Bulk superconductivity and role of fluctuations in the iron-based superconductor FeSe at high pressures
Elena Gati, Anna E. B\"ohmer, Sergey L. Bud'ko, and Paul C. Canfield

TL;DR
This study investigates how pressure influences bulk superconductivity and magnetic fluctuations in FeSe, revealing a complex interplay that resembles behaviors seen in cuprate superconductors.
Contribution
It provides the first thermodynamic evidence of bulk superconductivity across a wide pressure range and highlights the role of fluctuations in FeSe.
Findings
Superconductivity remains bulk across all pressures studied.
Magnetic and superconducting fluctuations coexist over a broad temperature range.
Superconductivity competes with magnetism in FeSe.
Abstract
The iron-based superconductor FeSe offers a unique possibility to study the interplay of superconductivity with purely nematic as well magnetic-nematic order by pressure (p) tuning. By measuring specific heat under p up to 2.36GPa, we study the multiple phases in FeSe using a thermodynamic probe. We conclude that superconductivity is bulk across the entire p range and competes with magnetism. Our analysis suggests that superconducting and magnetic fluctuations exist over a wide temperature range above the respective bulk transition temperatures, whenever magnetism is present. These observations highlight similarities between FeSe and underdoped cuprate superconductors where fluctuations play a crucial role.
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Bulk superconductivity and role of fluctuations in the iron-based superconductor FeSe at high pressures
Elena Gati1,2
Anna E. Böhmer1,2,⋆
Sergey L. Bud’ko1,2
Paul C. Canfield1,2
1 Ames Laboratory, US Department of Energy, Iowa State University, Ames, Iowa 50011, USA
2 Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, USA
⋆ current address: Institute for Solid State Physics, Karlsruhe Institute of Technology, 76021 Karlsruhe, Germany
Abstract
The iron-based superconductor FeSe offers a unique possibility to study the interplay of superconductivity with purely nematic as well magnetic-nematic order by pressure () tuning. By measuring specific heat under up to 2.36 GPa, we study the multiple phases in FeSe using a thermodynamic probe. We conclude that superconductivity is bulk across the entire range and competes with magnetism. In addition, whenever magnetism is present, fluctuations exist over a wide temperature range above both the bulk superconducting and the magnetic transitions. Whereas the magnetic fluctuations are likely temporal, the superconducting fluctuations may be either temporal or spatial. These observations highlight similarities between FeSe and underdoped cuprate superconductors.
pacs:
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††preprint: APS/123-QED
FeSe is considered to be an exceptional member 1; 2 of the family of iron (Fe)-based superconductors 3; 4; 5; 6; 7 for various reasons. First, FeSe is the structurally simplest of all members. It superconducts 8 below a critical temperature K and can be significantly enhanced in thin films 9; 10; 11; 12 and intercalated FeSe 13 or by pressure () 14; 15; 16; 17; 18; 19. Second, FeSe undergoes a structural transition 8; 20; 21 from a tetragonal to an orthorhombic state at K at ambient which was shown to be nematic 22; 23; 24; 25, i.e., driven by electronic degrees of freedom. In contrast to other Fe-based superconductors 26, the nematic transition in FeSe is not accompanied or closely followed by an antiferromagnetic transition 27; 21. Thus, it was suggested that FeSe represents an ideal platform to study a purely nematic phase and its interrelation with superconductivity 1. Third, FeSe was found to be characterized by strong electronic correlations 28 leading to a small Fermi energy 2 which is comparable in size to the superconducting gap. This has recently raised the question whether FeSe is located deep in the crossover regime between weak-coupling BCS to strong-coupling BEC superconductivity 29; 30; 31; 32; 33; 34. The latter is characterized by superconducting fluctuations over a wide temperature () range above .
The extent to which the properties of FeSe are comparable to those of other Fe-based superconductors has been strongly debated over the years 1. In this regard, the study of the - phase diagram (see Fig. 1 (a)) yielded important new insights 27; 35; 36; 37; 38; 39; 40; 41; 42; 43; 44; 45; 46; 47 (see Fig. S1). Above a characteristic pressure , bulk magnetic order 27; 43, which is likely stripe-type antiferromagnetic order 36; 48; 35, was observed at the magnetic transition temperature (i.e., the magnetic-nematic state). At even higher pressures, above a second characteristic pressure , the magnetic-nematic ground state was found to be stabilized through a simultaneous first-order transition with 35; 36; 44. This demonstrated that the phase diagram of FeSe at higher shows the same generic features in terms of the magnetic and structural transitions as other Fe-based superconductors, i.e., two subsequent, second-order phase transitions with that can be tuned to a simultaneous first-order transition () 35; 36; 44. However, whether the purely nematic state at low pressures fits into this universal picture, is still a subject of debates 49; 50; 51; 52; 53; 54; 55.
With respect to the superconductivity of FeSe under pressure, there is an ongoing discussion about its nature. It was proposed early on that superconductivity exists over a wide range, i.e., in the purely nematic (), but also in the magnetic-nematic range (). In the latter regime, the simultaneous enhancement of and raised the idea of cooperative promotion of superconductivity and magnetism 43; 56, contrary to other Fe-based superconductors. However, this scenario has not be substantiated to date, since microscopic probes, such as NMR 36, failed to detect any signature of superconductivity in the magnetic-nematic state for . This has therefore even led to the question whether bulk superconductivity exists in FeSe for 36; 57.
By studying the specific heat () under of a single crystal59 of FeSe up to 2.36 GPa, we determine the full thermodynamic - phase diagram of FeSe. We are therefore able to address various open issues related to superconductivity: our results confirm the bulk nature of superconductivity over the full range investigated, in particular also in the magnetic-nematic state for . In this regime, our data suggest a competition of superconductivity and magnetism in FeSe. Even further, we argue that superconducting and magnetic fluctuations of temporal and/or spatial nature exist in FeSe at high over a wide range of temperatures above the respective bulk transition temperatures. These results therefore put FeSe in close similarity to the strongly correlated cuprate superconductors.
The specific heat of a vapor grown FeSe single crystal 59 was measured with an ac-technique (see Fig. 1 (b)) inside a liquid-medium piston-cylinder pressure cell in a home-built setup 58 (for more details, see SI).
First, we focus on the data close to the structural and magnetic transitions at and , respectively, in FeSe under , as shown in Fig. 1 (b) and 2 (and in Figs. S2-S7) to determine the characteristic pressures and from our experiment. is monotonically suppressed with increasing until it becomes indiscernible above 1.32 GPa (see Figs. 1 (b) and S3). Magnetic ordering is observed in our data for GPa (see Fig. 2 (a) and Fig. S5 for low data). This therefore defines in the - phase diagram of FeSe (0.84 GPa0.91 GPa).
Upon increasing , first increases steeply up to 1.2 GPa, then shows a slight reduction up to 1.9 GPa and then increases quickly for higher pressures. At the same time, the specific heat anomaly at (see Fig. 2 (a)) evolves from a step-like shape, characteristic for second-order phase transitions at lower , to a symmetric peak at higher , which might be the result of a slightly broadened singularity of a first-order transition. This observation is therefore consistent with the picture 35; 36 that the magnetic transition becomes first order close to where it merges with the structural transition. To define the characteristic pressure at which the character of the magnetic transition changes, we follow three complimentary approaches. This includes measurements of the thermal hysteresis (see Fig. 2 (b) and Fig. S7) and an analysis of the asymmetry and the width of the specific heat peak (see Fig. 2 (c)). We define the asymmetry as , with ( and ) being the temperatures at which the specific heat anomaly exhibits its maximum value (50 of the maximum value) and the width as . All together, all three quantities exhibit a sudden change at GPa.
Next, we present in Fig. 3 the evolution of the specific heat jump across the superconducting transition at in the three distinct pressure regimes (a) , (b) and (c) (see Figs. S8 and S9 for raw data). At all up to 2.36 GPa, we resolve a clear specific heat anomaly at low , associated with the superconducting transition at . To determine and the superconducting jump size , we use an equal-area construction in (see dotted lines in inset of Fig. 3 (a)). For , we find an increase of together with an increase of (see Fig. 3 (a)). Soon after the onset of magnetism at , and are suppressed with for . Above , increases slowly, however, continues to be monotonically suppressed with increasing .
Remarkably, we also find a sudden change of the shape of the anomaly from almost mean-field-like at to a more -like shape with an extended high- tail at . This change can be quantified in terms of a broadening parameter (see Fig. S10) which defines the width of superconducting transition and is shown in Fig. 3 (d) (right axis): it is almost constant as a function of for , then exhibits a clear jump at (see also Fig. S11) and levels off again, until it increases rapidly for . We stress that such sudden changes in the broadening, as observed here at and again at , are unlikely to result from pressure inhomogeneities related to the freezing of the pressure medium 60, and therefore rather reflect a change of intrinsic physics of FeSe.
We can now proceed with discussing the two central results of this study. The first one relates to the question of bulk superconductivity in FeSe under and its relationship with magnetism. Here, the observation of a finite at all speaks in strong favor of bulk superconductivity in FeSe, which coexists with nematic order at low as well as with magnetic-nematic order at high . The fact that , which, in simple BCS theory, is a measure of the superconducting condensation energy, is strongly suppressed with for (see Fig. 3 (d)) indicates that magnetism competes with superconductivity in FeSe, resulting in either microscopic coexistence or in a macroscopic phase segregation 61. Importantly, competition is also the case for the region , even though and both increase with . This unusual possibility is included in an earlier model 62 on competing spin-density wave and superconducting order in itinerant systems, which provides the general tendency that competition leads to a decrease of (rather than a decrease of itself), when is increased. Our specific heat results of the bulk and values (see Figs. 4 and S1 (a)) indeed show that this is the case in FeSe at high : notably, is suppressed with decreasing (see Fig. 3 (e)). Therefore, our results strengthen the similarities of FeSe to other Fe-based superconductors 7; 63; 64; 65; 66; 67; 68; 69; 61.
The second result is summarized in the --phase diagram in Fig. 4 (a) (see Fig. S1 for simplified versions of this phase diagram). In this figure, we compare the transition temperatures , and from the present work (full symbols), with those reported in literature70, based on x-ray scattering 35; 45, NMR 37, resistance 38; 39; 40; 41, magnetization 41 and SR 43; 44 (open symbols). Surprisingly, whereas the majority of values and values for , as well as the values themselves, are rather consistent, the and values for show strong discrepancies. Given that specific heat measurements provide the bulk, thermodynamic (and static) transition temperatures, we suggest below one possible way to rationalize these findings is in terms of superconducting and magnetic fluctuations which exist for over a wide range above and , respectively.
In terms of superconductivity for , not only is the discrepancy of bulk values from the present study () and those from previous reports from transport and susceptibility (, Fig. 4 (a) and (b)) remarkable, but it must be recalled that there is a simultaneous, sudden change in the shape of the anomaly at , depicted in Fig. 3. A sudden increase in broadening of the feature at at was also observed in other quantities 41; 56, such as resistance, despite being much larger there. Contrary to changes in transport features, though, the observed change in the specific heat feature is considered as a well-established signature 71; 72; 73 of superconducting fluctuations 30 above the mean-field . In this situation, the onset of diamagnetism 72; 31 at is likely found at higher temperatures than the bulk , consistent with our results. Revisiting susceptibility data39; 41 demonstrates that the bulk actually corresponds to the temperature at which FeSe exhibits saturating diamagnetism (see Fig. 4 (b)). Thus, a comparison of onset and can be used to estimate the range in which superconducting fluctuations exist. This range is small, but present for and it increases rapidly above (10 K at 2.36 GPa, see Figs. 4, S1 and S13). This mirrors the observed broadening of the feature at . Taken together, all these observations are consistent with a picture, in which significant changes of the Fermi surface 38; 74; 75 at and increase the -range of fluctuations. Such extended fluctuations in the presence of competing magnetic order, suggested in the present work, might also naturally account for the absence of pronounced features at in microscopic NMR data 36 at .
Concerning the magnetic transition, we find that the values from are at the lower bound of values reported so far. It is remarkable, though, that similar values were inferred using the same technique in different studies (see, e.g., the two sets of open blue circles from resistance studies in Fig. 4). This argues against experimental artifacts arising from a combination of different samples with slightly different stochiometry and different pressure media being solely responsible for the discrepancy in values. Instead, it seems likely that the observed spread in is related to the time scale of each experiment, ranging from for SR 43; 44 up to for NMR 36; 37 up to static for and x-ray probes (measuring the increase of orthorhombicity associated with the development of long-range order 35). We refrain from including the values inferred from the resistance in the present discussion, as the associated time scale, given by the scattering time, cannot be unequivocally defined. As from the two static probes ( and x-ray) fall on top of each other (, see Fig. 4 (b) and S1 (b)) and at any given , this is highly suggestive of magnetic fluctuations existing far above the static . The extent in of these fluctuations above can be estimated from the spread of transition temperatures in Fig. 4. This spread increases upon increasing , even more rapidly above , and reaches more than K above 2 GPa. The width of the specific heat peak at (see Fig. 2 (c)) provides further support for this statement, as it shows a progressive increase above (see Fig. S12), which reflects a sizable loss of magnetic entropy preceding the bulk upon cooling.
Another scenario which could give rise to a similar phenomenology of the - phase diagram, as well as the specific heat features, invokes electronic inhomogeneity 76 giving rise to a spatially-fluctuating state. It is important to note though, that this inhomogeneity then must be intrinsically induced by the occurrence of magnetism, as evident from our phase diagram in Fig. 4. It could, e.g., arise from the formation of domains in the magnetically-ordered state which are pinned by extrinsic disorder, inevitable in any real crystal. Whereas such a scenario certainly promotes a non-bulk superconducting state above , causing zero resistance well above the bulk (such as the recently proposed fragile superconducting state 77), it unlikely explains the correlation of time scales and transition temperatures for the magnetic transition. Thus, whereas for the superconducting transition either temporal or spatial fluctuations are consistent with our data, the results speak in favor of a temporal nature of the magnetic fluctuations.
To verify which of these two scenarios is applicable in FeSe, it will be of crucial importance to identify the characteristic energy scales of the different orders in FeSe under pressure. One important key question here will be to resolve the magnetic structure of FeSe for which has still not been unequivocally determined to date. Nevertheless, we want to stress that our picture of the - phase diagram of FeSe presents close similarity to the ones of the high- cuprate superconductors 78. In the latter case, there is growing evidence for the coexistence of superconductivity in the underdoped regime with other competing phases, such as charge-density waves 79 enhancing fluctuations 80; 81 associated with both orders over a wide range above the respective bulk transition temperatures 78; 82. Whereas this comparison is purely phenomenological at present, FeSe might serve as an important reference system to investigate the origin of such extended fluctuating regimes in the presence of competing orders, as superconductivity can be tuned through non-magnetic and magnetic states solely via pressure which does not introduce any additional disorder.
In conclusion, the presented specific heat data demonstrate that superconductivity is bulk in FeSe up to 2.36 GPa, and competes with magnetism, whenever present. In the presence of magnetism, our results strongly suggest that superconducting and magnetic fluctuations exist over a wide temperature range above the respective bulk transition temperatures. This puts the phase diagram of FeSe under pressure in close similarity to those of underdoped cuprates in which the enhancement of phase fluctuations due to competing orders is considered as a key ingredient for high- superconductivity.
Acknowledgements.
We thank A. Kreyssig (Kreyßig), V. G. Kogan, D. Ryan and B. Andersen for useful discussions. In addition, we thank G. Drachuck for useful discussions and technical support with the ac specific heat setup in the initial stages of this work. Work at the Ames Laboratory was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division. The Ames Laboratory is operated for the U.S. Department of Energy by Iowa State University under Contract No. DEAC02-07CH11358.
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