A Novel Mathematical and Physics-Based Approach to Greenhouse Gas (GHG) accounting: Integrating Temporal and Spatial Emissions for Precision Reporting

A Novel Mathematical and Physics-Based Approach to Greenhouse Gas (GHG) accounting: Integrating Temporal and Spatial Emissions for Precision Reporting

Abstract: Greenhouse Gas (GHG) quantification and analysis are critical for global emissions reduction frameworks. Traditional reporting methodologies often fail to integrate time-variable emissions and spatial-temporal dispersion into analytical models. This paper introduces a double-integrated mathematical model grounded in thermodynamics, partial differential equations, and flux analysis to improve GHG monitoring and forecasting precision across energy systems and industrial processes.

1. Introduction Global GHG emissions are typically evaluated through inventories that rely on approximations and sectoral data. However, to ensure accuracy, it is essential to integrate time-variable emission sources, thermal transfer mechanisms, and system boundaries into emission models. Herein, we expand on two primary integrations:

  • Double Integration for Cumulative Emission Calculations
  • Flux Dispersion to Account for Atmospheric Transfer Dynamics

2. Mathematical Framework: Double Integration of GHG Flux

2.1 Temporal Integration of Emissions The instantaneous emission rate E(t) can be defined as a function of time-dependent emission factors and operational parameters. The total emissions G(t) can be calculated by integrating E(t)E(t)E(t) over a specific time period [t0,tf]:

G(t)=∫t0tfE(t)dt


If the emission flux E(t) varies with both space xxx and time, a double integration is required:

G=∬SE(x,t)dAdt

where dA represents an infinitesimal area within the spatial boundary SSS. This captures spatial heterogeneity in emissions, critical for industrial sites with uneven emission profiles.

2.2 Physics of GHG Flux and Atmospheric Dynamics Greenhouse gases, once emitted, are subject to thermal expansion, diffusion, and advection within the atmosphere. The continuity equation for atmospheric transfer is given by:

∂t/∂ρ+∇⋅(ρv)=S

where:

  • ρ = density of the GHG
  • v= velocity vector of atmospheric dispersion
  • S= source term (emission rate per unit volume)

By solving this equation under steady-state conditions with boundary constraints, we derive flux gradients that predict GHG concentrations over time and space.

3. Thermal Transfer and Entropy Integration

Given the thermal properties of GHGs (e.g., CO₂, CH₄), energy conservation laws dictate their contribution to radiative forcing. The Boltzmann entropy equation explains the heat transfer effect:

ΔS=∫Tδ/Q

where ΔS is the change in system entropy and δQ is the heat transfer caused by GHG energy absorption.

To relate this to emission profiles, we integrate thermal transfer with the emission flux:

ΔQ=∬SαE(x,t)dAdt


where α is the radiative forcing coefficient unique to each GHG species.


4. Application to Energy Systems When analyzing emissions from energy generation systems (e.g., fossil fuel combustion), the proposed mathematical model integrates both combustion efficiency and enthalpy losses:

Combustion Emission Rate:

Ecomb=ηmf⋅Cf⋅Foxid

Mathematical research plays a critical role in understanding and addressing greenhouse gas (GHG) emissions, particularly methane (CH₄), which is a highly potent contributor to global warming. By utilizing advanced mathematical tools, researchers can model reaction kinetics, such as methane oxidation in the atmosphere, using differential equations and rate laws to predict the behavior of these reactions over time. For instance, the Arrhenius equation is employed to understand how temperature variations affect the rate of methane decomposition. Additionally, methane's atmospheric lifetime, estimated at approximately 12 years, is calculated through its reaction with hydroxyl radicals (OH), helping to quantify its long-term warming potential, which is 25–30 times greater than that of carbon dioxide (CO₂).

Thermodynamic calculations, such as enthalpy changes (ΔH), are used to determine the energy released during methane combustion or oxidation, illustrating the exothermic nature of these processes. Furthermore, metrics like the Global Warming Potential (GWP) are derived mathematically to assess methane’s cumulative impact over specific time horizons, such as 20 or 100 years. Numerical simulations, including computational fluid dynamics and atmospheric chemistry models, allow researchers to analyze methane’s dispersion, reaction pathways, and overall contribution to GHG levels with great precision. These models also help in projecting methane emissions' future impact and evaluating mitigation strategies, such as reducing emissions or increasing the availability of hydroxyl radicals.

In reporting, mathematical insights offer significant advantages. Data visualization through graphs and energy diagrams provides a clear representation of reaction kinetics and energy pathways, making complex processes more comprehensible. Projections based on mathematical models, such as methane’s GWP or emission reduction scenarios, provide policymakers with the quantitative evidence needed to shape effective environmental regulations. Additionally, scenario analyses can highlight potential outcomes under different mitigation strategies, ensuring that reports are actionable and informative. By grounding reports in validated mathematical models, researchers ensure scientific accuracy, credibility, and clarity, offering stakeholders essential tools for decision-making and climate action planning.

Greenhouse Gas Protocol (GHG Protocol) EY UN Climate Change



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