fit.<\/p>\n<p>Next, they observe that\u00a0protophobic couplings\u00a0can be\u00a0relatively natural. Indeed: the Standard Model\u00a0<em>Z<\/em> boson is approximately protophobic at low energies&#8212;a fact well known to\u00a0those hunting for dark matter with direct detection experiments. For exotic new physics, one can engineer protophobia\u00a0through a\u00a0phenomenon called\u00a0kinetic mixing where two force particles mix into one another.\u00a0A tuned admixture of electric charge\u00a0and baryon number,\u00a0<em>(Q-B)<\/em>, is protophobic.<\/p>\n<p>Baryon number, however, is\u00a0an anomalous global symmetry&#8212;this means that one has to work hard to make a\u00a0baryon-boson that mixes with the photon (see\u00a0<a href=\"http:\/\/arxiv.org\/abs\/1304.0576\">1304.0576<\/a>\u00a0and\u00a0<a href=\"http:\/\/arxiv.org\/abs\/1409.8165\">1409.8165<\/a>\u00a0for examples). Another alternative is if the\u00a0photon kinetically mixes with not baryon number, but the anomaly-free combination of &#8220;baryon-minus-lepton number,&#8221;\u00a0<em>Q-(B-L)<\/em>.\u00a0This then forces one to apply additional model-building modules to deal with the neutrino interactions that come along with this scenario.<\/p>\n<p>In the language of the &#8216;model building blocks&#8217; above,\u00a0result of this process\u00a0looks schematically like this:<\/p>\n<figure id=\"attachment_4155\" aria-describedby=\"caption-attachment-4155\" style=\"width: 600px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_longgame_Be.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4155\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_longgame_Be.png\" alt=\"Model building block\" width=\"600\" height=\"375\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_longgame_Be.png 650w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Pheno_longgame_Be-300x187.png 300w\" sizes=\"auto, (max-width: 600px) 100vw, 600px\" \/><\/a><figcaption id=\"caption-attachment-4155\" class=\"wp-caption-text\">A complete theory is completely mathematically self-consistent and\u00a0satisfies existing constraints.\u00a0The additional bells and whistles required for consistency\u00a0make additional predictions for experimental searches.\u00a0Pieces of the theory can sometimes\u00a0 be used to address\u00a0other anomalies.<\/figcaption><\/figure>\n<p>The theory collaboration presented <a href=\"https:\/\/arxiv.org\/abs\/1608.03591\">examples of the two cases<\/a>,\u00a0and point out how the additional &#8216;bells and whistles&#8217; required may tie to additional experimental handles to test these hypotheses.\u00a0These are simple\u00a0existence proofs\u00a0for how complete models may be constructed.<\/p>\n<h2>What&#8217;s next?<\/h2>\n<p>We have delved rather deeply into the theoretical considerations of the Atomki anomaly. The analysis revealed some unexpected features with the types of new particles that could explain the anomaly (dark photon-like, but not exactly a dark photon), the role of nuclear effects (isospin mixing and breaking), and the kinds of features a complete theory needs to have to fit everything (be careful with anomalies and neutrinos).\u00a0The\u00a0<em>single most important next step<\/em>, however, is and has always been\u00a0<em><strong>experimental verification of the result<\/strong><\/em>.<\/p>\n<p>While the Atomki experiment continues to run with\u00a0an upgraded detector, what&#8217;s really exciting is that a swath of\u00a0experiments that are either ongoing or in construction will be able to probe the exact interactions required by the new particle interpretation of the anomaly.\u00a0This means that the result can be independently\u00a0verified or excluded\u00a0within a few years.\u00a0A selection of upcoming experiments is highlighted in section IX of\u00a0<a href=\"https:\/\/arxiv.org\/abs\/1608.03591\">1608.03591<\/a>:<\/p>\n<figure id=\"attachment_4138\" aria-describedby=\"caption-attachment-4138\" style=\"width: 426px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-6.03.25-PM.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-4138 size-full\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-6.03.25-PM.png\" alt=\"Experimental searches\" width=\"426\" height=\"388\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-6.03.25-PM.png 426w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-6.03.25-PM-300x273.png 300w\" sizes=\"auto, (max-width: 426px) 100vw, 426px\" \/><\/a><figcaption id=\"caption-attachment-4138\" class=\"wp-caption-text\">Other experiments that can probe the new particle interpretation of the Atomki anomaly. The horizontal axis is the new particle mass, the vertical axis is its coupling to electrons (normalized to the electric charge). The dark blue band is the target region for the Atomki anomaly. Figure from <a href=\"https:\/\/arxiv.org\/abs\/1608.03591\">1608.03591<\/a>; assuming 100% branching ratio to electrons.<\/figcaption><\/figure>\n<p>We highlight one particularly interesting\u00a0search: recently a\u00a0<a href=\"http:\/\/arxiv.org\/abs\/1509.06765\">joint team of theorists and experimentalists at MIT proposed<\/a> a way for\u00a0the <a href=\"http:\/\/lhcb-public.web.cern.ch\/lhcb-public\/\">LHCb experiment<\/a>\u00a0to search for dark photon-like particles with masses and interaction strengths that were previously unexplored. The proposal makes use of the LHCb&#8217;s ability to pinpoint the production position of charged particle\u00a0pairs and the copious amounts of\u00a0<em>D<\/em> mesons produced at Run 3 of the LHC.\u00a0As seen in the figure above, the LHCb reach with this search thoroughly covers the Atomki anomaly region.<\/p>\n<h2>Implications<\/h2>\n<p>So where we stand is this:<\/p>\n<ul>\n<li>There is\u00a0an unexpected result in a nuclear experiment that may be interpreted as a sign for new physics.<\/li>\n<li>The\u00a0next steps in this story are independent\u00a0experimental cross-checks; the threshold for a &#8216;discovery&#8217; is if\u00a0another experiment can verify these results.<\/li>\n<li>Meanwhile, a theoretical framework for understanding the results in terms of a new particle has been built and is ready-and-waiting. Some of the results of this analysis are\u00a0important for faithful interpretation of the experimental results.<\/li>\n<\/ul>\n<p><strong><em>What if it&#8217;s nothing?<\/em><\/strong><\/p>\n<p>This is the conservative take&#8212;and indeed,\u00a0we may well find that in a few years, the possibility that Atomki was observing a new particle\u00a0will be completely\u00a0dead. Or perhaps a source of systematic error will be identified and the bump will go away. That&#8217;s part of doing science.<\/p>\n<p>Meanwhile, there\u00a0are some important take-aways in this scenario. First is the reminder that the <a href=\"https:\/\/arxiv.org\/abs\/1311.0029\">search for light, weakly coupled particles<\/a> is an important frontier in\u00a0particle physics. Second, for this particular anomaly, there are some neat take aways such as a demonstration of\u00a0how\u00a0effective field theory can be applied to nuclear physics (see e.g. chapter 3.1.2 of the <a href=\"https:\/\/books.google.com\/books?id=tsDACwAAQBAJ&amp;source=gbs_navlinks_s\">new book by Petrov\u00a0and Blechman<\/a>) and how\u00a0tweaking our models of new particles can avoid troublesome experimental bounds.\u00a0Finally, it&#8217;s a nice example of how particle physics and nuclear physics are not-too-distant cousins and how\u00a0progress can be made in particle&#8211;nuclear collaborations&#8212;one of the Irvine group authors (Susan Gardner) is a bona fide nuclear theorist who was on sabbatical from the University of Kentucky.<\/p>\n<p><strong><em>What if it&#8217;s real?<\/em><\/strong><\/p>\n<p>This is a big &#8220;what if.&#8221; On the other hand,\u00a0a\u00a06.8\u03c3 effect is not a statistical fluctuation and there is no known nuclear physics to produce a new-particle-like bump given the analysis presented by the Atomki experimentalists.<\/p>\n<p>The threshold for &#8220;real&#8221; is\u00a0independent verification. If other experiments can confirm the anomaly, then this could\u00a0be\u00a0a huge step in our quest to go beyond the Standard Model. While this type of particle is unlikely to help with the <a href=\"http:\/\/www.quantumdiaries.org\/2012\/07\/01\/the-hierarchy-problem-why-the-higgs-has-a-snowballs-chance-in-hell\/\">Hierarchy problem of the Higgs mass<\/a>, it could\u00a0be a sign for other kinds of new physics. One example\u00a0is the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Grand_Unified_Theory\">grand\u00a0unification<\/a> of the electroweak and strong forces;\u00a0some of the\u00a0ways in which these forces unify imply the existence of an additional\u00a0force particle that may be light and may even have the types of couplings suggested by the anomaly.<\/p>\n<p><em><strong>Could it\u00a0be related to other anomalies?<\/strong><\/em><\/p>\n<p>The Atomki anomaly isn&#8217;t the first\u00a0particle physics curiosity to show up at\u00a0the MeV scale.\u00a0While none of these other anomalies are\u00a0necessarily related to the\u00a0type of particle required for the Atomki result (they may not even be compatible!),\u00a0it is helpful to remember that\u00a0the MeV scale may still have surprises in store for us.<\/p>\n<ul>\n<li><strong>The KTeV anomaly<\/strong>: The rate at which neutral pions decay into electron&#8211;positron pairs appears to be off from the expectations based on chiral perturbation theory. In\u00a0<a href=\"https:\/\/arxiv.org\/abs\/0712.0007\">0712.0007<\/a>, a group of theorists found that this discrepancy could be fit to a new particle with\u00a0<em>axial<\/em> couplings. If one\u00a0fixes the mass of the\u00a0proposed particle to be 20 MeV, the resulting couplings happen to be in the same ballpark as those required for the Atomki anomaly. The important caveat here is that parameters for an axial\u00a0vector to fit the Atomki anomaly are unknown, and mixed vector&#8211;axial states are\u00a0severely constrained by atomic parity violation.<\/li>\n<\/ul>\n<figure id=\"attachment_4140\" aria-describedby=\"caption-attachment-4140\" style=\"width: 787px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-6.39.48-PM.png\"><img loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-4140\" src=\"http:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-6.39.48-PM.png\" alt=\"KTeV anomaly\" width=\"787\" height=\"125\" srcset=\"https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-6.39.48-PM.png 787w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-6.39.48-PM-300x48.png 300w, https:\/\/www.particlebites.com\/wp-content\/uploads\/2016\/08\/Screen-Shot-2016-08-24-at-6.39.48-PM-768x122.png 768w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><\/a><figcaption id=\"caption-attachment-4140\" class=\"wp-caption-text\">The KTeV anomaly interpreted\u00a0as a new particle,\u00a0<em>U<\/em>. From <a href=\"https:\/\/arxiv.org\/abs\/0712.0007\">0712.0007.<\/a><\/figcaption><\/figure>\n<ul>\n<li><strong>The\u00a0anomalous magnetic moment of the muon<\/strong> and the <strong>cosmic lithium problem<\/strong>:\u00a0much of the progress in the field of light, weakly coupled forces comes from Maxim Pospelov. The anomalous\u00a0magnetic moment of the muon, <em>(g-2)<sub>\u03bc<\/sub><\/em>,\u00a0has a long-standing discrepancy from the Standard Model (see e.g. <a href=\"http:\/\/www.quantumdiaries.org\/2011\/12\/01\/dispatch-from-the-intensity-frontier-muon-g-2\/\">this blog post<\/a>). While this may come from an error in the very, very intricate calculation and the subtle ways in which experimental data feed into it, <a href=\"https:\/\/arxiv.org\/abs\/0811.1030\">Pospelov<\/a> (and also <a href=\"https:\/\/arxiv.org\/abs\/hep-ph\/0607318\">Fayet<\/a>) noted that the shift may come from a light (in the 10s of MeV range!), weakly coupled new particle like a dark photon. Similarly, <a href=\"https:\/\/arxiv.org\/abs\/1510.08858\">Pospelov and collaborators showed<\/a> that a new light particle in the 1-20 MeV range may help explain another longstanding mystery: the surprising lack of lithium in the universe (<a href=\"http:\/\/physics.aps.org\/synopsis-for\/10.1103\/PhysRevLett.116.211303\">APS <em>Physics<\/em> synopsis<\/a>).<\/li>\n<\/ul>\n<ul>\n<li><strong>The Proton Radius Problem:\u00a0<\/strong>the charge radius of the proton\u00a0appears to be smaller than expected when measured using the\u00a0Lamb shift of muonic hydrogen versus electron scattering experiments. See <a href=\"http:\/\/www.particlebites.com\/?p=1021\">this ParticleBite summary<\/a>, and <a href=\"https:\/\/arxiv.org\/abs\/1502.05314\">this recent review<\/a>. \u00a0Some attempts to explain this discrepancy have <a href=\"http:\/\/arxiv.org\/abs\/1011.4922\">involved MeV-scale new particles<\/a>, though the <a href=\"https:\/\/arxiv.org\/abs\/1401.6154\">endeavor is\u00a0difficult<\/a>.\u00a0There&#8217;s been some\u00a0renewed popular interest after a new result using\u00a0deuterium <a href=\"http:\/\/science.sciencemag.org\/content\/353\/6300\/669\">confirmed the discrepancy.<\/a>\u00a0However, there was\u00a0a report\u00a0that a result at the <a href=\"http:\/\/www.ectstar.eu\/node\/1659\">proton radius problem conference in Trento<\/a>\u00a0suggests that\u00a0the <a href=\"http:\/\/www2.mpq.mpg.de\/~haensch\/hydrogen\/index.php\/H1s2sResearch\/RydbergProject\">2S-4P determination<\/a> of the Rydberg constant may\u00a0solve the puzzle (though discrepant with other Rydberg measurements). <em>[Those slides do not appear to be\u00a0public.]<\/em><\/li>\n<\/ul>\n<p><em><strong>Could it be related to dark matter?<\/strong><\/em><\/p>\n<p>A lot of recent progress in dark matter has revolved around the possibility that\u00a0in addition to dark matter, there may be additional\u00a0light particles that mediate interactions between dark matter and the Standard Model. If these particles are light enough, they can change the way that we expect to find dark matter in\u00a0sometimes surprising ways.\u00a0One interesting avenue is called\u00a0<a href=\"https:\/\/astrobites.org\/2015\/08\/26\/from-large-to-small-astrophysical-signs-of-dark-matter-particle-interactions\/\">self-interacting dark\u00a0matter<\/a>\u00a0and is based on the observation that\u00a0these light force carriers can deform the dark matter distribution in galaxies in ways that seem to fit astronomical\u00a0observations.\u00a0A 20 MeV dark photon-like particle\u00a0even fits the profile of what&#8217;s required by\u00a0the self-interacting dark matter paradigm, though\u00a0it is very difficult to make\u00a0such a particle consistent with both the Atomki\u00a0anomaly and the constraints from direct detection.<\/p>\n<p><em><strong>Should I be excited?<\/strong><\/em><\/p>\n<p>Given all of the caveats listed\u00a0above, some feel that it is\u00a0too early to be in &#8220;drop everything, this is new physics&#8221; mode. Others may take this as a hint that&#8217;s worth exploring further&#8212;as has been done for many anomalies in the recent past.\u00a0For researchers, it\u00a0is prudent\u00a0to be cautious, and it is paramount\u00a0to be careful; but so long as one\u00a0does both, then\u00a0being excited about a\u00a0new\u00a0possibility is part what makes our job fun.<\/p>\n<p>For the general public,\u00a0the tentative hopes of new physics that pop up&#8212;whether it&#8217;s the Atomki anomaly, or the <a href=\"http:\/\/www.particlebites.com\/?p=3770\">750 GeV diphoton bump<\/a>,\u00a0<a href=\"https:\/\/astrobites.org\/2014\/03\/12\/gamma-rays-from-the-galactic-center-a-dark-matter\/\">a GeV bump from the galactic center<\/a>, \u03b3-ray lines at\u00a0<a href=\"http:\/\/resonaances.blogspot.com\/2014\/02\/signal-of-neutrino-dark-matter.html\">3.5 keV<\/a> and <a href=\"http:\/\/resonaances.blogspot.com\/2012\/09\/fermi-line-contd.html\">130 GeV<\/a>, or <a href=\"https:\/\/www.quantamagazine.org\/20150320-penguin-anomaly-hints-at-missing-particles\/\">penguins at LHCb<\/a>&#8212;these\u00a0are the signs that\u00a0we&#8217;re\u00a0making use of all of the data available to search for new physics. Sometimes these hopes fizzle away, often they leave behind useful lessons about physics and directions forward. Maybe one of these\u00a0days an anomaly will stick\u00a0and show us the way forward.<\/p>\n<h2>Further Reading<\/h2>\n<p>Here are some of the\u00a0popular-level press on the Atomki result. See the references at the top of this\u00a0ParticleBite for references to\u00a0the primary\u00a0literature.<\/p>\n<p><a href=\"https:\/\/ucrtoday.ucr.edu\/39192\">UC Riverside Press Release<br \/>\n<\/a><a href=\"https:\/\/news.uci.edu\/research\/uci-physicists-confirm-possible-discovery-of-fifth-force-of-nature\/\">UC Irvine Press Release<br \/>\n<\/a><a href=\"http:\/\/www.nature.com\/news\/has-a-hungarian-physics-lab-found-a-fifth-force-of-nature-1.19957\">Nature News<br \/>\n<\/a><a href=\"https:\/\/www.quantamagazine.org\/20160607-new-boson-claim-faces-scrutiny\/\">Quanta Magazine<br \/>\n<\/a><a href=\"https:\/\/www.quantamagazine.org\/20160614-have-physicists-discovered-a-new-boson\/\">Quanta Magazine: Abstractions<br \/>\n<\/a><a href=\"http:\/\/www.symmetrymagazine.org\/article\/the-atomki-anomaly\">Symmetry Magazine<br \/>\n<\/a><a href=\"http:\/\/www.latimes.com\/science\/sciencenow\/la-sci-sn-fifth-force-of-nature-20160816-snap-story.html\">Los Angeles Times<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Recently there&#8217;s some press regarding early hints of a new particle observed in a nuclear physics experiment. In this bite, we&#8217;ll summarize the result that has raised the eyebrows of some physicists, and the hackles of others.<\/p>\n","protected":false},"author":3,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[47,57],"tags":[],"class_list":["post-3970","post","type-post","status-publish","format-standard","hentry","category-beyond-standard-model","category-experimental-techniques"],"_links":{"self":[{"href":"https:\/\/www.particlebites.com\/index.php?rest_route=\/wp\/v2\/posts\/3970","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.particlebites.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.particlebites.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.particlebites.com\/index.php?rest_route=\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/www.particlebites.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=3970"}],"version-history":[{"count":134,"href":"https:\/\/www.particlebites.com\/index.php?rest_route=\/wp\/v2\/posts\/3970\/revisions"}],"predecessor-version":[{"id":4697,"href":"https:\/\/www.particlebites.com\/index.php?rest_route=\/wp\/v2\/posts\/3970\/revisions\/4697"}],"wp:attachment":[{"href":"https:\/\/www.particlebites.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=3970"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.particlebites.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=3970"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.particlebites.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=3970"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}