EPISODE · Oct 13, 2025 · 18 MIN
LHAASO’s Giant Peanut: A Challenge to Extreme Particle Physics
from Multi-messenger astrophysics · host Astro-COLIBRI
Join us as we discuss the groundbreaking discovery by the LHAASO Collaboration of a vast and unique ultra-high-energy (UHE) $\gamma$-ray source. This mysterious object, nicknamed the **"Peanut"** for its distinctive asymmetric shape, spans approximately $0.45^\circ \times 4.6^\circ$ and is located far off the Galactic plane, at a high Galactic latitude ($b \approx -17.5^\circ$), a region where UHE $\gamma$-ray sources are typically sparse.**Key Takeaways:*** **Extreme Energies Detected:** The LHAASO (Large High Altitude Air Shower Observatory) detected $\gamma$-rays in this region exceeding 100 TeV (Tera-electronvolts), with the highest-energy event reaching $760^{+60}_{-40}$ TeV. These UHE $\gamma$-rays are signatures of **extreme particle acceleration** in astrophysical sources.* **The Millisecond Pulsar Mystery:** The **highly aged millisecond pulsar (MSP) J0218+4232** is the sole candidate accelerator positionally coincident with the Peanut. The observed $\gamma$-ray luminosity ($L_{\gamma} \approx 9.36 \times 10^{32} \text{ erg s}^{-1}$) can be powered by the MSP’s spin-down power ($\dot{E} \approx 2.44 \times 10^{35} \text{ erg s}^{-1}$) if the energy conversion efficiency is greater than $0.4\%$.* **Challenging Prevailing Models:** If confirmed, this MSP association would be the **first evidence of a millisecond pulsar powering PeV particles**, directly challenging conventional models which posit that MSPs cannot sustain acceleration to PeV energies.* **Anisotropic Diffusion:** The Peanut's asymmetric, strip-like morphology is clear evidence of **anisotropic particle distribution** over a large area. Analysis suggests that particle transport plays the dominant role in shaping the Peanut structure. The resulting diffusion coefficient estimates indicate that particles travel about 400 times faster parallel to the strip than perpendicular to it ($D_{\parallel} \simeq 400 D_{\perp}$), compatible with estimates for the Galactic halo.* **Next Steps:** The definitive origin of the Peanut remains uncertain, potentially revealing a **new class of extreme Galactic accelerators** (PeVatrons). Further multiwavelength observations are necessary to constrain the mechanisms involved.**Reference Article:****"A Giant Peanut-shaped Ultra-High-Energy Gamma-Ray Emitter Off the Galactic Plane"** by The LHAASO Collaboration.Acknowledements: Podcast prepared with Google/NotebookLM. Illustration credits: LHAASO Collaboration
What this episode covers
Join us as we discuss the groundbreaking discovery by the LHAASO Collaboration of a vast and unique ultra-high-energy (UHE) $\gamma$-ray source. This mysterious object, nicknamed the **"Peanut"** for its distinctive asymmetric shape, spans approximately $0.45^\circ \times 4.6^\circ$ and is located far off the Galactic plane, at a high Galactic latitude ($b \approx -17.5^\circ$), a region where UHE $\gamma$-ray sources are typically sparse.**Key Takeaways:*** **Extreme Energies Detected:** The LHAASO (Large High Altitude Air Shower Observatory) detected $\gamma$-rays in this region exceeding 100 TeV (Tera-electronvolts), with the highest-energy event reaching $760^{+60}_{-40}$ TeV. These UHE $\gamma$-rays are signatures of **extreme particle acceleration** in astrophysical sources.* **The Millisecond Pulsar Mystery:** The **highly aged millisecond pulsar (MSP) J0218+4232** is the sole candidate accelerator positionally coincident with the Peanut. The observed $\gamma$-ray luminosity ($L_{\gamma} \approx 9.36 \times 10^{32} \text{ erg s}^{-1}$) can be powered by the MSP’s spin-down power ($\dot{E} \approx 2.44 \times 10^{35} \text{ erg s}^{-1}$) if the energy conversion efficiency is greater than $0.4\%$.* **Challenging Prevailing Models:** If confirmed, this MSP association would be the **first evidence of a millisecond pulsar powering PeV particles**, directly challenging conventional models which posit that MSPs cannot sustain acceleration to PeV energies.* **Anisotropic Diffusion:** The Peanut's asymmetric, strip-like morphology is clear evidence of **anisotropic particle distribution** over a large area. Analysis suggests that particle transport plays the dominant role in shaping the Peanut structure. The resulting diffusion coefficient estimates indicate that particles travel about 400 times faster parallel to the strip than perpendicular to it ($D_{\parallel} \simeq 400 D_{\perp}$), compatible with estimates for the Galactic halo.* **Next Steps:** The definitive origin of the Peanut remains uncertain, potentially revealing a **new class of extreme Galactic accelerators** (PeVatrons). Further multiwavelength observations are necessary to constrain the mechanisms involved.**Reference Article:****"A Giant Peanut-shaped Ultra-High-Energy Gamma-Ray Emitter Off the Galactic Plane"** by The LHAASO Collaboration.Acknowledements: Podcast prepared with Google/NotebookLM. Illustration credits: LHAASO Collaboration
NOW PLAYING
LHAASO’s Giant Peanut: A Challenge to Extreme Particle Physics
No transcript for this episode yet