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Article 2022 · 48 citations

Carbon hysteresis hypothesis as a new approach to emission behavior: A case of top five emitters

Caglar, Abdullah Emre, Mert, Mehmet

Abstract

The purpose of the current study is to explain the unstoppable dramatic increases in emissions by proposing a new hypothesis as carbon hysteresis hypothesis. If the emissions have a path dependence or a unit root, a given shock to the emissions will make its equilibrium to a new level in long-run. In this case, the carbon hysteresis hypothesis will be valid. On the other hand, if the emission series is stationary, emissions will resist given shocks in long-run, hence there will be no hysteresis effect. Furthermore, this study reveals the direction of hysteresis. Accordingly, the positive hysteresis indicates continuous increase in emissions while the negative hysteresis indicates continuous decrease in emissions that means carbon reduction.This study achieves robust results by three different structural break panel unit root strategies. In doing so, the panel unit root tests are performed to test carbon hysteresis on the top-five emitting countries: China, India, Japan, Russian Federation and USA over the time period 1965-2020.The main conclusion is that the carbon hysteresis hypothesis is valid for these countries. Moreover, we estimated six different trend models for each regime of sample period for all countries to determine the direction of the hysteresis. In conclusion, this study proposes a new hypothesis to assist countries on their way to the reduction targets.(c) 2022 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.

Keywords
Positive hysteresis Negative hysteresis Path dependence EKC hypothesis Panel unit root PANEL STATIONARITY TEST UNIT-ROOT TEST CO2 EMISSIONS EMPIRICAL-EVIDENCE ECONOMIC-GROWTH ENERGY CONVERGENCE COUNTRIES IMPACT INCOME
WoS Categories
Geosciences, Multidisciplinary
Sustainable Development Goals
Citation
Journal
GONDWANA RESEARCH
Year
2022
Volume
109
Pages
171-182
ISSN
1342-937X
eISSN
1878-0571
DOI
10.1016/j.gr.2022.05.002
WoS UID
WOS:000805269200006
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