X-ray and Radio Campaign of the Z-source GX 340+0 II: the X-ray polarization in the normal branch

Kavli Affiliate: Deepto Chakrabarty| First 5 Authors: Yash Bhargava, Yash Bhargava, , , | Summary:We present the first X-ray polarization measurement of the neutron star low-mass X-ray binary and Z-source, GX 340$+$0, in the normal branch (NB) using a 200 ks observation with the Imaging X-ray Polarimetric Explorer (IXPE). This observation was performed in 2024 […]


Continue.. X-ray and Radio Campaign of the Z-source GX 340+0 II: the X-ray polarization in the normal branch

Measurement of the time-integrated CP asymmetry in $D^{0}rightarrow K^{0}_{S}K^{0}_{S}$ decays using Belle and Belle II data

Kavli Affiliate: T. Higuchi | First 5 Authors: Belle, Belle II Collaborations, :, I. Adachi, L. Aggarwal | Summary: We measure the time-integrated CP asymmetry in $D^{0} rightarrow K^{0}_{S}K^{0}_{S}$ decays reconstructed in $e^{+}e^{-} rightarrow coverline{c}$ events collected by the Belle and Belle II experiments. The corresponding data samples have integrated luminosities of 980 fb$^{-1}$ and […]


Continue.. Measurement of the time-integrated CP asymmetry in $D^{0}rightarrow K^{0}_{S}K^{0}_{S}$ decays using Belle and Belle II data

Measurement of the time-integrated CP asymmetry in $D^{0}rightarrow K^{0}_{S}K^{0}_{S}$ decays using Belle and Belle II data

Kavli Affiliate: T. Higuchi | First 5 Authors: Belle, Belle II Collaborations, :, I. Adachi, L. Aggarwal | Summary: We measure the time-integrated CP asymmetry in $D^{0} rightarrow K^{0}_{S}K^{0}_{S}$ decays reconstructed in $e^{+}e^{-} rightarrow coverline{c}$ events collected by the Belle and Belle II experiments. The corresponding data samples have integrated luminosities of 980 fb$^{-1}$ and […]


Continue.. Measurement of the time-integrated CP asymmetry in $D^{0}rightarrow K^{0}_{S}K^{0}_{S}$ decays using Belle and Belle II data

Measurement of the time-integrated CP asymmetry in $D^0rightarrow K^0_SK^0_S$ decays using Belle and Belle II data

Kavli Affiliate: T. Higuchi | First 5 Authors: , , , , | Summary: We measure the time-integrated CP asymmetry in $D^0 rightarrow K^0_SK^0_S$ decays reconstructed in $e^+e^- rightarrow coverlinec$ events collected by the Belle and Belle II experiments. The corresponding data samples have integrated luminosities of 980 fb$^-1$ and 428 fb$^-1$, respectively. The $D^0$ […]


Continue.. Measurement of the time-integrated CP asymmetry in $D^0rightarrow K^0_SK^0_S$ decays using Belle and Belle II data

Redefining in Dictionary: Towards a Enhanced Semantic Understanding of Creative Generation

Kavli Affiliate: Jing Wang | First 5 Authors: Fu Feng, Yucheng Xie, Jing Wang, Xin Geng, | Summary: Creativity, both in human and diffusion models, remains an inherently abstract concept; thus, simply adding "creative" to a prompt does not yield reliable semantic recognition by the model. In this work, we concretize the abstract notion of […]


Continue.. Redefining in Dictionary: Towards a Enhanced Semantic Understanding of Creative Generation

Redefining in Dictionary: Towards an Enhanced Semantic Understanding of Creative Generation

Kavli Affiliate: Jing Wang | First 5 Authors: Fu Feng, Yucheng Xie, Xu Yang, Jing Wang, Xin Geng | Summary: “Creative” remains an inherently abstract concept for both humans and diffusion models. While text-to-image (T2I) diffusion models can easily generate out-of-domain concepts like “a blue banana”, they struggle with generating combinatorial objects such as “a […]


Continue.. Redefining in Dictionary: Towards an Enhanced Semantic Understanding of Creative Generation

Hair is complicated: Gravitational waves from stable and unstable boson-star mergers

Kavli Affiliate: Ulrich Sperhake| First 5 Authors: Bo-Xuan Ge, Bo-Xuan Ge, , , | Summary:We explore the gravitational-wave emission from head-on collisions of equal-mass solitonic boson-star binaries from simulations spanning a two-dimensional parameter space, consisting of the central scalar-field amplitude of the stars and the solitonic potential parameter. We report the gravitational-wave energies emitted by […]


Continue.. Hair is complicated: Gravitational waves from stable and unstable boson-star mergers