Particle Conversions Beyond the WKB Approximation and Solar-Induced Gravitational Waves from Dark Photon Dark Matter

Kavli Affiliate: Jia Liu | First 5 Authors: Tengyu Ai, Yuxuan He, Jia Liu, Xiaolin Ma, Xiao-Ping Wang | Summary: We investigate the conversion of kinetic mixing dark photon dark matter into gravitational waves within the magnetic field of the Sun. Our study reveals that the WKB approximation is invalid in this scenario. We derive […]


Continue.. Particle Conversions Beyond the WKB Approximation and Solar-Induced Gravitational Waves from Dark Photon Dark Matter

Rich and diverse molecular gas environments of closely-separated dual quasars viewed by ALMA

Kavli Affiliate: John D. Silverman | First 5 Authors: Shenli Tang, John D. Silverman, Zhaoxuan Liu, Manda Banerji, Tomoko Suzuki | Summary: We present a study of the molecular gas in five closely-spaced ($R_{perp}<20$ kpc) dual quasars ($L_{rm bol}gtrsim10^{44}~mathrm{erg~s}^{-1}$) at redshifts $0.4<z<0.8$ with the Atacama Large Millimeter/submillimeter Array. The dual quasar phase represents a distinctive […]


Continue.. Rich and diverse molecular gas environments of closely-separated dual quasars viewed by ALMA

Measurement of $CP$ asymmetries in $B^0 to K^0_S π^0 γ$ decays at Belle II

Kavli Affiliate: T. Higuchi | First 5 Authors: Belle II Collaboration, I. Adachi, L. Aggarwal, H. Ahmed, H. Aihara | Summary: We report measurements of time-dependent $CP$ asymmetries in $B^0 to K^0_S pi^0 gamma$ decays based on a data sample of $(388pm6)times10^6$ $Bbar{B}$ events collected at the $Upsilon(4S)$ resonance with the Belle II detector. The […]


Continue.. Measurement of $CP$ asymmetries in $B^0 to K^0_S π^0 γ$ decays at Belle II

Measurement of branching fractions, CP asymmetry, and isospin asymmetry for $boldsymbol{Brightarrowργ}$ decays using Belle and Belle II data

Kavli Affiliate: T. Higuchi | First 5 Authors: Belle II Collaboration, I. Adachi, K. Adamczyk, L. Aggarwal, H. Aihara | Summary: We present measurements of $B^{+}rightarrowrho^{+}gamma$ and $B^{0}rightarrowrho^{0}gamma$ decays using a combined data sample of $772 times 10^6$ $Boverline{B}$ pairs collected by the Belle experiment and $387times 10^6$ $Boverline{B}$ pairs collected by the Belle II […]


Continue.. Measurement of branching fractions, CP asymmetry, and isospin asymmetry for $boldsymbol{Brightarrowργ}$ decays using Belle and Belle II data

Measurement of branching fractions, CP asymmetry, and isospin asymmetry for $boldsymbol{Brightarrowργ}$ decays using Belle and Belle II data

Kavli Affiliate: T. Higuchi | First 5 Authors: Belle II Collaboration, I. Adachi, K. Adamczyk, L. Aggarwal, H. Aihara | Summary: We present measurements of $B^{+}rightarrowrho^{+}gamma$ and $B^{0}rightarrowrho^{0}gamma$ decays using a combined data sample of $772 times 10^6$ $Boverline{B}$ pairs collected by the Belle experiment and $387times 10^6$ $Boverline{B}$ pairs collected by the Belle II […]


Continue.. Measurement of branching fractions, CP asymmetry, and isospin asymmetry for $boldsymbol{Brightarrowργ}$ decays using Belle and Belle II data

Masses of Sunyaev-Zel’dovich Galaxy Clusters Detected by The Atacama Cosmology Telescope: Stacked Lensing Measurements with Subaru HSC Year 3 data

Kavli Affiliate: David Spergel | First 5 Authors: Masato Shirasaki, Cristóbal Sifón, Hironao Miyatake, Erwin Lau, Zhuowen Zhang | Summary: We present a stacked lensing analysis of 96 galaxy clusters selected by the thermal Sunyaev-Zel’dovich (SZ) effect in maps of the cosmic microwave background (CMB). We select foreground galaxy clusters with a $5sigma$-level SZ threshold […]


Continue.. Masses of Sunyaev-Zel’dovich Galaxy Clusters Detected by The Atacama Cosmology Telescope: Stacked Lensing Measurements with Subaru HSC Year 3 data

Across the soft gamma-ray regime: utilizing simultaneous detections in the Compton Spectrometer and Imager (COSI) and the Background and Transient Observer (BTO) to understand astrophysical transients

Kavli Affiliate: Tadayuki Takahashi | First 5 Authors: Hannah C. Gulick, Eliza Neights, Samer Al Nussirat, Claire Tianyi Chen, Kaylie Ching | Summary: The Compton Spectrometer and Imager (COSI) is a NASA funded Small Explorer (SMEX) mission slated to launch in 2027. COSI will house a wide-field gamma-ray telescope designed to survey the entire sky […]


Continue.. Across the soft gamma-ray regime: utilizing simultaneous detections in the Compton Spectrometer and Imager (COSI) and the Background and Transient Observer (BTO) to understand astrophysical transients

Revisiting the Ultraviolet Tail of the Primordial Gravitational Wave

Kavli Affiliate: Misao Sasaki | First 5 Authors: Shi Pi, Misao Sasaki, Ao Wang, Jianing Wang, | Summary: High-frequency primordial gravitational waves (PGWs) with wave numbers larger than the Hubble parameter at the end of inflation are originated from the ultraviolet (UV) modes, which are never stretched out of the horizon. Such a UV tail […]


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Revisiting for maximal flavor violating $Z^{‘}_{eμ}$ and its phenomenology constraints

Kavli Affiliate: Jia Liu | First 5 Authors: Jia Liu, Muyuan Song, Haohao Zhang, , | Summary: Lepton flavor violation (LFV), observed conclusively in neutrino oscillations, remains a pivotal area of investigation due to its absence in the Standard Model (SM). Beyond the Standard Model (BSM) physics explores charged lepton flavor violation (CLFV), particularly through […]


Continue.. Revisiting for maximal flavor violating $Z^{‘}_{eμ}$ and its phenomenology constraints

Ada-adapter:Fast Few-shot Style Personlization of Diffusion Model with Pre-trained Image Encoder

Kavli Affiliate: Jia Liu | First 5 Authors: Jia Liu, Changlin Li, Qirui Sun, Jiahui Ming, Chen Fang | Summary: Fine-tuning advanced diffusion models for high-quality image stylization usually requires large training datasets and substantial computational resources, hindering their practical applicability. We propose Ada-Adapter, a novel framework for few-shot style personalization of diffusion models. Ada-Adapter […]


Continue.. Ada-adapter:Fast Few-shot Style Personlization of Diffusion Model with Pre-trained Image Encoder