Inclusive reactions from finite Minkowski spacetime correlation functions

被引:0
|
作者
Carrillo, Marco A. [1 ,2 ]
Briceno, Raul A. [3 ,4 ]
Sturzu, Alexandru M. [5 ]
机构
[1] Old Dominion Univ, Dept Phys, Norfolk, VA 23529 USA
[2] Thomas Jefferson Natl Accelerator Facil, 12000 Jefferson Ave, Newport News, VA 23606 USA
[3] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[4] Lawrence Berkeley Natl Lab, Nucl Sci Div, Berkeley, CA 94720 USA
[5] Coll William & Mary, Dept Phys, Williamsburg, VA 23187 USA
关键词
PHASE-SHIFTS; STATES;
D O I
10.1103/PhysRevD.110.054503
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The need to determine scattering amplitudes of few-hadron systems for arbitrary kinematics expands a broad set of subfields of modern-day nuclear and hadronic physics. In this work, we expand upon previous explorations on the use of real-time methods, like quantum computing or tensor networks, to determine few-body scattering amplitudes. Such calculations must be performed in a finite Minkowski spacetime, where scattering amplitudes are not well defined. Our previous work presented a conjecture of a systematically improvable estimator for scattering amplitudes constructed from finite-volume correlation functions. Here we provide further evidence that the prescription works for larger kinematic regions than previously explored as well as a broader class of scattering amplitudes. Finally, we devise a new method for estimating the order of magnitude of the error associated with finite time separations needed for such calculations. In units of the lightest mass of the theory, we find that to constrain amplitudes using real-time methods within O(10%), the spacetime volumes must satisfy mL O(10-102)) and mT O(102-104).
引用
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页数:19
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