Warm quintessential inflation in the weak dissipative regime accounts for both inflation and dark energy observations while naturally reheating the Universe using the original quintessential inflation model.
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Weakly dissipative quintessence explains DESI phantom crossing in dark energy without pathological dynamics.
citing papers explorer
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Warm Quintessential Inflation
Warm quintessential inflation in the weak dissipative regime accounts for both inflation and dark energy observations while naturally reheating the Universe using the original quintessential inflation model.
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Dissipative Dark Energy can explain the DESI phantom crossing
Weakly dissipative quintessence explains DESI phantom crossing in dark energy without pathological dynamics.