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SOIL MECHANICS AND FOUNDATION ENGINEERING

SECOND EDITION

SOIL MECHANICS AND FOUNDATION ENGINEERING

SECOND EDITION

Adhiparasakthi Engineering College, Melmaruvathur Kancheepuram District, Tamil Nadu

Preface

Popularity of this book amongst the undergraduate students and practising engineers has made the author to revive the book with updated materials.

The second edition of the book comprises 24 chapters dealing with four components, viz. Basic Principles of Soil Mechanics, Laboratory Determination of Soil Parameters Under Different Field Conditions, Earth Pressure Problems Including Foundations and Advanced Topics on Soil Mechanics Applications.

Chapters 1–9 deal with Basic Principles of Soil Mechanics. Chapter 1 deals with soil formation and composition, highlighting the types of weathering, soil formation in nature and major soil deposits of India. Chapters 2 and 3 explain the methods of identification and classification of soil including Bureau of Indian Standards, with the background knowledge of the index properties of soils. The basic properties of soils are compaction, permeability, consolidation and shear strength. Chapters 4–9 detail these properties. Principles of compaction and field compactions are explained in Chapter 4. Flow through porous medium and its applications are dealt within Chapters 5 and 6. Stresses in nature and applied stresses cause consolidation and failure due to shear. These aspects are dealt with at length in Chapters 7, 8 and 9. Chapter 7 details the different types of loading and the methods of computing stresses. Chapter 8 explains the basic theory of consolidation followed by computation of settlements while Chapter 9 explains the methods of determining shear strength of different types of soils under different loading and drainage conditions.

Chapter 10 discusses the basic techniques of testing of soils as per the Bureau of Indian Standards. Further, it includes methods of material collection, data presentation, computation and presentation of results and discussion. Necessary diagrams and standard values are included in the chapter.

Chapters 11–19 explain the principles of earth pressure and its applications in the design of earth-retaining structures, stability of slopes and foundations. Principles of earth pressure theories, in particular, the classical earth pressure theories of Coulomb and Rankine, and other modern theories are dealt with in Chapter 11. Chapter 12 gives the design concepts of retaining walls, including sheet piles and cuts, for both active and passive cases with different backfill conditions. Stability of slopes for different soil conditions, seepage conditions and pure pressure conditions are dealt with in detail in Chapter 13 with different methods of analysis.

Chapter 14 deals with the bearing capacity of soils and the connected theories for various ground conditions. Determination of safe bearing capacity and allowable soil pressure for different loading conditions are presented in Chapter 14. Chapters 15–17 cover the subjects on foundation engineering viz. shallow foundations, pile foundations drilled and caisson foundations. The subject matter has been dealt with in depth so as to introduce the student

to the field of foundation engineering such that he/she will gain the ability to investigate and select the most suitable type of foundation. A foundation engineer or a student can select the best foundation, provided he/she knows the subsoil conditions and methods of ground improvements. These aspects are dealt with in Chapters 18 and 19. The latest methods of ground investigation and soil improvement techniques are explained in these chapters.

Advanced topics on Soil Mechanics Applications viz. Embankment Dams, Dynamic Loading of Soils, Environmental Geotechnology and Introductory Rock Mechanics are explained in Chapters 20–23. Chapter 24 on Highway Pavements, an application of soil mechanics, has been added in this second edition. Chapter 20 on Embankment Dams covers both homogeneous and non-homogeneous dams, including rock-fill dams. Theory of vibrations, theory of machine and machine foundations and design requirements are explained in Chapter 21. Chapter 22 gives a brief account of Environmental Geotechnology. An introduction on rock mechanics has been given in Chapter 23 which explains the index properties of rocks, classification and in situ stresses.

The second edition would not have been possible but for the excellent encouragement given by M/S Pearson Education for which the author expresses his gratitude.

Pondicherry

January 2013 P. Purushothama Raj

Soil Formation and Composition 1

CHAPTER HIGHLIGHTS

Origin of soils – Types of rocks – Effects of weathering – Soil formation –Major soil deposits of India – Components of soils – Size and shape of soil particles – Inter-particle forces – Soil minerals – Soil–water system – Soil structure

1.1 INTRODUCTION

Soil is an unconsolidated material that has resulted from the disintegration of rocks. It includes sediments and deposits beneath rivers and seas and on land along with all organic and inorganic materials overlying the bedrock. It, thus, constitutes the earth’s surface both on land and beneath water.

The type and characteristics of soil depend largely on its origin. Transportation causes the sizes and shapes of the particles to alter and sort into sizes. Cementation due to carbonates, oxides, or organic matter provides additional particle binding. Thus, the engineering properties, viz., permeability, consolidation, and shear strength, of a soil deposit are governed by the mode of formation, stress history, groundwater condition, and physico-chemical characteristics of the parent material.

Soil deposits constitute an assemblage of solid particles resulting in the formation of certain voids or pore spaces. These voids are in turn filled with a gas or liquid or both. These components, viz., solid particle, gas, and liquid, play a significant role in the fundamental behaviour of soil. Thus, we can visualize the soil deposit as a particulate system comprising three phases, viz., the solid phase, the liquid phase, and the gaseous phase.

This chapter deals with the geological aspects of the formation of several types of soil deposits. The composition of such soil deposits has been treated as a three-phase system. The factors contributing to the behaviour of each phase and to the soil structure formation are dealt with in this chapter.

Soil

1.2 ORIGIN OF SOILS

The earth’s crust consists of both rock and weathered rock (as soil) up to an approximate depth of 20 km. Soils (weathered rocks) originated from the rocks and minerals of the earth’s crust. The principal minerals subjected to weathering to produce soil at or near the earth’s surface and available in the order of abundance are quartz, feldspar, pyroxene, amphibole, etc. Continuous slow weathering processes, aided by crustal deformities in the past, are believed to have decomposed the solid rock to fragments, creating soils. The type of soil developed depends on the rock type, its mineral constituents, and the climatic regime of the area. Rock types are grouped into three major classes: igneous, sedimentary, and metamorphic.

Cooling and hardening of molten magma resulted in the formation of igneous rocks. Slow cooling of molten magma yields large crystals, while rapid cooling results in small crystals. Granite, syenites, diorites, and gabbros have large crystals, while basalts, rhyolites, and andesites have small crystals.

Rocks containing quartz or orthoclase minerals with high silica content (e.g., granite and rhyolite) mostly decompose into sands* or gravelly** soils with a little clay.*** On the other hand, rocks (e.g., gabbros and basalt) whose minerals contain iron, magnesium, calcium, or sodium with a little silica decompose to yield fine-textured silty+ and clayey soils. Clays are not fragments of primary minerals from the parent rock but secondary minerals formed by the decomposition of primary minerals. Thus, the behaviour of clay is different from that of gravel and sand as the latter are composed of primary minerals.

Transportation agents such as wind, water, and ice may move the loose weathered rock materials and deposit them in layers called sediments. Such sediments, with the cementing properties of fragments, when subjected under heavy pressure to compaction and cementation, result in sedimentary rocks. Sedimentary type of rocks are classified as chemical (e.g., limestones and dolomites), clastic (e.g., shale and sandstone), and biochemical or organic (e.g., fossil limestone, chalk, coral, and coal in the form of peat, lignite, bitumen, or anthracite).

Sedimentary rocks, and to a lesser extent igneous rocks, when subjected to metamorphism (changes brought about by combinations of heat, pressure, and plastic flow), undergo changes in their texture, structure, and mineral composition, resulting in rocks called metamorphic rocks. Metamorphism is of two types, thermal and dynamic. Thermal metamorphism occurs primarily due to temperature increase and high hydrostatic pressure, whereas dynamic metamorphism is due to differential pressure. Metamorphism changes limestone to marble, sandstone to quartzite, and shale to slate.

Metamorphic rocks may be categorized as foliated or non-foliated. Foliation occurs during the process of metamorphism when some metamorphic rocks reduce back to sedimentary rocks. Gneiss and schist decompose into silt–sand mixtures with mica, slates and phyllites to clays, marble to limestone, and quartzite to sands and gravels.

The cyclic process of transforming rock to soil and vice versa is a continuous process occurring over millions of years through complex chemical and physical processes. This phenomenon, referred to as the geological cycle, is schematically shown in Fig. 1.1.

Particle sizes: *sand, 0.075 to 2 mm; **gravel, 2 to 4.75 mm; ***clay, < 0.002 mm; +silt, 0.002 to 0.075 mm.

Igneous rocks

Possible melting of deep rocks

Heat, pressure, and solution

Melting of deeply

buried rocks

Metamorphic rocks

Erosion and weathering

Gravel, sand, mud, and other sediments

Heat, pressure, and

solution

Weathering, deposition, and consolidation

Sedimentary rocks

1.3 TYPES OF WEATHERING

Rock disintegration, also called weathering, is one of the important geological processes. This disintegration of rock produces and deposits unconsolidated sediments as soils for plant and animal life. Weathering may be either physical (or mechanical) or chemical.

1.3.1 Physical Weathering

The process by which rock disintegrates into smaller fragments due to factors like stress changes, climatic changes, etc., without involving any change in its properties is called physical or mechanical weathering.

The principal factor causing physical weathering is climatic change. Adverse temperature changes coupled with different thermal coefficients of rock minerals produce rock fragments. The effect will be greater when temperature changes cause a freeze–thaw cycle. Similarly, heavy rainfall also brings about physical weathering.

Stress readjustments during regional uplift, accompanied by water runoff, cause the outer shell to separate from the main rock. This process is called exfoliation and may also be caused by sudden temperature changes.

On a rugged topography, heavy wind and rain may cause erosion of the rock surface and move disintegrated fragments. This is a continuing event and depends on the type of topography and the velocity of wind and water. Abrasion of rock is caused by ice under pressure or by the pushing of large unconsolidated materials. Mechanical weathering may also be caused by organic activity, such as cracking forces exerted by plants growing in the crevasses of rocks and the moving of fragments towards the surface by animals or insects.

Fig. 1.1 Geological cycle (Source: Bowles, 1984)

1.3.2 Chemical Weathering

Due to alteration in the chemical properties of rock minerals, new compounds are formed. This is referred to as chemical weathering. Rainwater coming in contact with rock surfaces reacts forming hydrated iron oxide, carbonates, and sulphates. If there is a volume increase, the disintegration continues further. Rainwater with pH < 7, or with carbonic acid, may react chemically with some rock (e.g., limestone) and completely dissolve it. Further, during a geological time period, even a weak acid solution may cause decomposition. Due to leaching, sedimentary rocks may lose their cementing properties.

1.4 SOIL FORMATION

Based on the method of formation, soil may be categorized as residual and transported. Residual soils are formed from the weathering of rocks and practically remain at the location of origin with a little or no movement of individual soil particles. Transported soils are those that have formed at one location (like residual soils) but are transported and deposited at another location.

1.4.1 Residual Soils

Weathering (due to climate effects) and leaching of water-soluble materials in the rock are the geological processes in the formation of these soils. The rate of rock decomposition is greater than the rate of erosion or transportation of weathering material and results in the accumulation of residual soils. As the leaching action decreases with depth, there is a progressively lesser degree of rock weathering from the surface downwards, resulting in reduced soil formation, until one finally encounters unaltered rock (Fig. 1.2). Residual soils generally comprise a wide range of particle sizes, shapes, and composition. In general, the rate of weathering is greater in warm, humid regions than in cold, dry regions. Humid, warm regions are favourable to chemical weathering. Also, because of the

Soil – Humus

Surficial Soil Zone (Oldest Soil Material)

Completely Weathered Rock Zone (Virtually all Soil Material)

Highly Weathered Rock Zone (Mostly Soil Material)

Moderately Weathered Rock Zone (Distintegrated Rock)

Slightly Weathered Rock Zone

Unweathered Rock with Fissures and Fractures in Upper Zone

1.2 Stages of formation of residual soil (Source: McCarthy, 1982)

Fig.

presence of vegetation, there is less possibility of transportation of the decomposed materials as sediments. Residual soils exist in different parts of the world, viz., Asia, Africa, south-eastern North America, Central America, and South America. Sowers (1963) reported that the depth of residual soils varies from 6 to 25 m in general and from 7.5 to 15 m in South India.

1.4.2 Transported Soils

Weathered materials have been moved from their original location to new locations by one or more of the transportation agencies, viz., water, glacier, wind, and gravity, and deposited to form transported soils. Such deposits are further classified depending on the mode of transportation causing the deposit.

Water-transported Soils. Swift-running water is capable of moving a considerable volume of soil. Soil may be transported in the form of suspended particles or by rolling and sliding along the bottom of the stream. The size of the particle that can be in suspension is related to the square of the velocity of the flowing water. Particles transported by water range in size from boulders to clay.

Coarser particles are dropped when a decrease in water velocity occurs as the stream or river deepens, widens, or changes direction. Fine particles still remain in suspension and get deposited in quieter waters downstream. This is a typical case of a stream moving downhill, passing over a valley, and ultimately reaching a large body of water. Soils that are carried and deposited by rivers are called alluvialdeposits. River deltas are formed in this manner. Soils carried by rivers, while entering a lake, deposit all the coarse particles because of a sudden decrease in velocity. Such coarse soil deposits are called lakedeltas. But the finegrained particles move to the centre of the lake and settle when the water becomes quiet. Alternate layers are formed with season, and such lake deposits are called lacustrinedeposits These deposits are weak and compressible and pose problems for foundations. If coarse and fine-grained deposits are formed in sea water areas, then they are called marinedeposits. Marine sediments are made up of terrestrial and marine contributions. The terrestrial contribution consists of particulate material eroded from the shore, as well as mineral matter, in true or colloidal solution, and this contribution decreases both in proportion and in grain size with increasing distance from the shoreline. The marine contribution is represented by the organic and inorganic remnants of dead marine life, and this normally increases with time (Iyer, 1975).

In marine deposits, marine life and environment play a more significant role than the salt concentration of the water. The clay particles absorb certain chemical elements from the organisms, which in turn can extract mineral substances from sea water. Some acids produced by the digestive tracts of marine organisms can alter the composition of the clay minerals (Iyer, 1975).

Marine clay deposits (excluding the deep deposits which have been subjected to many further changes and are overlain by other deposits) are generally weak, compressible, and problematic for foundations. If such a deposit is exposed above sea level and experiences leaching of sodium due to percolation of fresh water, it becomes very sensitive to disturbance. Glacial soils transported by rivers from melting glacial water create deposits of stratified glacial drift and are referred to as glaciofluvialdeposit or stratifieddrift.

Glacial Deposits. Compaction and re-crystallization of snow leads to the formation of glaciers. Glacier growth and movement depend on the formation of ice. Glacial deposits

Soil Mechanics and Foundation Engineering

form a very large group of transported soils. A glacier moves extremely slowly but deforms and scours the surface and the bedrock over which it passes. Melting of a glacier causes deposition of all the materials, and such a deposit is referred to as till. The land form or topographic surface after a glacier has receded is called a groundmoraine or tillplain. Till deposits which have been overrun by glaciers contain coarser particles and form good construction material.

Soils deposited by the surface and sub-surface glacial rivers that remain in the form of long-winding ridges are called eskers. They may vary from about 10 to 30 m in height and about 0.5 km to several kilometres in length. Isolated mounds of glacial debris varying from about 10 to 70 m in height and 200 to 800 m in length are called drumlins. Large boulders picked up by a glacier, transported to a new location, and dropped are called erratics.

Glacial deposits provide a poor to excellent foundation. In many locations it is often found that the material is dense and contains considerable sand and gravel. It is believed that glaciers covered a large portion of the land during the ice age. Northern USA, Northern Europe, and Canada were subjected to continent glaciers. Now glaciers cover approximately 10% of the earth’s surface. Almost all glaciers are now concentrated in Greenland and Antarctica.

Wind-transported Soils. Like water, wind can erode, transport, and deposit fine-grained soils. Soils carried by wind are subsequently deposited as aeoliandeposits. Dunes are formed due to the accumulation of such wind-deposited sands. Dunes are a rather common occurrence in the desert areas of Africa, Asia, and the USA. Sands from dunes may be used to a limited extent for construction purposes.

Fine-grained soils such as silts and clays can be transported by wind in arid regions. Wind-blown silts and clays deposited with some cementing minerals in a loose, stable condition are classified as loess. Loess deposits have low density, high compressibility, and poor bearing resistance when wet. Loess is a clastic sediment comprising a uniformly sorted mixture of silt, fine sand, and clay-size particles. The structure of a loess deposit is susceptible to collapse on saturation.

Gravity Deposits. Gravity can transport materials only for a short distance. As the movement is limited, there is no appreciable change in the materials moved. Gravity deposits are termed talus. They include the material at the base of cliff and landslide deposits. The talus material at the cliff is formed due to the disintegration and subsequent failure of the cliff face. These fragments are generally loose and porous.

Swamp and Marsh Deposits. In water-stagnated areas where the water table is fluctuating and vegetational growth is possible, swamp and marsh deposits develop. Soils transported and deposited under this environment are soft, high in organic content, and unpleasant in odour. Accumulation of partially or fully decomposed aquatic plants in swamps or marshes is termed muck or peat. Muck is a fully decomposed material, spongy, light in weight, highly compressible, and not suitable for construction purposes.

1.4.3 Desiccated Soils

If a fine-grained soil is exposed to atmosphere, water is drawn from the interior to the surface. From the surface, the water gets evaporated. This sort of drainage is referred to as drainage by desiccation. During this process the soil becomes stiffer and ultimately becomes hard. The point at which evaporation ceases depends on the relative humidity of the air around.

Under field conditions, desiccation may take place whenever the surface of the soil is not permanently flooded. Due to periodic desiccation, even fine-grained silty sands show apparent cohesion.* As the apparent cohesion is very large, even rains of long duration cannot completely remove the cohesion. This phenomenon of desiccation is very much pronounced in soils of semi-arid and arid regions. Such soils are quite often mistaken for soft rocks. In the case of soft clays, the desiccation proceeds very slowly from the exposed surface and forms a thick crust, and the thickness grows with age.

1.5 MAJOR SOIL DEPOSITS OF INDIA

Among different types of soils spread over the Indian Peninsula, only five major deposits have been identified (Katti et al., 1975), viz., marine deposits, black cotton soils, laterite and lateritic soils, alluvial deposits, and desert soils. Figure 1.3 shows the regions covered by these soil deposits.

1.5.1 Marine Deposits

The marine deposits all along the Indian coast are generally derived from terrestrial sources. These deposits cover a narrow belt of tidal flats all along the coast from Porbandar in the west to Puri in the east. However, they are present over wide areas in places such as Rann of Kutch. These tidal flats experience high tide inundation. The deposits are very soft to soft clays, and the thickness varies from 5 to 20 m. The clay is medium sensitive and inorganic in nature. These deposits generally need a pre-treatment before application of any external load (Iyer, 1975). In order to prevent failures during construction, controlled loading should be planned (Katti et al., 1975).

1.5.2 Black Cotton Soils

Black cotton soil is one of the major soil deposits of India and is spread over a wide area of 3,00,000 km2. The primary bed rock is basalt or trap, and in some locations, quartzites, schists, and sedimentary rocks are also reported (Katti et al., 1975). The black cotton soil is expansive in nature due to the presence of montmorillonite and illite clay minerals. The top black subsoil varies in thickness up to a maximum of 20 m. Based on the pedological conditions, crack depth and pattern vary. The soil surface is hard during summer and becomes slushy during the rainy season. The effect of seasonal moisture change brings in volume changes up to a maximum depth of 1.5 m. Because of the swelling and shrinking nature of the soil, there is a necessity for treatment of the soil, and special foundations need to be adopted in such soils to prevent failure of structures.

1.5.3 Laterites and Lateritic Soils

In tropical regions of high moisture and temperature, weathering activity is so intense that a tremendously thick soil (exceeding 30 m) may be formed from the parent rock through processes collectively termed laterization. Laterization is mainly due to the decomposition of

*A temporary shear strength gained by weathering.

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