Early Bright Galaxies from Helium Enhancements in High-Redshift Star Clusters

Kavli Affiliate: Alexander P. Ji | First 5 Authors: Harley Katz, Alexander P. Ji, O. Grace Telford, Peter Senchyna, | Summary: The first few cycles of JWST have identified an overabundance of UV-bright galaxies and a general excess of UV luminosity density at $zgtrsim10$ compared to expectations from most (pre-JWST) theoretical models. Moreover, some of […]


Continue.. Early Bright Galaxies from Helium Enhancements in High-Redshift Star Clusters

Early Bright Galaxies from Helium Enhancements in High-Redshift Star Clusters

Kavli Affiliate: Alexander P. Ji | First 5 Authors: Harley Katz, Alexander P. Ji, O. Grace Telford, Peter Senchyna, | Summary: The first few cycles of JWST have identified an overabundance of UV-bright galaxies and a general excess of UV luminosity density at $zgtrsim10$ compared to expectations from most (pre-JWST) theoretical models. Moreover, some of […]


Continue.. Early Bright Galaxies from Helium Enhancements in High-Redshift Star Clusters

Early Bright Galaxies from Helium Enhancements in High-Redshift Star Clusters

Kavli Affiliate: Alexander P. Ji | First 5 Authors: Harley Katz, Alexander P. Ji, O. Grace Telford, Peter Senchyna, | Summary: The first few cycles of JWST have identified an overabundance of UV-bright galaxies and a general excess of UV luminosity density at $zgtrsim10$ compared to expectations from most (pre-JWST) theoretical models. Moreover, some of […]


Continue.. Early Bright Galaxies from Helium Enhancements in High-Redshift Star Clusters

LightTransfer: Your Long-Context LLM is Secretly a Hybrid Model with Effortless Adaptation

Kavli Affiliate: Wei Gao | First 5 Authors: Xuan Zhang, Fengzhuo Zhang, Cunxiao Du, Chao Du, Tianyu Pang | Summary: Scaling language models to handle longer contexts introduces substantial memory challenges due to the growing cost of key-value (KV) caches. Motivated by the efficiency gains of hybrid models and the broad availability of pretrained large […]


Continue.. LightTransfer: Your Long-Context LLM is Secretly a Hybrid Model with Effortless Adaptation

Machine-Learning Analysis of Radiative Decays to Dark Matter at the LHC

Kavli Affiliate: Marcela Carena | First 5 Authors: Ernesto Arganda, Marcela Carena, Martín de los Rios, Andres D. Perez, Duncan Rocha | Summary: The search for weakly interacting matter particles (WIMPs) is one of the main objectives of the High Luminosity Large Hadron Collider (HL-LHC). In this work we use Machine Learning (ML) techniques to […]


Continue.. Machine-Learning Analysis of Radiative Decays to Dark Matter at the LHC

Machine-Learning Analysis of Radiative Decays to Dark Matter at the LHC

Kavli Affiliate: Marcela Carena | First 5 Authors: Ernesto Arganda, Marcela Carena, Martín de los Rios, Andres D. Perez, Duncan Rocha | Summary: The search for weakly interacting matter particles (WIMPs) is one of the main objectives of the High Luminosity Large Hadron Collider (HL-LHC). In this work we use Machine-Learning (ML) techniques to explore […]


Continue.. Machine-Learning Analysis of Radiative Decays to Dark Matter at the LHC

Search for non-virialized axions with 3.3-4.2 $μ$eV mass at selected resolving powers

Kavli Affiliate: Chao-Lin Kuo | First 5 Authors: A. T. Hipp, A. Quiskamp, T. J. Caligiure, J. R. Gleason, Y. Han | Summary: The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions compose a fraction of the dark matter with a non-negligible local density. Detecting these low-velocity dispersion flows requires a […]


Continue.. Search for non-virialized axions with 3.3-4.2 $μ$eV mass at selected resolving powers

Search for non-virialized axions with 3.3-4.2 $μ$eV mass at selected resolving powers

Kavli Affiliate: Chao-Lin Kuo | First 5 Authors: A. T. Hipp, A. Quiskamp, T. J. Caligiure, J. R. Gleason, Y. Han | Summary: The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions compose a fraction of the dark matter with a non-negligible local density. Detecting these low-velocity dispersion flows requires a […]


Continue.. Search for non-virialized axions with 3.3-4.2 $μ$eV mass at selected resolving powers

Search for non-virialized axions with 3.3-4.2 $μ$eV mass at selected resolving powers

Kavli Affiliate: Chao-Lin Kuo | First 5 Authors: A. T. Hipp, A. Quiskamp, T. J. Caligiure, J. R. Gleason, Y. Han | Summary: The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions compose a fraction of the dark matter with a non-negligible local density. Detecting these low-velocity dispersion flows requires a […]


Continue.. Search for non-virialized axions with 3.3-4.2 $μ$eV mass at selected resolving powers