ν = q · P M = E − E′ is the lepton’s energy loss in the nucleon rest frame (in earlier literature sometimes ν = q · P ). Here, E and E′ are the initial and final lepton energies in the nucleon rest frame. Q2 = −q2 = 2(EE′−−→k · −→k ′)−m2 −m2 ′ where m (m ′) is the initial (final) lepton mass. If EE′ sin2(θ/2) m2 , m2 ′ , then ≈ 4EE′ sin2(θ/2), where θ is the lepton’s scattering angle with respe...

We introduce a new semantics for modal predicate logic, with respect to which a rich class of first-order modal logics is complete, namely all normal first-order modal logics that are extensions of free quantified K. This logic is defined by combining positive free logic with equality PFL . = and the propositional modal logic K. We then uniformly construct—for each modal predicate logic L—a can...

ν = q · P M = E − E′ is the lepton’s energy loss in the nucleon rest frame (in earlier literature sometimes ν = q · P ). Here, E and E′ are the initial and final lepton energies in the nucleon rest frame. Q2 = −q2 = 2(EE′−−→k · −→k ′)−m2 −m2 ′ where m (m ′) is the initial (final) lepton mass. If EE′ sin2(θ/2) m2 , m2 ′ , then ≈ 4EE′ sin2(θ/2), where θ is the lepton’s scattering angle with respe...

This paper uses frame techniques to characterize the Schatten class properties of integral operators. The main result shows that if the coefficients {〈k,Φm,n〉} of certain frame expansions of the kernel k of an integral operator are in l, then the operator is Schatten p-class. As a corollary, we conclude that if the kernel or Kohn-Nirenberg symbol of a pseudodifferential operator lies in a parti...

Abstract The third realization of the International Celestial Reference Frame (ICRF3) was adopted in August 2018 and includes positions extragalactic objects at three frequencies: 8.4 GHz, 24 32 GHz. In this paper, we present celestial reference frames estimated from Very Long Baseline Interferometry measurements K-band (24 GHz) including data until June 2022. set starts May 2002 currently cons...

In this paper we firstly propose simple and computationally efficient wireless channel modeling algorithm that explicitly takes into account firstand second-order statistics of frame error observations. For this purpose we use discrete-time Markov modulated processes with at most single event (error) at any time slot. We then adopt the special solution of the inverse eigenvalue problem initiall...

We deal with beginning stability theory for “reasonable” non-elementary classes without any remnants of compactness like dealing with models above Hanf number or by the class being definable by Lω1,ω. We introduce and investigate good λ-frame, show that they can be found under reasonable assumptions and prove we can advance from λ to λ+ when non-structure fail. That is, assume 2 +n < 2 +n+1 for...

1. A simple network consisting of two nodes, X and Z is shown in Fig 1. The nodes are separated by a distance of L = 800 m, and each node has a single frame of F = 1500 bits (including all headers and preambles) to send to each other. Both nodes attempt to transmit at time t = 0. In case that a node detects a collision, the node executes the exponential back-off algorithm. In the exponential ba...

Nomenclature A = n×n matrix with elements depending by) , 1 (2 n i i   variances A 1 = (n-1)×(n-1) matrix with elements depending by) , 1 (2 n i i   variances a = output acceleration (perturbed signal) a c = cross-axis acceleration a i = input acceleration B = n×1 matrix with all elements equal to 1 B 1 = (n-1)×1 matrix with all elements equal to 1 B = bias b i = sensors measurement biases)...