This analysis used the backpropagation Levenberg-Marquardt technique coupled through neural networks (BPLMT-NN). The magnetohydrodynamic (MHD) viscous nanofluid flow due to the rotating disk (MHD-VNRD) through the slip effect was investigated. In the existence of a velocity slip condition, this communication investigated the boundary coating flow of viscous nanofluid under MHD conditions. The flow was produced by a disk that was revolving. A fluid effects electricity under the effect of a magnetic field that is transverse. The magnetic field that is generated is neglected when the magnetic Reynolds number is low. The properties of Brownian and thermophoresis motion were demonstrated using a nanofluid simulation. Hypotheses about the boundary coating and low magnetic Reynolds number were made while formulating the problem. To transform nonlinear partial differential equations into a scheme of ordinary differential equations, the similarity transformation was utilized. On the profiles of velocity, temperature, and concentration, a data set for the suggested (BPLMT-NN) was created for the impacts of several important parameters and was illustrated via the explicit Runge-Kutta technique. Using the (BPLMT-NN) testing, training, and validation approach, the estimated result of various situations was endorsed, and the suggested model was evaluated for fitness. After that, the proposed (BPLMT-NN) was validated using mean square error (MSE), regression analysis, and histogram investigations. The novelty of the proposed BPLMT-NN technique has various applications, such as disease diagnosis, robotic control systems, ecosystem evaluation, etc. We conducted analyses of some statistical data like gradient, performance, and epoch of the proposed fluid model. Based on closeness, as well as recommended and reference results, the suggested approach has made a distinction with precision level varying from 10−09 to 10−11.
Citation: Yousef Jawarneh, Samia Noor, Ajed Akbar, Rafaqat Ali Khan, Ahmad Shafee. Intelligent neural networks approach for analysis of the MHD viscous nanofluid flow due to rotating disk with slip effect[J]. AIMS Mathematics, 2025, 10(5): 10387-10412. doi: 10.3934/math.2025473
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Abstract
This analysis used the backpropagation Levenberg-Marquardt technique coupled through neural networks (BPLMT-NN). The magnetohydrodynamic (MHD) viscous nanofluid flow due to the rotating disk (MHD-VNRD) through the slip effect was investigated. In the existence of a velocity slip condition, this communication investigated the boundary coating flow of viscous nanofluid under MHD conditions. The flow was produced by a disk that was revolving. A fluid effects electricity under the effect of a magnetic field that is transverse. The magnetic field that is generated is neglected when the magnetic Reynolds number is low. The properties of Brownian and thermophoresis motion were demonstrated using a nanofluid simulation. Hypotheses about the boundary coating and low magnetic Reynolds number were made while formulating the problem. To transform nonlinear partial differential equations into a scheme of ordinary differential equations, the similarity transformation was utilized. On the profiles of velocity, temperature, and concentration, a data set for the suggested (BPLMT-NN) was created for the impacts of several important parameters and was illustrated via the explicit Runge-Kutta technique. Using the (BPLMT-NN) testing, training, and validation approach, the estimated result of various situations was endorsed, and the suggested model was evaluated for fitness. After that, the proposed (BPLMT-NN) was validated using mean square error (MSE), regression analysis, and histogram investigations. The novelty of the proposed BPLMT-NN technique has various applications, such as disease diagnosis, robotic control systems, ecosystem evaluation, etc. We conducted analyses of some statistical data like gradient, performance, and epoch of the proposed fluid model. Based on closeness, as well as recommended and reference results, the suggested approach has made a distinction with precision level varying from 10−09 to 10−11.
1.
Introduction
Random numbers are very important in statistical, probability theory, and mathematical analysis in such complex cases, where the real numbers are difficult to record. The random numbers are generated from the uniform distribution when an interval is defined for their selection of random numbers. The random numbers are generated in sequence and depict the behavior of the real data. In addition, random data can be used for estimation and forecasting purposes. According to [1], "The method is based on running the model many times as in random sampling. For each sample, random variates are generated on each input variable; computations are run through the model yielding random outcomes on each output variable. Since each input is random, the outcomes are random. In the same way, they generated thousands of such samples and achieved thousands of outcomes for each output variable. In order to carry out this method, a large stream of random numbers was needed". To generate random numbers, a random generator is applied. The random numbers have no specific pattern and are generated from the chance process. Nowadays, the latest computer can be used to generate random numbers using a well-defined algorithm; see [1]. Bang et al. [2] investigated normality using random-number generating. Schulz et al. [3] presented a pattern-based approach. Tanyer [4] generated random numbers from uniform sampling. Kaya and Tuncer [5] proposed a method to generate biological random numbers. Tanackov et al. [6] presented a method to generate random numbers from the exponential distribution. Jacak et al. [7] presented the methods to generate pseudorandom numbers. More methods can be seen in [8,9,10].
The neutrosophic statistical distributions were found to be more efficient than the distributions under classical statistics. The neutrosophic distributions can be applied to analyze the data that is given in neutrosophic numbers. Sherwani et al. [11] proposed neutrosophic normal distribution. Duan et al. [12] worked on neutrosophic exponential distribution. Aliev et al. [13] generated Z-random numbers from linear programming. Gao and Ralescu [14] studied the convergence of random numbers generated under an uncertain environment. More information on random numbers generators can be seen in [15,16,17,18]. In recent works, Aslam [19] introduced a truncated variable algorithm for generating random variates from the neutrosophic DUS-Weibull distribution. Additionally, in another study [20], novel methods incorporating sine-cosine and convolution techniques were introduced to generate random numbers within the framework of neutrosophy. Albassam et al. [21] showcased probability/cumulative density function plots and elucidated the characteristics of the neutrosophic Weibull distribution as introduced by [22]. The estimation and application of the neutrosophic Weibull distribution was also presented by [21].
In [22], the Weibull distribution was introduced within the realm of neutrosophic statistics, offering a more inclusive perspective compared to its traditional counterpart in classical statistics. [21] further examined the properties of the neutrosophic Weibull distribution introduced by [22]. Despite an extensive review of existing literature, no prior research has been identified regarding the development of algorithms for generating random numbers using both the neutrosophic uniform and Weibull distributions. This paper aims to bridge this gap by presenting innovative random number generators tailored specifically for the neutrosophic uniform distribution and the neutrosophic Weibull distribution. The subsequent sections will provide detailed explanations of the algorithms devised to generate random numbers for these distributions. Additionally, the paper will feature multiple tables showcasing sets of random numbers across various degrees of indeterminacy. Upon thorough analysis, the results reveal a noticeable decline in random numbers as the degree of indeterminacy increases.
2.
Neutrosophic uniform distribution
Let xNU=xNL+xNUIxNU;IxNUϵ[IxLU,IxUU] be a neutrosophic random variable that follows the neutrosophic uniform distribution. Note that the first part xNL denotes the determinate part, xNUIxNU the indeterminate part, and IxNUϵ[IxLU,IxUU] the degree of indeterminacy. Suppose f(xNU)=f(xLU)+f(xUU)INU;INUϵ[ILU,IUU] presents the neutrosophic probability density function (npdf) of neutrosophic uniform distribution (NUD). Note that the npdf of NUD is based on two parts. The first part xNL, f(xLU) denotes the determinate part and presents the probability density function (pdf) of uniform distribution under classical statistics. The second part xNUIxNU, f(xUU)INU denotes the indeterminate part and IxNUϵ[IxLU,IxUU], INUϵ[ILU,IUU] are the measures of indeterminacy associated with neutrosophic random variable and the uniform distribution. The npdf of the uniform distribution by following [22] is given as
Note here that the npdf of uniform distribution is a generalization of pdf of the uniform distribution. The neutrosophic uniform distribution reduces to the classical uniform distribution when IxUU = 0. The neutrosophic cumulative distribution function (ncdf) of the neutrosophic uniform distribution is given by
Note that the first part presents the cumulative distribution function (cdf) of the uniform distribution under classical statistics, and the second part is the indeterminate part associated with ncdf. The ncdf reduces to cdf when IxUU = 0. The simplified form of ncdf of the Uniform distribution when L=U=S can be written as
where α and β are the scale and shape parameters of the Weibull distribution. The npdf of the Weibull distribution reduces to pdf of the Weibull distribution when INS=0. The ncdf of the Weibull distribution is expressed by
F(xNSW)=1−{e−(xNSWα)β(1+INW)}+INW;INWϵ[ILW,IUW].
(8)
The ncdf of the Weibull distribution reduces to cdf of the Weibull distribution under classical statistics when INW = 0. The neutrosophic mean of the Weibull distribution is given as [22]
μNW=αΓ(1+1/β)(1+INW);INWϵ[ILW,IUW].
(9)
The neutrosophic median of the Weibull distribution is given by
˜μNW=α(ln(2))1/β(1+INW);INWϵ[ILW,IUW].
(10)
4.
Simulation methodology
This section presents the methodology to generate random variates from the proposed neutrosophic uniform distribution and the neutrosophic Weibull distribution. Let uNϵ[uL,uU] be a neutrosophic random uniform from uN∼UN([0,0],[1,1]). The neutrosophic random numbers from NUD and NWD will be obtained as follows:
Step-4: From the routine, the first value of xNSW will be generated.
Step-5: Repeat the routine k times to generate k random numbers from NWD.
4.1. Examples
To illustrate the proposed simulation methods, two examples will be discussed in this section.
4.1.1. Example 1
Suppose that xNSU is a neutrosophic uniform random variable with parameters ([20,20],[30,30]) and a random variate xNSU under indeterminacy is needed. To generate a random number from NUD, the following steps have been carried out.
Step-1: Generate a uniform random number uN=0.05 from uN∼UN([0,0],[1,1]).
Step-2: Fix the values of INS=0.1.
Step-3: Generate values of xNSU using the expression xNSU=20+(0.05(1+0.1))(30−20)=20.5.
Step-4: From the routine, the first value of xNSU=20.5 will be generated.
Step-5: Repeat the routine k times to generate k random numbers from NUD.
4.1.2. Example 2
Step-1: Generate a uniform random number uN=0.30 from uN∼UN([0,0],[1,1]).
Step-2: Fix the values of INS=0.20, α=5, and β=0.5.
Step-3: Generate values of xNSW using the expression xNSW=5[−ln(1−(uN−INW)1+INW)]10.5=0.04.
Step-4: From the routine, the first value of xNSW=0.04 will be generated.
Step-5: Repeat the routine k times to generate k random numbers from NWD.
5.
Simulation study
In this section, random numbers are generated by simulation using the above-mentioned algorithms for NUD and NWD. To generate random numbers from NUD, several uniform numbers are generated from uN∼UN([0,0],[1,1]) and placed in Tables 1 and 2. In Tables 1 and 2, several values of INS are considered to generate random numbers from the NUD. Table 1 is depicted by assuming that NUD has the parameters aNS = 10 and bNS = 20 and Table 2 is shown by assuming that NUD has the parameters aNS = 20 and bNS = 30. From Tables 1 and 2, the following trends can be noted in random numbers generated from NUD.
Table 1.
Random numbers from NUD when aNS = 10 and bNS = 20.
1) For fixed INS, aNS = 10 and bNS = 20, as the values of u increase from 0.05 to 0.95, there is an increasing trend in random numbers.
2) For fixed u, aNS = 10 and bNS = 20, as the values of INS increase from 0 to 1.1, there is a decreasing trend in random numbers.
3) For fixed values of u and INS, as the values of aNS and bNS increases, there is an increasing trend in random numbers.
The random numbers for NWD are generated using the algorithm discussed in the last section. The random numbers for various values of u, INS, α, and β are considered. The random numbers when α=5 and β=0 are shown in Table 3. The random numbers when α=5 and β=1 are shown in Table 4. The random numbers when α=5 and β=2 are shown in Table 5.
Table 3.
Random numbers from NUD when α=5 and β=0.5.
In this section, the performance of simulations using classical simulation and neutrosophic simulation will be discussed using the random numbers from the NUD and the NWD distribution. As explained earlier, the proposed simulation method under neutrosophy will be reduced to the classical simulation method under classical statistics when no uncertainty is found in the data. To study the behavior of random numbers, random numbers from NUD when INS=1.1, aNS = 20, and bNS = 30 are considered and depicted in Figure 3. In Figure 3, it can be seen that the curve of random numbers from the classical simulation is higher than the curve of random numbers from the neutrosophic simulation. From Figure 3, it is clear that the proposed neutrosophic simulation method gives smaller values of random numbers than the random numbers generated by the neutrosophic simulation method. The random numbers from NWD when INS=0.9, α=5, and β=0.5 are considered and their curves are shown in Figure 4. From Figure 4, it can be seen that random numbers generated by neutrosophic simulation are smaller than the random numbers generated by the classical simulation method under classical statistics. The random numbers generated by the neutrosophic simulation are close to zero. The random numbers from NWD when INS=0.1, α=5, and β=1 (exponential distribution) are considered and their curves are shown in Figure 5. From Figure 5, it can be seen that the curve of random numbers generated by neutrosophic simulation is lower than the curve of random numbers generated by the classical simulation method under classical statistics. The random numbers from NWD when INS=0.1, α=5, and β=2 are considered and their curves are shown in Figure 6. From Figure 6, it can be seen that the curve of random numbers generated by neutrosophic simulation is lower than the curve of random numbers generated by the classical simulation method under classical statistics. From Figures 4–6, it can be concluded that the proposed simulation gives smaller values of random numbers as compared to the classical simulation method under classical statistics.
Figure 3.
Random numbers behavior from NUD when INS=1.1, aNS = 20, and bNS = 30.
The simulation method under neutrosophic statistics and classical methods was discussed in the last sections. From Tables 1 and 2, it can be seen that random numbers from the NUD can be generated when INS<1, INS=1 and INS>1. On the other hand, the random numbers from the NWD can be generated for INS<1, INS=1, and INS>1 when the shape parameter β<1. From Table 4 and 5, it can be noted that for several cases, the NWD generates negative results or random numbers do not exist. Based on the simulation studies, it can be concluded that the NWD generates random numbers INS<1, INS=1, and INS>1 only when β<1. To generate random numbers from NWD when β≥1, the following expression will be used
xNSW=α[−ln(1−uN+INW1+INW)]1β;1−uN+INW≥0.
8.
Concluding remarks
In this paper, we initially introduced the NUD and presented a novel method for generating random numbers from both NUD and the NWD. We also introduced algorithms for generating random numbers within the context of neutrosophy. These algorithms were applied to generate random numbers from both distributions using various parameters. We conducted an extensive discussion on the behavior of these random numbers, observing that random numbers generated under neutrosophy tend to be smaller than those generated under uncertain environments. It is worth noting that generating random numbers from computers is a common practice. Tables 1–5 within this paper offer valuable insights into how the degree of determinacy influences random number generation. Additionally, these tables can be utilized for simulation purposes in fields marked by uncertainty, such as reliability, environmental studies, and medical science. From our study, we conclude that the proposed method for generating random numbers from NUD and NWD can be effectively applied in complex scenarios. In future research, exploring the statistical properties of the proposed NUD would be advantageous. Additionally, investigating the proposed algorithm utilizing the accept-reject method could be pursued as a future research avenue. Moreover, there is potential to develop algorithms using other statistical distributions for further investigation.
Use of AI tools declaration
The authors declare they have not used Artificial Intelligence (AI) tools in the creation of this article.
Acknowledgements
The authors are deeply thankful to the editor and reviewers for their valuable suggestions to improve the quality and presentation of the paper.
Conflict of interest
The authors declare no conflicts of interest.
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Figure 2. The MHD-VNRD model's neural network architecture
Figure 3. The structure of a particular neuron type
Figure 4. The workflow method for BPLMT-NN that is applied for the MHD-VNRD model
Figure 5(ⅰ). Suggested BPLMT-NN error histogram, performance, and fitness solutions for solving Case 4 of Scenarios 1–3 in the MHD-VNRD model
Figure 5(ⅱ). Suggested BPLMT-NN error histogram, performance, and fitness solutions for solving Case 4 of Scenarios 4–6 in the MHD-VNRD model
Figure 6(ⅰ). Proposed BPLMT-NN state transition and regression efficiency to solve the MHD-VNRD model for Scenarios 1–3 of Case 4
Figure 6(ⅱ). Proposed BPLMT-NN state transition and regression efficiency to solve the MHD-VNRD model for Scenarios 4–6 of Case 4
Figure 7(ⅰ). Evaluation of suggested numerical consequences with recommended BLMS-ANNs Scenarios 1–3 of the MHD-VNRD model
Figure 7(ⅱ). Evaluation of suggestion numerical consequences with recommended BLMS-ANNs for Scenarios 4–6 of the MHD-VNRD model
Figure 8(ⅰ). Suggested BPLMT-NN evaluation includes findings of absolute error analysis of the reference set of data for the MHD-VNRD model in Scenarios 1–3
Figure 8(ⅱ). Suggested BPLMT-NN evaluation includes findings of absolute error analysis of the reference set of data for the MHD-VNRD model in Scenarios 4–6