Quantum Hamiltonian Algorithms for Maximum Independent Sets

Kavli Affiliate: Frank Wilczek | First 5 Authors: Xianjue Zhao, Peiyun Ge, Hongye Yu, Li You, Frank Wilczek | Summary: We compare two quantum Hamiltonian algorithms that address the maximum independent set problem: one based on emergent non-abelian gauge matrix in adiabatic evolution of an energetically isolated manifold of states; and one based on designed […]


Continue.. Quantum Hamiltonian Algorithms for Maximum Independent Sets

Quantum Hamiltonian Algorithms for Maximum Independent Sets

Kavli Affiliate: Frank Wilczek | First 5 Authors: Xianjue Zhao, Peiyun Ge, Hongye Yu, Li You, Frank Wilczek | Summary: We compare two quantum Hamiltonian algorithms that address the maximum independent set problem: one based on emergent non-abelian gauge matrix in adiabatic evolution of an energetically isolated manifold of states; and one based on designed […]


Continue.. Quantum Hamiltonian Algorithms for Maximum Independent Sets

Quantum Hamiltonian Algorithms for Maximum Independent Sets

Kavli Affiliate: Frank Wilczek | First 5 Authors: Xianjue Zhao, Peiyun Ge, Hongye Yu, Li You, Frank Wilczek | Summary: With qubits encoded into atomic ground and Rydberg states and situated on the vertexes of a graph, the conditional quantum dynamics of Rydberg blockade, which inhibits simultaneous excitation of nearby atoms, has been employed recently […]


Continue.. Quantum Hamiltonian Algorithms for Maximum Independent Sets

First Detection and Modeling of Spatially Resolved Ly$α$ in TW Hya

Kavli Affiliate: Gregory J. Herczeg | First 5 Authors: Seok-Jun Chang, Nicole Arulanantham, Max Gronke, Gregory J. Herczeg, Edwin A. Bergin | Summary: Lyman-$alpha$ (Ly$alpha$) is the strongest emission line in UV spectra from T-Tauri stars. Due to its resonant nature, Ly$alpha$ emission carries information about the physical properties of the H I medium via […]


Continue.. First Detection and Modeling of Spatially Resolved Ly$α$ in TW Hya

First Detection and Modeling of Spatially Resolved Ly$α$ in TW Hya

Kavli Affiliate: Gregory J. Herczeg | First 5 Authors: Seok-Jun Chang, Nicole Arulanantham, Max Gronke, Gregory J. Herczeg, Edwin A. Bergin | Summary: Lyman-$alpha$ (Ly$alpha$) is the strongest emission line in the accretion-generated UV spectra from T-Tauri stars and, as such, plays a critical role in regulating chemistry within the surrounding protoplanetary disks. Due to […]


Continue.. First Detection and Modeling of Spatially Resolved Ly$α$ in TW Hya

First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52,μ$eV range with a coaxial dish antenna

Kavli Affiliate: Noah A. Kurinsky | First 5 Authors: Stefan Knirck, Gabe Hoshino, Mohamed H. Awida, Gustavo I. Cancelo, Martin Di Federico | Summary: We present first results from a dark photon dark matter search in the mass range from 44 to 52 $mu{rm eV}$ ($10.7 – 12.5,{rm GHz}$) using a room-temperature dish antenna setup […]


Continue.. First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52,μ$eV range with a coaxial dish antenna

First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52,μ$eV range with a coaxial dish antenna

Kavli Affiliate: Noah A. Kurinsky | First 5 Authors: Stefan Knirck, Gabe Hoshino, Mohamed H. Awida, Gustavo I. Cancelo, Martin Di Federico | Summary: We present first results from a dark photon dark matter search in the mass range from 44 to 52 $mu{rm eV}$ ($10.7 – 12.5,{rm GHz}$) using a room-temperature dish antenna setup […]


Continue.. First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52,μ$eV range with a coaxial dish antenna

First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52,μ$eV range with a coaxial dish antenna

Kavli Affiliate: Noah A. Kurinsky | First 5 Authors: Stefan Knirck, Gabe Hoshino, Mohamed H. Awida, Gustavo I. Cancelo, Martin Di Federico | Summary: We present first results from a dark photon dark matter search in the mass range from 44 to 52 $mu{rm eV}$ ($10.7 – 12.5,{rm GHz}$) using a room-temperature dish antenna setup […]


Continue.. First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52,μ$eV range with a coaxial dish antenna

First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52,μ$eV range with a coaxial dish antenna

Kavli Affiliate: Noah A. Kurinsky | First 5 Authors: Stefan Knirck, Gabe Hoshino, Mohamed H. Awida, Gustavo I. Cancelo, Martin Di Federico | Summary: We present first results from a dark photon dark matter search in the mass range from 44 to 52 $mu{rm eV}$ ($10.7 – 12.5,{rm GHz}$) using a room-temperature dish antenna setup […]


Continue.. First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52,μ$eV range with a coaxial dish antenna

First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52,μ$eV range with a coaxial dish antenna

Kavli Affiliate: David W. Miller | First 5 Authors: Stefan Knirck, Gabe Hoshino, Mohamed H. Awida, Gustavo I. Cancelo, Martin Di Federico | Summary: We present first results from a dark photon dark matter search in the mass range from 44 to 52 $mu{rm eV}$ ($10.7 – 12.5,{rm GHz}$) using a room-temperature dish antenna setup […]


Continue.. First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52,μ$eV range with a coaxial dish antenna