Provide a comprehensive comparison with all existing dark
Research gap analysis derived from 3 physics papers in our local library.
The gap
The paper does not provide a comprehensive comparison with all existing dark matter detection experiments. The simulation is limited to a specific dark photon-mediated model with fermionic dark matter-electron interactions. The paper does n
Evidence profile
Sourced from the future work and limitations section and stated challenges of the source papers, classified as general, spanning 3 journals.
Research trend
Established — well-defined area with open sub-problems.
Supporting evidence — 3 representative gaps
- The CRESST experiment towards the next generation of sub GeV direct dark matter detection (2026) · Communications Physics · doi
35. Abdelhameed, A. H. et al. Geant4-based electromagnetic 62. Amole, C. et al. Dark matter search results from the complete exposure of background model for the CRESST dark matter experiment. Eur. Phys. J. C. 79, 881 (2019). [Erratum: Eur. Phys. J. C 79, 987 (2019)]. 36. Wulandari, H. et al. Neutron flux at the Gran Sasso underground laboratory revisited. Astropart. Phys. 22, 313–322 (2004). 37. Strauss, R. et al. A detector module with highly efficient surface-alpha event rejection operated in CRESST-II Phase 2. Eur. Phys. J. C. 75, 352 (2015). 38. Zema, V. Excess workshop 2022/2023. Presented at the EXCESS Workshop (2023). Workshop presentation “The low energy excess in CRESST-III” https://indico.cern.ch/event/1213348/contributions/ 5411385/. 39. Anthony-Petersen, R. et al. A stress-induced source of phonon bursts and quasiparticle poisoning. Nat. Commun. 15, 6444 (2024). 40. Stahlberg, M. Probing Low-Mass DarkMatter with CRESST-III—Data Analysis and First Results. Ph.D. thesis, TU Wien (2021). 41. Adams, D. Q. et al. Search for Majorana neutrinos exploiting millikelvin cryogenics with CUORE. Nature 604, 53–58 (2022). 42. Einfalt, L. Light Quenching in Scintillator-Based Cryogenic Detectors for Dark Matter Searches. Ph.D. thesis, TU Wien (2024). 43. Kinast, A. et al. Improving the quality of CaWO4 target crystals for CRESST. J. Low. Temp. Phys. 209, 1128–1134 (2022). 44. Strauss, R. et al. Beta/gamma and alpha backgrounds in CRESST-II Phase 2. J. Cosmol. Astropart. Phys. 06, 030 (2015). 45. An, H., Pospelov, M., Pradler, J. & Ritz, A. Direct detection constraints on dark photon dark matter. Phys. Lett. B 747, 331–338 (2015). 46. Hochberg, Y., Lin, T. & Zurek, K. M. Absorption of light dark matter in semiconductors. Phys. Rev. D. 95, 023013 (2017). 47. Zema, V. et al. Dark matter-electron scattering search using cryogenic light detectors. Phys. Rev. D. 110, 123012 (2024). 48. Bento, A. et al. Solar neutrinos in cryogenic detectors. Eur. Phys. J. C. 84, 1118 (2024). 49. Liu, Z. Z. et al. Constraints on spin-independent nucleus scattering with sub-GeV weakly interacting massive particle dark matter from the CDEX-1B experiment at the China Jinping Underground Laboratory. Phys. Rev. Lett. 123, 161301 (2019). 50. Agnese, R. et al. Search for low-mass dark matter with CDMSlite using a profile likelihood fit. Phys. Rev. D. 99, 062001 (2019). the PICO-60 C3F8 bubble chamber. Phys. Rev. D. 100, 022001 (2019).
generalfuture workevidence 5/5Keywords: phys dark matter cresst search excess workshop light cryogenic detectors based experiment underground laboratory astropart - Dark Parton Shower Effects for Cosmic Ray Boosted Dark Matter (2026) · Chinese Physics C · doi
The paper does not provide a comprehensive comparison with all existing dark matter detection experiments. The simulation is limited to a specific dark photon-mediated model with fermionic dark matter-electron interactions. The paper does not discuss the potential systematic uncertainties in the experimental searches.
generallimitations sectionevidence 5/5Keywords: paper does provide comprehensive comparison all existing dark - Dark Matter implications from the LZ, PandaX-4T and XENONnT Data (2026) · Physics Letters B · doi
The analysis is limited by the poorly constrained charge yields of 124 Xe double electron capture (DEC), which leads to systematic uncertainty. The study requires extending the analysis to higher recoil energies (≳ 100 -300 keV NR) to distinguish a potential dark matter signal from the DEC background. The paper notes that the contributions from CEνNS in LZ and XENONnT, neutrons in LZ, and surface events in PandaX-4T and XENONnT SR1 are negligible, but may still pose challenges in the analysis.
generalstated challengesevidence 5/5Keywords: analysis limited poorly constrained charge yields double electron
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