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Root-structure and the occurrence of full and lengthened grade in PIE root nouns<br />

Benedicte Nielsen Whitehead, University of Copenhagen<br />

The paper reviews the ablaut patterns of PIE root nouns, especially the conditions for<br />

nominatival lengthening and the choice of weak grade correlating to a specific form of the<br />

nominative.<br />

Certain basics of PIE root-noun apophony are today considered commonplace, such as<br />

the link between ablaut and specific semantic types: stative agent-nouns, action nouns,<br />

nomina rei actae (Schindler 1972); or the fact that that nominatival lengthening occurs only in<br />

stems with one final consonant (e.g. Möller 1880: 499).<br />

However, Schindler 1979: 60 also pointed out that in certain well-defined cases, root<br />

structure was a determining factor for the choice of a particular ablaut grade. This paper<br />

surveys 80 root nouns of presumed IE age and qualifies his findings as follows: a root noun<br />

will only ever appear in a form that displays (a) at least one initial consonant, (b) a syllabic<br />

element and (c) if possible, exactly one final consonant. I.e., the root maintains the basic<br />

phonological structure C N V 1 C 1 , when possible.<br />

The relevance of these observations is twofold. As will be illustrated, we should,<br />

firstly, pay special attention to a small handful of root nouns that do not adhere to these rules,<br />

and secondly, we should be careful when drawing conclusions about original ablaut patterns<br />

on the basis of attested forms.<br />

These facts challenge our otherwise firm convictions about the ablaut of PIE root<br />

nouns.<br />

References:<br />

Möller, H. 1880. “Zur declination. Germanisch ā ē ō in de endungen des nomens und die<br />

Entstehung des o (*a₂)”. PBB 7: 482-547.<br />

Schindler, J. 1972. Das Wurzelnomen im Arischen und Griechischen. Dissertation: Phil. Fak.,<br />

Universität Würzburg.<br />

Schindler, J. 1979. “C. Rezension”. Die Sprache 25 (1): 57-60.<br />

29

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