Oscillations of magnetization in topological line-node semimetals

We theoretically investigate the phase of the de Haas–van Alphen oscillations in topological line-node semimetals. In these semimetals the chemical potential of charge carriers can essentially depend on the magnetic field, and this dependence changes the phase of the oscillations as compared to the...

Повний опис

Збережено в:
Бібліографічні деталі
Дата:2018
Автори: Mikitik, G.P., Sharlai, Yu.V.
Формат: Стаття
Мова:English
Опубліковано: Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України 2018
Назва видання:Физика низких температур
Теми:
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/176168
Теги: Додати тег
Немає тегів, Будьте першим, хто поставить тег для цього запису!
Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Oscillations of magnetization in topological line-node semimetals / G.P. Mikitik, Yu.V. Sharlai// Физика низких температур. — 2018. — Т. 44, № 6. — С. 727-733. — Бібліогр.: 45 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id irk-123456789-176168
record_format dspace
spelling irk-123456789-1761682021-02-04T01:30:31Z Oscillations of magnetization in topological line-node semimetals Mikitik, G.P. Sharlai, Yu.V. Специальный выпуск К 90-летию со дня рождения A.A. Абрикосова We theoretically investigate the phase of the de Haas–van Alphen oscillations in topological line-node semimetals. In these semimetals the chemical potential of charge carriers can essentially depend on the magnetic field, and this dependence changes the phase of the oscillations as compared to the phase in a three-dimensional metal with a band-contact line. Our results elucidate recent experimental data on the Berry phase for certain electron orbits in ZrSiS, ZrSiTe, and ZrSiSe. 2018 Article Oscillations of magnetization in topological line-node semimetals / G.P. Mikitik, Yu.V. Sharlai// Физика низких температур. — 2018. — Т. 44, № 6. — С. 727-733. — Бібліогр.: 45 назв. — англ. 0132-6414 PACS: 71.20.–b, 75.20.–g, 71.30.+h http://dspace.nbuv.gov.ua/handle/123456789/176168 en Физика низких температур Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
topic Специальный выпуск К 90-летию со дня рождения A.A. Абрикосова
Специальный выпуск К 90-летию со дня рождения A.A. Абрикосова
spellingShingle Специальный выпуск К 90-летию со дня рождения A.A. Абрикосова
Специальный выпуск К 90-летию со дня рождения A.A. Абрикосова
Mikitik, G.P.
Sharlai, Yu.V.
Oscillations of magnetization in topological line-node semimetals
Физика низких температур
description We theoretically investigate the phase of the de Haas–van Alphen oscillations in topological line-node semimetals. In these semimetals the chemical potential of charge carriers can essentially depend on the magnetic field, and this dependence changes the phase of the oscillations as compared to the phase in a three-dimensional metal with a band-contact line. Our results elucidate recent experimental data on the Berry phase for certain electron orbits in ZrSiS, ZrSiTe, and ZrSiSe.
format Article
author Mikitik, G.P.
Sharlai, Yu.V.
author_facet Mikitik, G.P.
Sharlai, Yu.V.
author_sort Mikitik, G.P.
title Oscillations of magnetization in topological line-node semimetals
title_short Oscillations of magnetization in topological line-node semimetals
title_full Oscillations of magnetization in topological line-node semimetals
title_fullStr Oscillations of magnetization in topological line-node semimetals
title_full_unstemmed Oscillations of magnetization in topological line-node semimetals
title_sort oscillations of magnetization in topological line-node semimetals
publisher Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
publishDate 2018
topic_facet Специальный выпуск К 90-летию со дня рождения A.A. Абрикосова
url http://dspace.nbuv.gov.ua/handle/123456789/176168
citation_txt Oscillations of magnetization in topological line-node semimetals / G.P. Mikitik, Yu.V. Sharlai// Физика низких температур. — 2018. — Т. 44, № 6. — С. 727-733. — Бібліогр.: 45 назв. — англ.
series Физика низких температур
work_keys_str_mv AT mikitikgp oscillationsofmagnetizationintopologicallinenodesemimetals
AT sharlaiyuv oscillationsofmagnetizationintopologicallinenodesemimetals
first_indexed 2025-07-15T13:50:45Z
last_indexed 2025-07-15T13:50:45Z
_version_ 1837721139854442496
fulltext Low Temperature Physics/Fizika Nizkikh Temperatur, 2018, v. 44, No. 6, pp. 727–733 Oscillations of magnetization in topological line-node semimetals G.P. Mikitik and Yu.V. Sharlai B. Verkin Institute for Low Temperature Physics and Engineering of the National Academy of Sciences of Ukraine 47 Nauky Ave., Kharkiv 61103, Ukraine E-mail: mikitik@ilt.kharkov.ua Received December 26, 2017, published online April 25, 2018 We theoretically investigate the phase of the de Haas–van Alphen oscillations in topological line-node semi- metals. In these semimetals the chemical potential of charge carriers can essentially depend on the magnetic field, and this dependence changes the phase of the oscillations as compared to the phase in a three-dimensional metal with a band-contact line. Our results elucidate recent experimental data on the Berry phase for certain elec- tron orbits in ZrSiS, ZrSiTe, and ZrSiSe. PACS: 71.20.–b Electron density of states and band structure of crystalline solids; 75.20.–g Diamagnetism, paramagnetism, and superparamagnetism; 71.30.+h Metal-insulator transitions and other electronic transitions. Keywords: topological line-node semimetals, de Haas–van Alphen oscillations. 1. Introduction In recent years much attention has been given to the topological line-node semimetals in which the conduction and valence bands touch along lines in the Brillouin zone and disperse linearly in directions perpendicular to these lines [1–16]. It is necessary to emphasize that the contact of the electron energy bands along the lines is the widespread phenomenon in crystals [7,17–19]. For example, such con- tacts of the bands occur even in many simple metals, and graphite [20], beryllium [21], aluminium [22], LaRhIn5 [23] are among them. However, the degeneracy energy of the bands, dε , is not constant along such lines, and this energy dε varies in the interval from its minimum minε to its max- imum maxε values. A crystal with the band-contact line can be named the topological semimetal if the difference max min 2ε − ε ≡ ∆ is sufficiently small and if the chemical potential ζ of the electrons does not lie far away from the mean energy 0 max min( ) / 2dε ≡ ε + ε of the line. Rhombohedral graphite [3,24,25], Ca3P2 [6] and CaAgP [9], Cu3NZn and Cu3NPd [7,8], ZrSiS [11,12,16], ZrSiTe [13], alkaline-earth germanides and silicides [14], PbTaSe2 [15] are examples of the line-node semimetals. The magnetization of electrons in a crystal with the band-contact line characterized by large ∆ was theoretical- ly investigated many years ago [26,27], and it was found that the magnetic susceptibility of the electrons exhibits a giant anomaly when ζ approaches one of the energies minε or maxε which correspond to the points of the electron topo- logical transitions of 3½ kind [18]. In the topological sem- imetals the interval 2∆ is small, the critical energies minε and maxε are close to each other, and the character of the anomaly in the susceptibility changes. The magnetic sus- ceptibility in the case of the line-node semimetals was con- sidered for weak magnetic fields in Ref. 28 and for arbi- trary magnetic fields in Refs. 29, 30. It is well known [31,32] that at low temperatures the magnetization of electrons in metals exhibits the de Haas– van Alphen oscillations. These oscillations are described by a periodic function of ex / ( ) 2cS e H − πγ where exS is the extremal cross-section area of the Fermi surface, and γ is the constant in the semiclassical quantization rule. This γ is expressed in terms of the Berry phase BΦ for the elec- tron orbit in the extremal cross section (see Eq. (5) below). The characteristic feature of the topological line-node sem- imetals is that the de Haas–van Alphen oscillations are shifted in phase [30] as compared to the case of metals for which the band-contact lines are absent, and = 0BΦ , = 1/ 2γ . The shift is due to the Berry phase π for electron orbits surrounding the band-contact line [33]. Recently, the de Haas–van Alphen [34,35], Shubnikov–de Haas [36–39], and thermoelectric power [40] oscillations in magnetic fields were experimentally investigated in the line-node semimetals ZrSiS, ZrSiTe, and ZrSiSe, and intermediate © G.P. Mikitik and Yu.V. Sharlai, 2018 G.P. Mikitik and Yu.V. Sharlai values of the Berry phase (other than 0 and π) were ob- tained for a number of the electron orbits. In this paper we suggest an explanation of these unusual values of BΦ de- tected in the experiments. Our explanation is based on the following considerations: Due to small values of ∆, the dispersion relation for the elec- trons near the band-contact line is similar to the dispersion relation in layered metals [30]. It is known [41–44] that in such metals placed in the magnetic field H a crossover from the three-dimensional electron spectrum to the quasi-two- dimensional one occurs with increasing H . In the case of the quasi-two-dimensional spectrum a dependence of the chemical potential on the magnetic field is strong [32], and this dependence changes the phase shift of the oscillations. We show that in the crossover region of the magnetic fields and in the region of the quasi-two-dimensional spectrum the shift can differ from π and 0, simulating the case of the Ber- ry phase deviating from these values. 2. Formulas for magnetization To clarify the essence of the matter, we consider the sim- plest band-contact line, assuming that it has the shape of a straight line in the quasi-momentum space p, and that the electron dispersion relation in the vicinity of the contact line of the two bands “c” and “v” has the form: , 3 , 2 2 2 , 11 1 22 2 = ( ) , = , c v d c v c v p E E b p b p ε ε ± + (1) where the 3p axis coincides with the line; 3( )d pε de- scribes a dependence of the degeneracy energy along the line (the maxε and minε mentioned above are the maximum and minimum values of the function 3( )d pε ); 11b and 22b are positive constants specifying the Dirac spectrum in the directions perpendicular to the line. Below we also use the simplest approximation for the periodic function 3( )d pε , 3 3 3 2 ( ) = cos = cos ,d p p d p L π   ε ∆ ∆        (2) where = 2 /L dπ is the length of the line in the Brillouin zone, and d is the appropriate size of the unit cell of the crys- tal. Besides, we neglect the electron spin (but take into ac- count the two-fold degeneracy of the electron energy bands in spin in the formulas below), and consider the case of the zero temperature T and of the magnetic field H parallel to the line. The Fermi surface corresponding to the dispersion rela- tion (2) is a corrugated cylinder when the chemical potential ζ lies outside the interval from minε to maxε . If ζ is inside the interval, the Fermi surface has a self-intersecting shape, and at min=ζ ε or maxε the electron topological transitions of 3½ kind occur [18]. If the magnetic field H is directed along the line, the electron spectrum corresponding to the Hamiltonian (1) has the form [27]: 1/2 , 3 3( ) = ( ) ,l c v d e Hp p l c α ε ε ±     1/2 3 11 22= ( ) = 2( )p b bα α , (3) where l is a non-negative integer ( = 0l , 1,…), with the single Landau subband = 0l being shared between the branches “c” and “v”. Interestingly, even for 1l  , the spectrum (3) exactly coincides with that obtained from the semiclassical quantization rule, 3 2( , ) = ( ),l e HS p l c π ε + γ  (4) where 2 3 3( , ) = 2 [ ( )] /dS p pε π ε − ε α is the area of the cross section of the isoenergetic surface by the plane per- pendicular to the magnetic field and passing through the point with the coordinate 3p , the constant γ is expressed in term of the Berry phase BΦ for the appropriate electron orbit [33]: 1= , 2 2 BΦ γ − π (5) and =BΦ π in our case of the orbit surrounding the band- contact line. The magnetization of electrons in a line-node semimetal was calculated in Ref. 30 at an arbitrary shape of its band- contact line. Using this result, we obtain the following ex- pressions for the magnetization 3M directed along the band-contact line being considered: 3/2 1/2 1/2 3 32 0 1( , ) ( ), 2 LeM H H dp K u c  ζ = α   π ∫  (6) where the integration is carried out over this line; 3 1 1( ) = ( ,[ ] 1) ([ ] ), 2 2 2 K u u u uζ − + + + (7) ( , )s aζ is the Hurwitz zeta function, 2 3 3[ ( )] ( , ) = = , 2 d p c cS p u e H e H ζ − ε ζ α π  (8) and [ ]u is the integer part of u . In the topological semimetals, charge carriers (electron and holes) are located near the band-contact line, and their chemical potential ζ generally depends on the magnetic field, = ( )Hζ ζ . This dependence can be derived from the condition that the charge-carrier density ( , )n Hζ does not vary with increasing H , 0 0( , ) = ( ),n H nζ ζ (9) where 0n and 0ζ are the density and the chemical potential at = 0H . At = 0T the densities 0 0( )n ζ and ( , )n Hζ are described by the following expressions [30]: 728 Low Temperature Physics/Fizika Nizkikh Temperatur, 2018, v. 44, No. 6 Oscillations of magnetization in topological line-node semimetals 2 0 0 3 0 3 0 32 3 0 1( ) = ( ( )) ( ( )), 2 L d dn dp p pζ ζ − ε σ ζ − ε π α ∫ (10) 3 32 2 0 1( , ) = ( [ ]) ( ( )), 22 L d eHn H dp u p c ζ + σ ζ − ε π ∫  (11) where ( ) = 1xσ if > 0x , and 1− if < 0x . On calculating ( )Hζ with Eqs. (9)–(11), one can find the magnetization as a function of 0n or 0ζ , inserting ( )Hζ into Eqs. (6)–(8). In analyzing the effect of ( )Hζ on the phase of the de Haas–van Alphen oscillations, we shall plot the so-called Landau-level fan diagrams [32] commonly used in treat- ments of the experimental data. At = 0T the periodic in 1/ H magnetization of electrons in metals exhibits singu- larities (sharp maxima or minima [45]) when the lower or upper edge of the lth Landau subband crosses the Fermi level ζ . In the semiclassical limit ( 1l  ) and under the assumption that ζ is independent of H , such crossings occur at the magnetic fields lH determined by Eq. (4): ex 1 2= ( ), ( )l e l H cS π + γ ζ  where ex ( )S ζ is the minimum or maximum value of 3( , )S pζ with respect to 3p . Thus, if the positions lH of the singularities are known, the constant γ can be found with the Landau-level fan diagram: Plotting the Landau- level index l versus 1/ lH and continuing the obtained straight line up to the intersection of this line with the l axis in which (1/ ) = 0lH , the coordinate −γ of the inter- section enables one to obtain γ : =γ γ. It is important to emphasize that if ζ lies in the energy region where the Dirac spectrum occurs, one can use lH with 1l  in the construction of the fan diagrams since, as was mentioned above, the semiclassical spectrum resulting from formu- la (4) coincides with the exact one given by Eq. (3) even at small l. Note also that this procedure of determining γ , which characterizes the phase of the de Haas–van Alphen oscillations, is applicable to the case when ζ depends on H , but as shall be demonstrated below, γ thus extracted does not generally coincide with the constant γ specifying the semiclassical quantization rule. 3. Discussion The quantity u defined by Eq. (8) changes along the nodal line between its minimal minu and maximal maxu values which correspond to the minimal minS and maximal maxS values of 3( , )S pζ with respect to 3p . In the case of sufficiently weak magnetic fields when minu , maxu , max min 1u u−  , i.e., when max min max min 2 , , ,e H S S S S c π −   (12) the Landau subbands , 3( )l c v pε with different l overlap as in three-dimensional metals. According to Ref. 30, in this case formula (6) reduces to the well-known expression [32,42,44] describing the de Haas–van Alphen oscillations in a three-dimensional metal but with = 0γ . For 3( )d pε given by Eq. (2), this expression is a superposi- tion of two periodic functions determined by the two extremal cross-section areas min 3= ( , = 0)S S pζ and max =S 3( , = / 2)S p L= ζ . The dependence ( )Hζ is suffi- ciently weak in this three-dimensional case and practically has no effect on the oscillations [32]. Consider now stronger magnetic fields than in the case of inequalities (12). If | |ζ ∆ , the difference max minu u− be- comes less than unity when minu and maxu are still large. In this situation, the spectrum (2) transforms into the spectrum of a quasi-two-dimensional electron system since the differ- ent Landau subbands , 3( )l c v pε do not overlap, and they look like broadened Landau levels for which the spacing between the nearest Landau subbands in the vicinity of the Fermi level is larger than their width 2∆. At max min 1u u−  , the quantity u is practically independent of 3p running the line, 3( , ) ( )S p Sζ ≈ ζ , the corrugation of the Fermi surface be- comes unimportant, and formula (6) is simplified as follows: 3/2 1/2 1/2 3 1/2 1( , ) ( ),eM H H K u cd  ζ ≈ α   π  (13) where 2 ( )= , 2 c cSu e H e H ζ ζ ≈ α π  (14) and the function ( )K u at large u has the form [30]: =1 sin(2 )( ) ( [ ] 0.5) = . 2 2 l u u luK u u u l ∞ π ≈ − − − π ∑ (15) Equations (13)–(15) describe saw-tooth oscillations of 3M with changing 1/ H , and they coincide with the appro- priate expression [42–44] for a two-dimensional metal with the Dirac spectrum. A refined analysis of Eq. (6) at | |ζ ∆ and maxu , min 1u  gives 2 2 3 02 =1 | | 1 ( )sin 2 4 , 2 l e c cM l J l l e H e Hcd ∞  ζ ζ +∆ ζ∆ ≈− π π    α α π   ∑    (16) where 0 ( )J x is the Bessel function for which one has 0 ( ) 1J x ≈ at 1x and 1/2 0 ( ) (2 / ) cos( / 4)J x x x≈ π − π at 1x . Formula (16) agrees with the appropriate expression of Refs. 42, 44 and reproduces both Eqs. (13)–(15) at max min = 4 / 1u u c e H− ζ∆ α  and the formula for the de Haas–van Alphen oscillations in three-dimensional metals with = 0γ at max min 1u u−  . The crossover from the three-dimensional electron spec- trum to the quasi-two-dimensional one occurs at the magnet- ic field crH defined by the condition max min 1u u−  , Low Temperature Physics/Fizika Nizkikh Temperatur, 2018, v. 44, No. 6 729 G.P. Mikitik and Yu.V. Sharlai max min cr ( ) 4 | |= . 2 c S S cH e e − ζ ∆ π α    (17) For crH H , the spacing H∆ε between the Landau subbands in the vicinity of the Fermi level becomes compa- rable with their width 2∆. Thus, the quasi-two-dimensional regime of the oscillations takes place in the interval of the magnetic fields cr 1< <H H H where 1H is the field of the ultra-quantum limit, 2 1 ( ) = , 2 cS cH e e ζ ζ π α    (18) at which H∆ε reaches ζ , and the oscillations of the magnet- ization disappears. When H changes in this interval, the chemical potential ( )Hζ moves together with one of the Landau subbands, and then, at a certain value of H , it jumps from this subband to the neighboring one [32], Fig. 1. This strong dependence ( )Hζ noticeably changes the shape of the de Haas–van Alphen oscillations and can mask the cor- rect values of γ (and of the Berry phase) when γ is found with the Landau-level fan diagram. Indeed, the jumps can occur at the fields lH for which ( )n ζ in Eq. (11) becomes independent of ζ . This situation is realized when [ ]u in the right-hand side of Eq. (11) is one and the same integer along the whole line. Let us denote this integer as ( 1)l − . Then, Eq. (9) takes the form: 2 2 0 0 1 1= . 22 ( )l eL l H cn  −   π ζ (19) These lH also mark the singularities in the magnetization since immediately above and below lH the edges of the Landau subband touch the chemical potential, Fig. 1. It fol- lows from equation (19) that the dependence of 1/ lH on l is a straight line that intersects the l axis at = = 1/ 2l −γ , i.e., the Landau-level fan diagram plotted with the fields lH looks like in the case when = 1/ 2γ and the Berry phase BΦ is equal to zero. (The value of γ is defined up to an integer, and so = 1/ 2γ − and = 1/ 2γ are equivalent.) However, in reality one has =BΦ π , = 0γ , and the phase shift γ extract- ed from the oscillations in the quasi-two-dimensional regime does not permit one to find BΦ since γ ≠ γ now. The fore- going considerations are illustrated in Fig. 1 for which 0 / = 20ζ ∆ and max 0 cr 1 cr( ) / (2 ) / 5cS e H H Hζ π    . Consider now the case when ζ is of the order of ∆. In this situation 1 crH H , and the crossover occurs near the ultra- quantum limit. Since, as was explained above, we have = 0γ and 1/ 2− in the three-dimensional and in the quasi-two- dimensional regimes of the oscillations, respectively, one may expect that γ takes intermediate values if this quantity is found in the crossover region. In Fig. 2 we show the de Haas– van Alphen oscillations of 3M calculated with Eq. (6) at 0 / = 3ζ ∆ when max 0 cr 1 cr( ) / (2 ) / 1cS e H H Hζ π    . In this situation we find = 0.23 0.04γ − ± if the H -dependence of ζ is taken into account. Note that a relatively small con- tribution of the minimal cross section min max= / 4S S into the oscillations is also visible in the figure. This minimal cross section slightly affects the maxima in 3M associated with maxS , and so we find = 0.02 0.01γ ± even for the oscil- lations calculated at fixed 0=ζ ζ . In Fig. 3 we present the dependence of γ on 0ζ . In the construction of this figure, values of γ have been obtained, using the first four sharp maxima in the calculated functions 3(1/ )M H . The small jump in γ at 0 / 15ζ ∆ ≈ is due to that at 0 / > 15ζ ∆ all the four maxima in 3M are determined by the jumps in ζ , whereas at 0 / < 15ζ ∆ the chemical potential is continues for a part of these maxima, cf. Figs. 1 and 2. At 0 / 1ζ ∆ ≈ the jumps in ζ disappear completely. For 0 / < 3ζ ∆ one has max min/ > 4S S , i.e., the ratio of the oscillation Fig. 1. (a) The magnetization 3M , Eq. (6), versus 1 / H at fixed chemical potential 0= = 20ζ ζ ∆ (the dashed line) and at ( )Hζ shown in the lower panel (the solid line). Here max 0( ) =S ζ 2 02 ( ) /= π ζ + ∆ α , and max 0 cr( ) / (2 ) 5cS e Hζ π   . The inset depicts the Landau-level indexes l versus max 0( ) / (2 )lcS e Hζ π  ; 1 / lH are the positions of the maxima of the functions 3(1 / )M H shown by the solid and dashed curves in the main plot. (b) The dependence of ζ on 1 / H calculated with Eqs. (9)–(11) at 0 = 20ζ ∆ . We also mark the Landau subbands by the dark back- ground, and the short and long dashes indicate the lower and the upper edges of these subbands, respectively. 730 Low Temperature Physics/Fizika Nizkikh Temperatur, 2018, v. 44, No. 6 Oscillations of magnetization in topological line-node semimetals periods corresponding to the minimal and maximal cross sections is larger than 4, and the effect of the low-frequency oscillations on the first four peaks in 3M decreases. For this reason the break appears in the dependence 0( )γ ζ at 0 / 3ζ ∆ ≈ . In other words, this break as well as the jump at 0 / 15ζ ∆ ≈ are caused by the relatively small number of the peaks in 3M used in our plotting the Landau-level fan dia- grams. Consider now the situation when apart from the charge carriers located near the nodal line under study, there is an additional electron group in the semimetal. In particular, this situation occurs in ZrSiS. For simplicity, we shall ne- glect the quantization of electron energy in the magnetic fields for the charge carriers of this additional group. Note that this simplifying assumption is easily realized even at low temperatures if the cyclotron mass of these carries is essentially larger than the cyclotron mass of electrons near the nodal line. Then, with the additional electron group, equation (9) is modified as follows: 0 0 0 0 0 ( ) ( , ) ( ) = ( ), dN n H n d ζ ζ + ζ − ζ ζ ζ (20) where 0 0( ) /dN dζ ζ is the density of the electron states of the additional group at the Fermi level. We shall specify this density of the states by the formula 0 0 0 0 0 ( ) ( ) = , dN n d ζ ζ λ ζ ζ (21) where λ is the dimensionless parameter. If 0,λ → we return to the case of the single electron group located near the nod- al line. As was shown above, in this case one always has = 1/ 2γ − for the oscillations in the quasi-two-dimensional regime. If 1,λ we arrive at the case of the constant chem- ical potential which is stabilized by the large additional elec- tron group. In this case = = 0γ γ in the quasi-two- dimensional regime. Hence, it is reasonable to expect that γ will take intermediate values if 1.λ  In Fig. 4, we show the oscillation of 3M in the quasi-two-dimensional regime for three values of the parameter = 0,λ 1, ∞. It is seen that the phase of the oscillations at = 1λ indeed has a value which lies between the values corresponding to the other two cases. Thus, the intermediate values of γ can be found not only in the crossover region but also in the quasi-two-dimensional regime of the oscillations if there is an addition group of charge carriers in the semimetal. 4. Conclusions We theoretically investigate the phase of the de Haas– van Alphen oscillations in topological line-node semimetals, using the simple model for their nodal lines, Eqs. (1) and (2). There are two regimes of the oscillations. These regimes are determined by the relation between spacing H∆ε separating the Landau subbands in the vicinity of the Fermi level and the width of these subbands, 2∆, resulting from the disper- sion of the degeneracy energy along the nodal line. Fig. 2. (a) The magnetization 3M , Eq. (6), versus 1 / H at fixed chemical potential 0= = 3ζ ζ ∆ (the dashed line) and at ( )Hζ shown in the lower panel (the solid line). Here max 0( ) /cS ζ cr/(2 ) 1e Hπ   . (b) The dependence of ζ on 1 / H calculated with Eqs. (9)–(11) at 0 = 3ζ ∆ . All the notations and the inset are similar to Fig. 1. The intercept of the solid straight line in the inset gives = 0.23 0.04−γ ± . Fig. 3. Dependence of γ on 0ζ . The values of γ have been found with the Landau-level fan diagrams plotted using the first four sharp peaks in the functions 3(1 / ).M H Low Temperature Physics/Fizika Nizkikh Temperatur, 2018, v. 44, No. 6 731 G.P. Mikitik and Yu.V. Sharlai For not-too-strong magnetic fields when 2H∆ε ∆ , the three-dimensional regime of the oscillations occurs, the de- pendence of the chemical potential ζ on the magnetic field H is weak, and the constant γ defining the phase of the oscilla- tions coincides with the constant γ in the semiclassical quan- tization rule, i.e., =γ γ . Since the Berry phase =BΦ π and, according to Eq. (5), = 0γ for the electron orbits surrounding the nodal lines, one can detect these lines, measuring the phase of the de Haas–van Alphen oscillations in this case. With increasing magnetic fields, the spacing between the Landau subband becomes larger than 2∆, and the quasi-two- dimensional regime of the oscillations takes place. In this regime the dependence of ζ on H is strong. This depend- ence changes the shape and the phase of the oscillations, and γ ≠ γ in this regime. At low temperatures ( )HT ∆ε we find that | |= 1/ 2γ for the extremal cross sections for which = 0γ . Thus, the results of the phase measurements will imi- tate the case = 1/ 2γ and will not permit one to find the true values of γ and of the Berry phase. Due to the experimental data of Refs. 34–40, the special attention in our paper is given to the situations in which val- ues of | |γ can be intermediate between 0 and 1/2. We show that these situations can occur in the region of the magnetic fields where the crossover from the three-dimensional re- gime to the quasi-two-dimensional one takes place, and in the quasi-two-dimensional regime if there is an additional group of charge carriers in the semimetal. In these cases, measurements of γ (the phase of the oscillations) provide information on the electron energy spectrum of the semi- metal, see Fig. 3, rather than on the Berry phase of the elec- tron orbits. ________ 1. T.T. Heikkilä and G.E. Volovik, JETP Lett. 93, 59 (2011). 2. A.A. Burkov, M.D. Hook, and L. Balents, Phys. Rev. B 84, 235126 (2011). 3. D. Pierucci, H. Sediri, M. Hajlaoui, J.-C. Girard, T. Brumme, M. Calandra, E. Velez-Fort, G. Patriarche, M.G. Silly, G. Ferro, V. Soulière, M. Marangolo, F. Sirotti, F. Mauri, and A. Ouerghi, ACS Nano 9, 5432 (2015). 4. H. Weng, Y. Liang, Q. Xu, R. Yu, Z. Fang, X. Dai, and Y. Kawazoe, Phys. Rev. B 92, 045108 (2015). 5. K. Mullen, B. Uchoa, and D.T. Glatzhofer, Phys. Rev. Lett. 115, 026403 (2015). 6. L. S. Xie, L. M. Schoop, E. M. Seibel, Q. D. Gibson, W. Xie, and R. J. Cava, APL Mater. 3, 083602 (2015). 7. Y. Kim, B.J. Wieder, C.L. Kane and A.M. Rappe, Phys. Rev. Lett. 115, 036806 (2015). 8. R. Yu, H. Weng, Z. Fang, X. Dai, and X. Hu, Phys. Rev. Lett. 115, 036807 (2015). 9. A. Yamakage, Y. Yamakawa, Y. Tanaka, and Y. Okamoto, J. Phys. Soc. Jpn. 85, 013708 (2016). 10. M. Phillips and V. Aji, Phys. Rev. B 90, 115111 (2014). 11. L.M. Schoop, M.N. Ali, C. Straßer, V. Duppel, S.S.P. Parkin, B.V. Lotsch, and C.R. Ast, Nature Commun. 7, 11696 (2016). 12. M. Neupane, I. Belopolski, M.M. Hosen, D.S. Sanchez, R. Sankar, M. Szlawska, S.-Y. Xu, K. Dimitri, N. Dhakal, P. Maldonado, P.M. Oppeneer, D. Kaczorowski, F. Chou, M.Z. Hasan, and T. Durakiewicz, Phys. Rev. B 93, 201104(R) (2016). 13. A. Topp, J.M. Lippmann, A. Varykhalov, V. Duppel, B.V. Lotsch, C.R. Ast, and L.M. Schoop, New J. Phys. 18, 125014 (2016). 14. H. Huang, J. Liu, D. Vanderbilt, and W. Duan, Phys. Rev. B 93, 201114(R) (2016). 15. G. Bian, T-R. Chang, R. Sankar, S.-Y. Xu, H. Zheng, T. Neupert, C.-K. Chiu, S.-M. Huang, G. Chang, I. Belopolski, D.S. Sanchez, M. Neupane, N. Alidoust, C. Liu, B. Wang, C.-C. Lee, H.-T. Jeng, C. Zhang, Z. Yuan, S. Jia, A. Bansil, F. Chou, H. Lin, and M.Z. Hasan, Nature Commun. 7, 10556 (2016). 16. Y. Chen, Y.-M. Lu, and H.-Y. Kee, Nature Commun. 6, 6593 (2015). 17. C. Herring, Phys. Rev. 52, 365 (1937). 18. G.P. Mikitik and Yu.V. Sharlai, Phys. Rev. B 90, 155122 (2014). 19. C. Fang, Y. Chen, H.-Y. Kee, and L. Fu, Phys. Rev. B 92, 081201(R) (2015). 20. G.P. Mikitik and Yu.V. Sharlai, Phys. Rev. B 73, 235112 (2006). 21. G.P. Mikitik and Yu.V. Sharlai, Fiz. Nizk. Temp. 41, 1279 (2015) [Low Temp. Phys. 41, 996 (2015)]. 22. F. Szmulowicz, Solid State Comm. 148, 410 (2008). 23. G.P. Mikitik and Yu.V. Sharlai, Phys. Rev. Lett. 93, 106403 (2004). 24. J.W. McClure, Carbon 7, 425 (1969). 25. N.B. Kopnin and T.T. Heikkilä, Surface Superconductivity in Rhombohedral Graphite, Ch. 9 in Carbon-based Superconductors: Towards High-Tc Superconductivity, Junji Haruyama, Pan Stanford (2014), see also arXiv: 1210.7075. Fig. 4. The magnetization 3M , Eq. (6), versus 1 / H at fixed chemi- cal potential 0= = 400ζ ζ ∆ (the dashed line), at ( )Hζ calculated with Eqs. (9)–(11) for 0 = 400ζ ∆ (the solid line), and at ( )Hζ calcu- lated with Eqs. (10), (11), (20), and (21) for 0 = 400ζ ∆ and = 1λ (the dotted line). Here max 0 cr( ) / (2 ) 100cS e Hζ π   . All the nota- tions are similar to Fig. 1. The Landau-level fan diagram plotted using the sharp maxima of the dotted line in the interval between max 0( ) / (2 ) = 20cS e Hζ π  and 40 gives = 0.33 0.04.γ − ± 732 Low Temperature Physics/Fizika Nizkikh Temperatur, 2018, v. 44, No. 6 https://doi.org/10.1134/S002136401102007X https://doi.org/10.1103/PhysRevB.84.235126 https://doi.org/10.1021/acsnano.5b01239 https://doi.org/10.1103/PhysRevB.92.045108 https://doi.org/10.1103/PhysRevLett.115.026403 https://doi.org/10.1063/1.4926545 https://doi.org/10.1103/PhysRevLett.115.036806 https://doi.org/10.1103/PhysRevLett.115.036806 https://doi.org/10.1103/PhysRevLett.115.036807 https://doi.org/10.7566/JPSJ.85.013708 https://doi.org/10.1103/PhysRevB.90.115111 https://doi.org/10.1038/ncomms11696 https://doi.org/10.1103/PhysRevB.93.201104 https://doi.org/10.1088/1367-2630/aa4f65 https://doi.org/10.1103/PhysRevB.93.201114 https://doi.org/10.1038/ncomms10556 https://doi.org/10.1038/ncomms7593 https://doi.org/10.1103/PhysRev.52.365 https://doi.org/10.1103/PhysRevB.90.155122 https://doi.org/10.1103/PhysRevB.92.081201 https://doi.org/10.1103/PhysRevB.73.235112 https://doi.org/10.1063/1.4938520 https://doi.org/10.1016/j.ssc.2008.09.028 https://doi.org/10.1103/PhysRevLett.93.106403 https://doi.org/10.1016/0008-6223(69)90073-6 Oscillations of magnetization in topological line-node semimetals 26. G.P. Mikitik and I.V. Svechkarev, Fiz. Nizk. Temp. 15, 295 (1989) [Sov. J. Low Temp. Phys. 15, 165 (1989)]. 27. G.P. Mikitik and Yu.V. Sharlai, Fiz. Nizk. Temp. 22, 762 (1996) [Low Temp. Phys. 22, 585 (1996)]. 28. M. Koshino and I.F. Hizbullah, Phys. Rev. B 93, 045201 (2016). 29. G.P. Mikitik and Yu.V. Sharlai, Phys. Rev. B 94, 195123 (2016). 30. G.P. Mikitik and Yu.V. Sharlai, Phys. Rev. B 97, 085122 (2018). 31. A.A. Abrikosov, Fundamentals of the Theory of Metals, North Holland, Amsterdam (1988). 32. D. Shoenberg, Magnetic Oscillations in Metals, Cambridge University Press, Cambridge, England (1984). 33. G.P. Mikitik and Yu.V. Sharlai, Phys. Rev. Lett. 82, 2147 (1999). 34. J. Hu, Z. Tang, J. Liu, X. Liu, Y. Zhu, D. Graf, K. Myhro, S. Tran, C.N. Lau, J. Wei, and Z. Mao, Phys. Rev. Lett. 117, 016602 (2016). 35. J. Hu, Z. Tang, J. Liu, Y. Zhu, J. Wei, and Z. Mao, Phys. Rev. B 96, 045127 (2017). 36. M.N. Ali, L.M. Schoop, C. Garg, J.M. Lippmann, E. Lara, B. Lotsch, and S.S.P. Parkin, Sci. Adv. 2, e1601742 (2016). 37. X. Wang, X. Pan, M. Gao, J. Yu, J. Jiang, J. Zhang, H. Zuo, M. Zhang, Z. Wei, W. Niu, Z. Xia, X. Wan, Y. Chen, F. Song, Y. Xu, B. Wang, G. Wang, and R. Zhang, Adv. Electron. Mater. 2, 1600228 (2016). 38. S. Pezzini, M.R. van Delft, L. Schoop, B. Lotsch, A. Carrington, M.I. Katsnelson, N.E. Hussey, and S. Wiedmann, Nat. Phys. 14, 178 (2018). 39. R. Singha, A.K. Pariari, B. Satpati, and P. Mandal, PNAS 114, 2468 (2017). 40. M. Matusiak, J.R. Cooper, and D. Kaczorowski, Nature Commun. 8, 15219 (2017). 41. T. Champel and V.P. Mineev, Philos. Mag. B 81, 55 (2001). 42. I.A. Luk'yanchuk and Y. Kopelevich, Phys. Rev. Lett. 93, 166402 (2004). 43. I.A. Luk'yanchuk, Fiz. Nizk. Temp. 37, 56 (2011) [Low Temp. Phys. 37, 45 (2011)]. 44. V.P. Gusynin, V.M. Loktev, I.A. Luk'yanchuk, S.G. Sharapov, and A.A. Varlamov, Fiz. Nizk. Temp. 40, 355 (2014) [Low Temp. Phys. 40, 270 (2014)]. 45. G.P. Mikitik and Yu.V. Sharlai, Fiz. Nizk. Temp. 33, 586 (2007) [Low Temp. Phys. 33, 439 (2007)]. ___________________________ Low Temperature Physics/Fizika Nizkikh Temperatur, 2018, v. 44, No. 6 733 https://doi.org/10.1103/PhysRevB.93.045201 https://doi.org/10.1103/PhysRevB.94.195123 https://doi.org/10.1103/PhysRevB.97.085122 https://doi.org/10.1017/CBO9780511897870 https://doi.org/10.1103/PhysRevLett.82.2147 https://doi.org/10.1103/PhysRevLett.117.016602 https://doi.org/10.1103/PhysRevB.96.045127 https://doi.org/10.1103/PhysRevB.96.045127 https://doi.org/10.1126/sciadv.1601742 https://doi.org/10.1002/aelm.201600228 https://doi.org/10.1038/nphys4306 https://doi.org/10.1073/pnas.1618004114 https://doi.org/10.1038/ncomms15219 https://doi.org/10.1038/ncomms15219 https://doi.org/10.1080/13642810108216525 https://doi.org/10.1103/PhysRevLett.93.166402 https://doi.org/10.1063/1.3551529 https://doi.org/10.1063/1.3551529 https://doi.org/10.1063/1.4869583 https://doi.org/10.1063/1.4869583 https://doi.org/10.1063/1.2737555 1. Introduction 2. Formulas for magnetization 3. Discussion 4. Conclusions