Introduction

Metal extrusion processes provide most of the semi-finished bar, wire, and tubes for various applications.1 Friction stir extrusion (FSE) is an emerging extrusion process, initially developed by TWI in 1992.2 FSE creates the extrudate by plunging rotating tools into material placed in a die. Tubes and wires are extruded without being melted. Compared with other metal extrusion processes, FSE is novel in that it relies on the intrinsic frictional heating to soften and plasticize the material. The extensive plastic deformation inherent to the process makes it possible to stir, consolidate, and convert the powders, chips, and other feedstock metals directly into useable product forms. Multiple types of raw materials such as solid bar, powder, and even scrap metal can be used.3,4,5,6 One of the advantages of FSE is its low energy consumption as a metal recyclizing technology compared with the common melting and casting based recycling technologies,7 which is substantiated by theoretical analysis,8 actual experimental measurement of the energy usage,5 and more recent study.4

Friction stir back extrusion (FSBE) is a specific form of FSE.2 In FSBE, feedstock materials are extruded backward with respect to the tool’s plunge direction. Both wires and tubes can be extruded with FSBE on various types of aluminum, magnesium, and copper alloys using machined chips or solid feedstocks.3,4,5,6,9,10,11,12,13 FSBE can also be used to fabricate composite material if using powder as feedstock material.14,15

Another advantage of FSE and FSBE is the equiaxed refined grain structure in the extrudate upon frictional heat and severe plastic deformation. Hence, it has great potential in providing lightweight tubes with enhanced strength and formability in the aerospace and automotive industries.

FSBE is still in its early stage of research and development for industrial applications. Various aspects of the process such as tool design and process conditions, as well as their influence on the microstructure and resultant properties, are the subject of considerable research. Strain and texture of wire FSBE were studied.16 Finite element models and experimental investigation of material flow and heat transfer were conducted as well.17,18,19 Most studies on FSBE of extruding tubes mainly used solid bar as feedstock material. So far, nearly all studies available in the open literature utilize tool settings and process conditions to subject the entire tube cross section to extensive severe plastic deformation.3,6,12 To further the understanding of FSBE, this work adopted a different experimental setup in that only the inner wall of a 6063 aluminum alloy tube was subjected to extensive frictional heating and severe plastic deformation. The microstructure changes through the extruded tube thickness were characterized and related to the process conditions such as forces and temperature.

Experimental

Experimental FSBE Setup

The essential features of the FSBE setup used in the present study are shown in Fig. 1a. The tool set consists of two parts: a friction stir tool made from MP159 superalloy and a die made from 17-4 PH steel. The FSBE tools are designed to fit into an MTS FSW machine that can generate 89 kN plunge force and 180 \( {\text{N}} \cdot {\text{m}} \) rotation torque at maximum. The rotating tool is plunged into a hollow feedstock tube, which is different from previous researches6,12,13,20 that used solid bar as feedstock. Therefore, only the material near the inner wall of the feedstock tube would be expected to be directly subjected to frictional heating and associated severe plastic deformation in FSBE. Frictional heating is generated at the interface between the rotating tool and inner surface of the billet. As the billet is heated up by the frictional heating, the billet material softens. The plunging action of the tool forces the softened material to flow through the die under extensive severe plastic deformation on the billet inner wall.

Fig. 1
figure 1

(a) A schematic drawing of the tools in the FSBE experimental setup in this study. The aluminum tube (orange) extrudes in the direction opposite to the tool plunging direction (backward extrusion), as marked by the arrow labeled “TED.” Six sets of thermocouples are located at four depths and at 1 mm and 1.5 mm from the tool and extrudate interface. (b) Process temperature data as functions of positions of the thermocouples

For the experiment, hot extruded hollow tubes of AA6063-T6 aluminum alloy were used. The hollow aluminum tubes had initial dimensions of 21.34 mm outer diameter (OD) and 16 mm inner diameter (ID). The ID of the extruded tube was the same as the OD of the plunger. Two different plungers were used in the study. One had a 16.8-mm OD, and the other had a 17.5-mm OD for more aggressive extrusion. The billet was deformed into a thin-wall tube and extruded out of the die in the direction opposite to that of the tool (see Fig. 1a).

Direct measurement of the temperature in the processing zone of the extruded material during FSBE was difficult. In this work, the temperature inside the die was measured instead. K-Type thermocouples (TC) were embedded 1.0 mm for TC 1 mm, 3 mm, 5 mm, 7 mm and 1.5 mm for TC 2,4,6,8 (Fig. 1a), respectively, from the die/extrudate interface to provide a reasonable estimate of the temperature inside the extrudate. We note that this technique was also used in friction stir welding research to understand the material thermal cycle,21,22,23 which was supported by direct temperature measurement inside the friction stir-processed region via in situ time-resolved neutron diffraction measurements.24,25,26 The thermocouple wires were embedded in predrilled channels and were attached to the end of the channel near the inner surface of the die hole. Temperature data were collected from positions at 7.62 mm, 22.86 mm, 50.8 mm, and 76.2 mm beneath the top surface of the die as shown in Fig. 1a.

The FSBE experiments consisted of two plunging steps. In the first plunging step, the tool rotated at 500 RPM and advanced at a rate of 63.5 mm/min to a depth of 31.75 mm followed by a second step at a rate of 76.2 mm/min to a depth of 86 mm.

Microhardness and Microstructure Characterization

The hardness test and microstructure characterization of the extruded tubes were performed on both the transverse section, which is perpendicular to the tube axis (labeled “TS” in Fig. 2a), and the longitudinal section, which is along the tube axis (labeled “LS” in Fig. 2a). The metallographic samples were polished and etched using Barkers reagent to reveal the grain structure. Optical micrographs were taken by a Nikon MA700 Eclipse metallurgy microscope with a polarized light source. A JEOL JSM-6500F scanning electron microscope with EDS and EBSD detectors was used to study the grain orientation, boundaries, and composition of secondary phases. EDS was done at 20 kV and 65 μA. For EBSD, the scan step was 1 μm at 30 kV. Vickers hardness mapping was conducted on both the transverse and longitudinal sections using a LECO LM100 AT microhardness tester at 10 g load and 75 μm spacing between indentations. XRD was conducted on both the original feedstock material and the extruded tubes using Cu Ka radiation (λ = 1.54 Å, 45 kV, 40 mA). Grain structures of the extruded tubes with a 17.5-OD mm plunger were revealed by electropolishing in a commercial electropolishing solution for aluminum from SiC Technologies (EP8537) at 65°C for 1–2 min.

Fig. 2
figure 2

Optical micrographs of 6063 alloy. (a) Schematic drawing of the characterized cross section. LS: longitudinal section; TS: transverse section. (b) Longitudinal view and (c) transverse view of the as-received material. (d) Longitudinal view of the extrudate. (e) Transverse view of the extrudate

Results and Discussion

Temperature and Process Conditions

Several tubes were extruded using the process conditions described in “Experimental” section. The initial hollowed feedstock tubes were 82.55 mm (3.25 inches) long. The extruded tubes were ~ 95.25 mm (3.75 inches) long. The extrusion ratio was ~ 1.15. The motion and force data were collected by the FSE system. The plunge force and torque reached and stabilized at ~ 1200 N and ~ 110 \( {\text{N}} \cdot {\text{m}} \), respectively.

The temperature data during the FSBE test were collected at a rate of 5 Hz with a dedicated temperature acquisition system. The relationship of the temperature with respect to the tool’s position is shown in Fig. 1b. At the distance 1 mm from the die/extrudate interface, the peak temperature was ~ 50°C higher than that at the distance of 1.5 mm (i.e., 0.5 mm further away) at the same depth. The highest measured temperature in the die was 550.7°C at both the 22.86 mm and 50.8 mm positions from the top of the die and 1 mm to the die/extrudate interface. It was higher than the precipitate dissolution temperature (521°C) but below the 616°C solidus temperature and 654°C liquidus temperature 6063 aluminum alloy.27 It was expected that the temperature inside the extrudate and at the interface of the extruding tool (the plunger) and the 6063 Al alloy would be > 550°C. On the other hand, the relatively high plunging force and processing torque suggested that massive or bulk melting of 6063 was unlike that during the FSBE experiment in this study. We also noted that the temperature at the measured locations lasted ~ 20 s over 520°C, the dissolution temperature of the precipitates. It was then cooled down naturally to room temperature. The effect of temperature on grain size and microstructure will be discussed in “Microstructure characterization” and “Microhardness mapping” sections.

Microstructure Characterization

Optical Microscope Imaging

The optical microscope images of the etched materials are shown in Fig. 2 for the extruded tubes made with a 16-mm plunger and in Fig. 3 for those with a 17.5-mm plunger. Figure 2b and c shows the original grain structure of the as-received 6063 Al alloy. The grain sizes of the as-received material were measured using ImageJ software.28 Grain size and morphology of the as-received material were similar on the longitudinal and transverse sections. Most of the grains were in the size range of 50–120 μm; the average grain size was 53.72 μm. The average grain diameter calculated by the EBSD graph was 58.2 μm

Fig. 3
figure 3

Optical micrographs of 6063 alloy extrusion with a larger diameter tool. (a) Transverse view of as-received material; the mean grain size is 50 ± 3 μm. (b) Transverse view of the center region of the extruded tube; the mean grain size is 18 ± 2 μm

Figure 2d and e shows the grain structure of the extruded tubes from transverse and longitudinal sections, respectively. Considerable grain refinement was observed near the tube ID surface with an average grain size of 20.6 μm The grain size and morphology near the ID surface were similar to the recrystallized grain structure in an FSW nugget zone reported by Sato et al.,29 therefore suggesting that the frictional heating and server plastic deformation expected in this region of the inner wall in our FSBE experiment setup would lead to dynamic recrystallization as in the case of the stir zone of FSW. A gradual transition in grain size could be seen from the ID to OD of the extruded tubes. It was noted that the grain size near the OD surface was larger than that of the as-received, indicating grain growth in this region under the FSBE experimental conditions applied in the present study.

Figure 3a and b shows the typical grain structure before and after the FSBE process with the larger 17.5-mm diameter tool. The grain size was determined using the circular intercept procedure per ASTM E112–12. The mean grain size of the as-received material was 50 ± 3 μm, close to the measured values using the ImageJ software. As shown in Fig. 3b, the grain structure of the extrude tubes had a smaller mean grain size of 18 ± 2 μm, depicting an improved grain refinement by increasing the tool’s diameter.

Energy-dispersive x-ray spectroscopy

Figure 4 shows the precipitate distribution of the extruded tube using the smaller 16-mm-diameter tool. Figure 4a shows the results near the interface between the tool and extruded tube. The uniformly distributed light-colored particles of 2–5 μm size (marked by white arrows) were identified as intermetallic precipitates. 6063 alloy is an Al–Mg–Si alloy system with Fe up to 0.35 wt.%. Mg–Si and AlFeSi intermetallic phases are the main precipitations in the material. One of the particles shown under higher magnification in Fig. 4b was further analyzed by EDS. Figure 4c shows the EDS spectrum of the area within the red rectangle in Fig. 4b. Relatively high concentrations of Fe (6.99 at.%) and Si (4.57 at.%) were measured in the particle, compared with measurements of 0.07 at.% Fe and 0.43 at.% Si in the adjacent dark-colored aluminum grain matrix. Element mappings of the region in Fig. 4b are shown as Fig. 4d, e, and f, respectively, for Mg, Fe, and Si, which also revealed enrichment of Fe and Si. Similar results were obtained from multiple precipitations. The ratio of Fe:Si was determined as 1.57. Therefore, the precipitation was identified as αAlFeSi precipitation, according to Refs. 30 and 31.

Fig. 4
figure 4

EDS results of the ID region of the extruded tube: (a) white arrows indicate AlFeSi particles in the material; (b) higher magnification view of the AlFeSi precipitates; (c) EDS spectrum of the red rectangle zone marked in (b); element mapping of (d) magnesium, (e) iron and (f) silicon of the region in (b)

Mg–Si intermetallic (β″, β′) are the major strengthening phases of the 6063 aluminum alloy.29,32,33 As the 6063 experiences a peak temperature higher than its dissolution temperature in FSBE, as measured in this study, it was expected that the Mg–Si intermetallic precipitates would be dissolved in the experiment, similar to the same observation of precipitate dissolution during friction stir welding.29,34,35 Previous studies detected Mg–Si precipitate particles of 100–500 nm size in T6 heat-treated 6061 and 6063 alloy,36,37,38 while no Mg–Si precipitation was identified from the EDS test of the processed material. The x-ray diffraction (XRD) measurement performed on the as-received material and extruded material corroborated this assessment. As shown in Table I, the lattice spacing of the extruded material was larger (4.052 Å) than that of as-received samples (4.046 Å), which indicates lattice expansion of the extruded materials as a result of supersaturation of Mg and Si in the matrix.

Table I 2θ of the x-ray diffraction peaks of the original material and FSBE extrudate

Electron Backscattering Diffraction

Figure 5 shows the EBSD pattern of the original feedstock 6063 Al alloy. OIM analysis 7 software (EDAX Inc.) was used to collect data for the grain size, boundaries, and misorientation. Figure 5a is an orientation map based on the [001] inverse pole figure (IPF) of the as-received material on the longitudinal section. Figure 5b shows the grain boundary map colored with the kernel average misorientation (KAM) of the same area. Low-angle grain boundaries (LAGBs) (2°–15°) and high-angle grain boundaries (HAGBs) (above 15°) are plotted with green and black lines in Fig. 5b. LAGBs were considered subgrain structures, and the average grain diameter was calculated by software using HAGBs to identify the grains. The average grain diameter was 59.18 μm with a 27.33 μm standard deviation.

Fig. 5
figure 5

EBSD image of the original as-received material: (a) orientation map colored by a [001] inverse pole figure (IPF) and (b) phase distribution and grain boundaries. Right: The legends list the color code of IPFs and phase-boundary maps

Figure 6a, b, and c shows the orientation maps based on the [001] inverse pole figures near the plunging tool interface [i.e., inner diameter zone (IDZ)], at the half wall thickness (HWTZ), and near the die interface [i.e., outer diameter zone (ODZ)] on the longitudinal section. Figure 6d–f shows the grain boundary maps colored with KAM of the same zones. The parameters used to characterize the grain elongation direction, the average grain angles in Fig. 6a, were 12.1°, 11.7°, and 13.2° at the IDZ, HWTZ, and ODZ zones, respectively.39 A small average grain angle indicates that the major axis of the grain preferably aligns to the images’ horizonal direction, which is also the circumferential direction of the tube. Grains shown in Fig. 6 are slightly elongated along the axial direction (denoted as ‘AD’ in Fig. 5) of the tube, likely related to the fact that the material is sheared in the out-of-plane direction and compressed in the radial direction (denoted as ‘RD’ in Fig. 5) as the rotating tool processes the tube’s ID.

Fig. 6
figure 6

EBSD images of the extruded tube: [001] inverse pole figure (IPF) image of (a) IDZ, (b) HWTZ, and (c) ODZ; boundary maps of (d) IDZ, (e) HWTZ, and (f) ODZ. Circle A highlights a recrystallized grain. Circle B highlights a grain with LAGB from DRV. AD: axial direction, RD: radial direction. RD arrow points at the direction from OD to ID

The FSBE process in this research produced an equiaxed grain structure, which is commonly seen in other published FSBE studies.5,6,9,10 Globular grains are dominant in the extrudate microstructure. The average grain size from the EBSD measurement is consistent with that obtained optically shown in Fig. 2: the grain size gradually increases from 20.6 μm at IDZ, 58.5 μm at HWTZ, and 89.1 μm at ODZ. The tube ID grain refinement can be attributed to the dynamic recovery (DRV) and dynamic recrystallization (DRX). During the plastic deformation under a high enough temperature (> 40% of the melting temperature of the material), dislocations inside the grain are annihilated or rearranged to form LAGBs by dislocation glide, climb, and cross-slip. Globular subgrain structures are formed with LAGB separation of the grain.40,41 As the extent of deformation increases, subgrains become smaller individual grains via two possible mechanisms: continuous dynamic recrystallization (CDRX) and geometric dynamic recrystallization (GDRX).42,43 Discontinuous dynamic recrystallization is not likely to happen in aluminum or its alloys because of its high stacking fault energy.44 The transition of the grain diameter in different areas may be due to variations in deformation history. In IDZ (see Fig. 6d), the strain input was large enough to produce refined grains by CDRX (typical grains are highlighted in the circle labeled A); some grains retained their initial size with subgrains inside via the DRV process in IDZ (highlighted in the circle labeled B). Large fractions of LAGBs (0.209 from the longitudinal view and 0.237 from the transverse view) and subgrains in IDZ indicate an incomplete grain refinement in the region. In HWTZ, only grains whose size is comparable to the size of grains in the original as-received material and LAGB by DRV are present because the strain input was insufficient in the area. The ODZ experienced a grain growth (89.1 μm) compared with the grain size in the initial microstructure. With the FSBE experimental setup in this present work, it is expected that there was minimal shear strain at the ODZ, as most of the frictional heating and shear deformation between the rotating tool and the 6063 Al alloy took place at the ID surface of the Al tube. On the other hand, the ODZ reached a peak temperature > 550°C, according to the temperature measurement. This high temperature would result in grain growth. LAGB marked by the arrow ‘C’ in Fig. 6f indicates that smaller grains in the as-received material merged into coarse grains. HAGB was turned into LAGB by the rearrangement of dislocation.29,45,46 Grain refinement in our FSBE process is limited to the inner surface of the extruded tube, resulting in considerable variations of grain sizes through the tube wall thickness.

Microhardness Mapping

The results of microhardness tests are shown in Fig. 7a. The average hardness measured on the original as-received billet had an average microhardness of HV 90–95, which is typical for the T6 aging condition of the 6063 alloy. The hardness of the extruded tube is in the range of HV 60–75, which is equivalent to the T4–T5 aging condition and higher than that of the completed supersaturated solid solution situation (HV 40–50).47 Despite the considerable grain size variations, the microhardness is evenly distributed from OD to ID with minor deviation. The hardness values in the extruded tubes are very similar to hardness in the thermal–mechanical affected zones of FSW with similar thermal cycles as reported in Refs. 29, 48, and 49.

Fig. 7
figure 7

(a) Microhardness value along the radial distance of the cross sections. (b) Histogram of the average grain size (red bar) and standard deviation (error bar) from the longitudinal view calculated by EBSD analysis software at different positions. OM: original material; IDZ, HWTZ, and ODZ of the extrudate

The effect of the grain size on hardness is not significant for precipitate-hardening alloys.50,51 An estimation of a difference in grain size-induced hardness in the ODZ and IDZ can be expressed using the Hall–Petch relationship:52

$$ \Delta H = k \cdot \left( {D_{\text{ID}}^{{ - \frac{1}{2}}} - D_{\text{OD}}^{{ - \frac{1}{2}}} } \right) $$

where the \( \Delta H \) is the microhardness difference and DID and DOD are the grain sizes of IDZ and ODZ. Average grain diameters (20.6 μm and 89.1 μm at IDZ and ODZ, respectively) are used in this case. Taking the appropriate value of the constant (k), which is ~ 40  \( {\text{HV}} \cdot \mu {\text{m}}^{1/2} \) in the literature,53 the difference in grain sizes in the present study would result in a maximum hardness difference of approximately 4.4 HV. This explains the relatively even hardness variation through the wall thickness despite the considerable changes in the grain size change.

Conclusion

A specially FSBE experimental setup was utilized to purposely introduce a deformation gradient through the wall thickness of the friction stir back-extruded 6063-T6 alloy tubes. The frictional heating and severe plastic deformation associated with FSBE were largely limited to the inner surface of the extruded tubes. Under the FSBE conditions in the present study, gradual grain size changes took place from the inner to outer surface. The as-received material had globular grains with an average diameter of 50–60 μm. Refined grains with ~ 20 μm average diameter were formed near the inner tube wall surface because of dynamic recovery and recrystallization. On the other hand, considerable grain growth up to ~ 90 μm from 50 μm of the as-received material was observed near the outer tube wall surface, attributed to thermally driven grain growth.

The friction stir back-extruded tube had a uniform microhardness distribution through the wall thickness. The microhardness was reduced to HV 60–75 in the extruded tubes from HV 90–95 of the as-received materials under T6 heat treatment conditions, which can be attributed to the relatively high extrusion temperature exceeding 550°C over the entire tube wall to cause complete dissolution of the Mg–Si intermetallic precipitates during the extrusion and uniform re-precipitation (natural aging) during the subsequent cooling.