{'fraction_non_alphanumeric': 0.03333333333333333, 'fraction_numerical': 0.035333333333333335, 'mean_word_length': 4.795366795366795, 'pattern_counts': {'":': 0, '<': 0, '<?xml version=': 0, '>': 1, 'https://': 0, 'lorem ipsum': 0, 'www.': 0, 'xml': 0}, 'pii_count': 0, 'substrings_counts': 0, 'word_list_counts': {'cursed_substrings.json': 0, 'profanity_word_list.json': 0, 'sexual_word_list.json': 0, 'zh_pornsignals.json': 0}}
Effect of hydrostatic pressure on the superconducting properties of quasi-1D superconductor K2Cr3As3

K2Cr3As3 is a newly discovered quasi-1D superconductor with a Tc  =  6.1 K and an upper critical field µ0Hc2(0)  ≈  40 T three times larger than the Pauli paramagnetic limit µ0Hp that is suggestive of a spin-triplet Cooper pairing. In this paper, we have investigated the effects of hydrostatic pressure on its Tc and µ0Hc2 by measuring the ac magnetic susceptibility χ'(T) under magnetic fields at various hydrostatic pressures up to 7.5 GPa. The major findings include: (1) Tc is suppressed gradually to below 2 K at 7.5 GPa; (2) the estimated µ0Hc2(0) decreases dramatically to below µ0Hp above ~2 GPa and becomes slight lower than the orbital limiting field μ0Hc2orb(0) estimated from the initial slope of upper critical field via μ0Hc2orb(0)  =  −0.73TcdHc2/dTc|Tc in the clean limit; (3) the estimated Maki parameter α  =  √2Hc2orb(0)/Hp drops from 4 at ambient pressure to well below 1 at P  >  2 GPa, suggesting the crossover from Pauli paramagnetic limiting to orbital limiting in the pair breaking process upon increasing pressure. These observations suggested that the application of hydrostatic pressure could drive K2Cr3As3 away from the ferromagnetic instability and lead to a breakdown of the spin-triplet pairing channel. We have also made a side-by-side comparison and discussed the distinct effects of chemical and physical pressures on the superconducting properties of K2Cr3As3.