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E 1.99:1802478
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Elliptic flow coalescence to identify the $f_0$(980) content |
1 |
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E 1.99:1802480
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<small>HIJING</small> can describe the anisotropy-scaled charge-dependent correlations at the BNL Relativistic Heavy Ion Collider |
1 |
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E 1.99:1802483
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Microbial potentiometric sensor technology for real-time detecting and monitoring of toxic metals in aquatic matrices |
1 |
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E 1.99:1802484
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Operation and performance of microhexcavity pixel detector in gas discharge and avalanche mode |
1 |
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E 1.99:1802485
|
Structural trends in atomic nuclei from laser spectroscopy of tin |
1 |
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E 1.99:1802486
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Gamow-shell-model description of Li isotopes and their mirror partners |
1 |
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E 1.99:1802488
|
Nuclear modification of leading hadrons and jets within a virtuality ordered parton shower |
1 |
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E 1.99:1802489
|
Energy and scale dependence of $\hat{q}$ and the ?JET puzzle? |
1 |
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E 1.99:1802493
|
Exact solution for the non-equilibrium attractor in number-conserving relaxation time approximation |
1 |
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E 1.99:1802502
|
Dynamical friction in superfluids |
1 |
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E 1.99:1802503
|
Baryon-Interacting Dark Matter heating dark matter and the emergence of galaxy scaling relations. |
1 |
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E 1.99:1802505
|
Early Dark Energy from Massive Neutrinos as a Natural Resolution of the Hubble Tension |
1 |
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E 1.99:1802511
|
Collapse of the waiting time effect in a spin glass |
1 |
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E 1.99:1802512
|
Axion periodicity and coupling quantization in the presence of mixing |
1 |
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E 1.99:1802513
|
Repulsive forces and the weak gravity conjecture |
1 |
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E 1.99:1802516
|
<sup>9</sup>Li($\textit{d,p}$) reaction as a specific probe of <sup>10</sup>Li, the paradigm of parity-inverted nuclei around the $\textit{N}$ = 6 closed shell |
1 |
|
E 1.99:1802517
|
In search of large signals at the cosmological collider |
1 |
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E 1.99:1802520
|
Low-dimensional de Sitter quantum gravity |
1 |
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E 1.99:1802526
|
A Hybrid Deep Learning Approach to Cosmological Constraints from Galaxy Redshift Surveys |
1 |
|
E 1.99:1802537
|
Warming nuclear pasta with dark matter kinetic and annihilation heating of neutron star crusts. |
1 |
