Amit Adhikary, Aoife Bharucha, Lorenzo Feligioni, Michele Frigerio
{"title":"Prospects for sub-EW-scale ALP searches via γ+bb¯ signatures at the LHC using jet substructure techniques","authors":"Amit Adhikary, Aoife Bharucha, Lorenzo Feligioni, Michele Frigerio","doi":"10.1103/bf6h-573f","DOIUrl":"https://doi.org/10.1103/bf6h-573f","url":null,"abstract":"The current Large Hadron Collider (LHC) data show no clear indication of new physics and only incremental improvements are anticipated at the energy frontier in the near future. However, while the focus of the LHC has been on constraining TeV scale physics, new particles could still be hiding below the electroweak scale. In order to obtain sensitivity to a new light boson with couplings to SM fermions, a potentially promising decay channel, for resonances with mass ≳</a:mo>O</a:mi>(</a:mo>10</a:mn>)</a:mo></a:mtext></a:mtext>GeV</a:mi></a:mrow></a:math>, would be the decay to <f:math xmlns:f=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><f:mi>b</f:mi><f:mover accent=\"true\"><f:mi>b</f:mi><f:mo stretchy=\"false\">¯</f:mo></f:mover></f:math> pairs. The measurement of such signatures is challenging due to the trigger requirements at the LHC. In this work, we explore the LHC sensitivity to a light pseudoscalar, or axionlike particle (ALP), in the <j:math xmlns:j=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><j:mi>b</j:mi><j:mover accent=\"true\"><j:mi>b</j:mi><j:mo stretchy=\"false\">¯</j:mo></j:mover></j:math> final state with an associated photon, using jet substructure techniques, in the mass range between 10 and 100 GeV. We obtain projected exclusions on the ALP-fermion coupling in a region of phase space which has not so far been probed by direct searches. We further discuss the impact that lower trigger thresholds may have on the LHC reach.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"118 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145183009","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Comparison of chiral limit studies in a curvature mass versus on-shell renormalized quark-meson model using ChPT","authors":"Vivek Kumar Tiwari","doi":"10.1103/9zzh-d65x","DOIUrl":"https://doi.org/10.1103/9zzh-d65x","url":null,"abstract":"Consistent chiral limit has been investigated in the curvature mass parametrized quark-meson (QM) model with the quark one-loop vacuum term (QMVT) employing the infrared regularized chiral perturbation theory predicted scaling of the pion, kaon decay constants f</a:mi></a:mrow>π</a:mi></a:mrow></a:msub></a:mrow></a:math>, <c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:mrow><c:msub><c:mrow><c:mi>f</c:mi></c:mrow><c:mrow><c:mi>K</c:mi></c:mrow></c:msub></c:mrow></c:math> and <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mrow><e:msubsup><e:mrow><e:mi>M</e:mi></e:mrow><e:mrow><e:mi>η</e:mi></e:mrow><e:mrow><e:mn>2</e:mn></e:mrow></e:msubsup><e:mo>=</e:mo><e:msubsup><e:mrow><e:mi>m</e:mi></e:mrow><e:mrow><e:mi>η</e:mi></e:mrow><e:mrow><e:mn>2</e:mn></e:mrow></e:msubsup><e:mo>+</e:mo><e:msubsup><e:mrow><e:mi>m</e:mi></e:mrow><e:mrow><e:msup><e:mrow><e:mi>η</e:mi></e:mrow><e:mrow><e:mo>′</e:mo></e:mrow></e:msup></e:mrow><e:mrow><e:mn>2</e:mn></e:mrow></e:msubsup></e:mrow></e:math> when the <g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mi>π</g:mi></g:math> and <i:math xmlns:i=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><i:mi>K</i:mi></i:math> meson masses are reduced as one moves away from the physical point in the Columbia plot. Comparing the QMVT model Columbia plots with the corresponding Columbia plots computed in the very recent work of Tiwari [], using the on-shell renormalized QM (RQM) model and the earlier work of Resch [] using functional renormalization group techniques in the extended mean field approximation of the QM (e-MFA:QM-FRG) model, it has been estimated how the first, second, and crossover chiral transition regions in the <k:math xmlns:k=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><k:msub><k:mi>m</k:mi><k:mi>π</k:mi></k:msub><k:mo>−</k:mo><k:msub><k:mi>m</k:mi><k:mi>K</k:mi></k:msub></k:math>(<m:math xmlns:m=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><m:msub><m:mi>m</m:mi><m:mrow><m:mi>u</m:mi><m:mi>d</m:mi></m:mrow></m:msub><m:mo>−</m:mo><m:msub><m:mi>m</m:mi><m:mi>s</m:mi></m:msub></m:math>) and the <o:math xmlns:o=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><o:mi>μ</o:mi><o:mo>−</o:mo><o:msub><o:mi>m</o:mi><o:mi>K</o:mi></o:msub></o:math>(<q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><q:mi>μ</q:mi><q:mo>−</q:mo><q:msub><q:mi>m</q:mi><q:mi>s</q:mi></q:msub></q:math>) planes get modified by different methods of implementing the quark one-loop vacuum fluctuations in the QM model. Since both the e-MFA:QM-FRG and the QMVT model use curvature meson masses to fix the parameters and the dimensional regularization of vacuum divergences are incorporated equivalently, the differences in their results can be attributed to different methods of approaching the chiral limit. The first order regions in the QMVT model while being much smaller than those in the RQM model have similar features but moderately","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"34 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145188947","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Piezoelectric bulk acoustic resonators for dark photon detection","authors":"Tanner Trickle","doi":"10.1103/yq4n-xq9y","DOIUrl":"https://doi.org/10.1103/yq4n-xq9y","url":null,"abstract":"The kinetically mixed dark photon is a simple, testable dark matter candidate with strong theoretical motivation. Detecting the feeble electric field dark photon dark matter produces requires extremely sensitive detectors. Bulk acoustic resonators (BARs), with their exceptionally high-quality phonon modes, are highly sensitive detectors, and have previously leveraged this sensitivity to search for gravitational waves in the MHz to GHz frequency range. The BAR phonons are typically read out by detecting the electric field generated by the BAR materials’ piezoelectricity. Here we show that this piezoelectricity also rewards such detectors sensitivity to dark photon dark matter, as the dark electric field can resonantly excite BAR phonons. A single 10 g piezoelectric BAR in a large, cold, environment can be orders of magnitude more sensitive to the kinetic mixing parameter than any current experiment, with only a month-long exposure and thermally limited backgrounds.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"53 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145188946","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Damon Cleaver, Christopher McCabe, Ciaran A. J. O’Hare
{"title":"Listening for ultraheavy dark matter with underwater acoustic detectors","authors":"Damon Cleaver, Christopher McCabe, Ciaran A. J. O’Hare","doi":"10.1103/jpzr-msx1","DOIUrl":"https://doi.org/10.1103/jpzr-msx1","url":null,"abstract":"Ultraheavy dark matter candidates evade traditional direct detection experiments due to their low particle flux. We explore the potential of large underwater acoustic arrays, originally developed for ultrahigh energy neutrino detection, to detect ultraheavy dark matter interactions. These particles deposit energy via nuclear scattering while traversing seawater, generating thermoacoustic waves detectable by hydrophones. We present the first robust first-principles calculation of dark matter-induced acoustic waves, establishing a theoretical framework for signal modeling and sensitivity estimates. Our framework incorporates frequency-dependent attenuation effects, including viscous and chemical relaxation, not considered in previous calculations. A sensitivity analysis for a hypothetical 100</a:mn></a:mtext></a:mtext>km</a:mi>3</a:mn></a:msup></a:math> hydrophone array in the Mediterranean Sea demonstrates that such an array could extend sensitivity to the previously unexplored mass range of <c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:mrow><c:mn>0.1</c:mn><c:mo>−</c:mo><c:mn>10</c:mn><c:mtext> </c:mtext><c:mtext> </c:mtext><c:mi mathvariant=\"normal\">μ</c:mi><c:mi mathvariant=\"normal\">g</c:mi></c:mrow></c:math> (<g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mo>∼</g:mo><g:msup><g:mn>10</g:mn><g:mn>20</g:mn></g:msup><g:mi>–</g:mi><g:msup><g:mn>10</g:mn><g:mn>23</g:mn></g:msup><g:mtext> </g:mtext><g:mtext> </g:mtext><g:mi>GeV</g:mi></g:math>), with sensitivity to both spin-independent and spin-dependent interactions. Our results establish acoustic detection as a complementary dark matter search method, enabling searches in existing hydrophone data and informing future detector designs.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"97 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145183008","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Gravitational form factors of the nucleon in the Skyrme model based on scale-invariant chiral perturbation theory","authors":"Mitsuru Tanaka, Daisuke Fujii, Mamiya Kawaguchi","doi":"10.1103/gzj5-7bln","DOIUrl":"https://doi.org/10.1103/gzj5-7bln","url":null,"abstract":"We investigate the role of the QCD scale anomaly in the gravitational form factors of the nucleon—particularly the D</a:mi>(</a:mo>t</a:mi>)</a:mo></a:math> form factor—as well as the associated stress distribution and internal forces, using a Skyrme model based on the scale-invariant chiral perturbation theory. A distinctive feature of this model is the inclusion of both the pion and the scalar meson, which respectively capture the effects of the current quark mass and gluonic quantum contributions to the scale anomaly. By varying the mass of the scalar meson, we evaluate the sensitivity of the gluonic scale anomaly to the nucleon properties. We find that the gluonic scale anomaly plays a crucial role in satisfying the stability conditions of the nucleon and provides an internal confining force. Moreover, we also evaluate the momentum-transfer dependence of <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mi>D</e:mi><e:mo stretchy=\"false\">(</e:mo><e:mi>t</e:mi><e:mo stretchy=\"false\">)</e:mo></e:math>, which closely reproduces the lattice QCD results. With an appropriate choice of the anomalous dimension associated with the quark mass, its forward-limit value (i.e., the <i:math xmlns:i=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><i:mi>D</i:mi></i:math>-term) also matches the lattice data well.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"67 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145183114","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Taushif Ahmed, Syed Mehedi Hasan, Andreas Rapakoulias
{"title":"Phase-space integrals through Mellin-Barnes representation","authors":"Taushif Ahmed, Syed Mehedi Hasan, Andreas Rapakoulias","doi":"10.1103/xj2h-89q7","DOIUrl":"https://doi.org/10.1103/xj2h-89q7","url":null,"abstract":"This letter introduces a novel analytical approach to calculating phase-space integrals, crucial for precision in particle physics. We develop a method to compute angular components using multifold Mellin-Barnes integrals, yielding results in terms of Goncharov polylogarithms for integrals involving three denominators. Our results include expressions for massless momenta to O</a:mi>(</a:mo>ε</a:mi>2</a:mn></a:msup>)</a:mo></a:math> and for massive momentum to <f:math xmlns:f=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><f:mi mathvariant=\"script\">O</f:mi><f:mo stretchy=\"false\">(</f:mo><f:mi>ε</f:mi><f:mo stretchy=\"false\">)</f:mo></f:math>. We derive recursion relations that reduce integrals with higher powers of denominators to simpler ones. We detail how to combine the angular part with the radial one which requires a careful handling of singularities.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"93 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145183197","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Observational evidence for early dark energy as a unified explanation for cosmic birefringence and the Hubble tension","authors":"Joby Kochappan, Lu Yin, Bum-Hoon Lee, Tuhin Ghosh","doi":"10.1103/x1qj-t4jz","DOIUrl":"https://doi.org/10.1103/x1qj-t4jz","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"100 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145189496","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Post-Newtonian dynamics of compact binaries with mass transfer","authors":"Zi-Han Zhang, Tan Liu, Zong-Kuan Guo","doi":"10.1103/qhf1-v5jr","DOIUrl":"https://doi.org/10.1103/qhf1-v5jr","url":null,"abstract":"","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"69 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145189497","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}