Micro and macro properties of silico-aluminophosphate geopolymer: Role of incinerated sewage sludge ash (ISSA)

The mechanistic insights into silico-aluminophosphate (SAP) geopolymer formation remain an enigma. Here, we aim to elucidate this process and improve the early-age performance of SAP geopolymers by utilizing incinerated sewage sludge ash (ISSA). Interestingly, phosphoric acid-ISSA interaction releas...

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Veröffentlicht in:Construction & building materials 2024-02, Vol.416, p.135231, Article 135231
Hauptverfasser: Alrefaei, Yazan, Ali, Hafiz Asad, Lao, Jian-Cong, Dai, Jian-Guo, Poon, Chi Sun
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Sprache:eng
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Zusammenfassung:The mechanistic insights into silico-aluminophosphate (SAP) geopolymer formation remain an enigma. Here, we aim to elucidate this process and improve the early-age performance of SAP geopolymers by utilizing incinerated sewage sludge ash (ISSA). Interestingly, phosphoric acid-ISSA interaction released Ca2+ and Al3+ ions from ISSA faster than the dealumination of metakaolin. These ions agglutinated with the active soluble (PO4)3- units, evidenced by transmission electron microscopy (TEM), enhancing the early-age compressive strength of ISSA-incorporated SAP geopolymer binders. In contrast, the later strengths were relatively similar to the reference. Such binders had primary silico-alumino-phosphate (S-A-P) gels, possibly intimate with calcium-phosphate (C-P) and alumino-phosphate (A-P) gels, improving the micromechanical properties of the binder. The elastic moduli of these gels lay between 23–25 GPa, higher than conventional N-A-S-H gels. Furthermore, ISSA switched the chemistry of reaction products by favoring AlIV-OP units over AlVI-OP units in SAP geopolymers, even though the Si environment remained unchanged, as confirmed by NMR. •Formation mechanism of SAP geopolymer with and without ISSA is reported.•ISSA addition enhanced the early-age compressive strength of SAP geopolymer.•ISSA reduced the phosphoric acid in the SAP geopolymers by up to 28% by weight.•The mechanisms that govern such observations are discussed in detail.
ISSN:0950-0618
1879-0526
DOI:10.1016/j.conbuildmat.2024.135231