{"id":464,"date":"2025-02-13T19:45:13","date_gmt":"2025-02-13T19:45:13","guid":{"rendered":"https:\/\/content.one.lumenlearning.com\/calculus2\/chapter\/physical-applications-learn-it-2\/"},"modified":"2025-02-13T19:45:13","modified_gmt":"2025-02-13T19:45:13","slug":"physical-applications-learn-it-2","status":"publish","type":"chapter","link":"https:\/\/content.one.lumenlearning.com\/calculus2\/chapter\/physical-applications-learn-it-2\/","title":{"raw":"Physical Applications: Learn It 2","rendered":"Physical Applications: Learn It 2"},"content":{"raw":"\n<h2>Mass and Density Cont.<\/h2>\n<h3>Mass\u2013Density Formula of a Two-Dimensional Disk<\/h3>\n<p id=\"fs-id1167793940456\">We now extend this concept to find the mass of a two-dimensional disk of radius [latex]r.[\/latex] As with the rod we looked at in the one-dimensional case, here we assume the disk is thin enough that, for mathematical purposes, we can treat it as a two-dimensional object.<\/p>\n<p>We assume the density is given in terms of mass per unit area (called <span class=\"no-emphasis\"><em>area density<\/em><\/span>), and further assume the density varies only along the disk\u2019s radius (called <span class=\"no-emphasis\"><em>radial density<\/em><\/span>). We orient the disk in the [latex]xy[\/latex]-plane, with the center at the origin. Then, the density of the disk can be treated as a function of [latex]x,[\/latex] denoted [latex]\\rho (x).[\/latex] We assume [latex]\\rho (x)[\/latex] is integrable.<\/p>\n<p>Just as we did with the one-dimensional rod, we need to partition the interval. Partition the interval [latex][0,r][\/latex] into [latex]n[\/latex] segments, each of width [latex]\u0394x[\/latex].<\/p>\n\n[caption id=\"\" align=\"aligncenter\" width=\"613\"]<img src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/2332\/2018\/01\/11213159\/CNX_Calc_Figure_06_05_003.jpg\" alt=\"This figure has two images. The first is labeled \u201ca\u201d and is a circle with radius r. The center of the circle is labeled 0. The circle also has the positive x-axis beginning at 0, extending through the circle. The second figure is labeled \u201cb\u201d. It has two concentric circles with center at 0 and the x-axis extending out from 0. The concentric circles form a washer. The width of the washer is from xsub(i-1) to xsubi and is labeled delta x.\" width=\"613\" height=\"324\"> Figure 3. (a) A thin disk in the xy-plane. (b) A representative washer.[\/caption]\n\n<p id=\"fs-id1167793952882\">We now approximate the density and area of the washer to calculate an approximate mass, [latex]{m}_{i}.[\/latex] Note that the area of the washer is given by<\/p>\n<div id=\"fs-id1167793787727\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]\\begin{array}{cc}\\hfill {A}_{i}&amp; =\\pi {({x}_{i})}^{2}-\\pi {({x}_{i-1})}^{2}\\hfill \\\\ &amp; =\\pi \\left[{x}_{i}^{2}-{x}_{i-1}^{2}\\right]\\hfill \\\\ &amp; =\\pi ({x}_{i}+{x}_{i-1})({x}_{i}-{x}_{i-1})\\hfill \\\\ &amp; =\\pi ({x}_{i}+{x}_{i-1})\\text{\u0394}x.\\hfill \\end{array}[\/latex]<\/div>\n<p id=\"fs-id1167794031090\">You may recall that we had an expression similar to this when we were computing volumes by shells. As we did there, we use [latex]{x}_{i}^{*}\\approx ({x}_{i}+{x}_{i-1})\\text{\/}2[\/latex] to approximate the average radius of the washer. We obtain<\/p>\n<div id=\"fs-id1167793266910\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]{A}_{i}=\\pi ({x}_{i}+{x}_{i-1})\\text{\u0394}x\\approx 2\\pi {x}_{i}^{*}\\text{\u0394}x.[\/latex]<\/div>\n<p id=\"fs-id1167793930438\">Using [latex]\\rho ({x}_{i}^{*})[\/latex] to approximate the density of the washer, we approximate the mass of the washer by<\/p>\n<div id=\"fs-id1167793918720\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]{m}_{i}\\approx 2\\pi {x}_{i}^{*}\\rho ({x}_{i}^{*})\\text{\u0394}x.[\/latex]<\/div>\n<p>Adding up the masses of the washers, we see the mass [latex]m[\/latex] of the entire disk is approximated by<\/p>\n<div id=\"fs-id1167793384645\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]m=\\displaystyle\\sum_{i=1}^{n} {m}_{i}\\approx \\displaystyle\\sum_{i=1}^{n} 2\\pi {x}_{i}^{*}\\rho ({x}_{i}^{*})\\text{\u0394}x.[\/latex]<\/div>\n<p id=\"fs-id1167794176147\">We again recognize this as a Riemann sum, and take the limit as [latex]n\\to \\infty .[\/latex] This gives us<\/p>\n<div id=\"fs-id1167793930066\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]m=\\underset{n\\to \\infty }{\\text{lim}} \\displaystyle\\sum_{i=1}^{n} 2\\pi {x}_{i}^{*}\\rho ({x}_{i}^{*})\\text{\u0394}x={\\displaystyle\\int }_{0}^{r}2\\pi x\\rho (x)dx.[\/latex]<\/div>\n<p id=\"fs-id1167793950100\">We summarize these findings in the following theorem.<\/p>\n<section class=\"textbox keyTakeaway\">\n<h3>mass\u2013density formula of a two-dimensional disk<\/h3>\n<p id=\"fs-id1167793625643\">Let [latex]\\rho (x)[\/latex] be an integrable function representing the radial density of a disk of radius [latex]r.[\/latex] Then the mass of the disk is given by<\/p>\n<div id=\"fs-id1167793469833\" class=\"equation\" style=\"text-align: center;\">[latex]m={\\displaystyle\\int }_{0}^{r}2\\pi x\\rho (x)dx[\/latex]<\/div>\n<\/section>\n<section class=\"textbox example\">\n<p>Let [latex]\\rho (x)=\\sqrt{x}[\/latex] represent the radial density of a disk. Calculate the mass of a disk of radius [latex]4[\/latex].<\/p>\n\n[reveal-answer q=\"fs-id1167793477594\"]Show Solution[\/reveal-answer] [hidden-answer a=\"fs-id1167793477594\"]\n\n<p id=\"fs-id1167793477594\">Applying the formula, we find<\/p>\n<div id=\"fs-id1167793510552\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]\\begin{array}{cc}\\hfill m&amp; ={\\displaystyle\\int }_{0}^{r}2\\pi x\\rho (x)dx\\hfill \\\\ &amp; ={\\displaystyle\\int }_{0}^{4}2\\pi x\\sqrt{x}dx=2\\pi {\\displaystyle\\int }_{0}^{4}{x}^{3\\text{\/}2}dx\\hfill \\\\ &amp; =2\\pi {\\frac{2}{5}{x}^{5\\text{\/}2}|}_{0}^{4}=\\frac{4\\pi }{5}\\left[32\\right]=\\frac{128\\pi }{5}.\\hfill \\end{array}[\/latex]<\/div>\n<div class=\"equation unnumbered\" style=\"text-align: left;\">[\/hidden-answer]<\/div>\n<\/section>\n<div>\n<section class=\"textbox tryIt\">\n<p>[ohm_question hide_question_numbers=1]287495[\/ohm_question]<\/p>\n<\/section>\n<\/div>\n","rendered":"<h2>Mass and Density Cont.<\/h2>\n<h3>Mass\u2013Density Formula of a Two-Dimensional Disk<\/h3>\n<p id=\"fs-id1167793940456\">We now extend this concept to find the mass of a two-dimensional disk of radius [latex]r.[\/latex] As with the rod we looked at in the one-dimensional case, here we assume the disk is thin enough that, for mathematical purposes, we can treat it as a two-dimensional object.<\/p>\n<p>We assume the density is given in terms of mass per unit area (called <span class=\"no-emphasis\"><em>area density<\/em><\/span>), and further assume the density varies only along the disk\u2019s radius (called <span class=\"no-emphasis\"><em>radial density<\/em><\/span>). We orient the disk in the [latex]xy[\/latex]-plane, with the center at the origin. Then, the density of the disk can be treated as a function of [latex]x,[\/latex] denoted [latex]\\rho (x).[\/latex] We assume [latex]\\rho (x)[\/latex] is integrable.<\/p>\n<p>Just as we did with the one-dimensional rod, we need to partition the interval. Partition the interval [latex][0,r][\/latex] into [latex]n[\/latex] segments, each of width [latex]\u0394x[\/latex].<\/p>\n<figure style=\"width: 613px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/2332\/2018\/01\/11213159\/CNX_Calc_Figure_06_05_003.jpg\" alt=\"This figure has two images. The first is labeled \u201ca\u201d and is a circle with radius r. The center of the circle is labeled 0. The circle also has the positive x-axis beginning at 0, extending through the circle. The second figure is labeled \u201cb\u201d. It has two concentric circles with center at 0 and the x-axis extending out from 0. The concentric circles form a washer. The width of the washer is from xsub(i-1) to xsubi and is labeled delta x.\" width=\"613\" height=\"324\" \/><figcaption class=\"wp-caption-text\">Figure 3. (a) A thin disk in the xy-plane. (b) A representative washer.<\/figcaption><\/figure>\n<p id=\"fs-id1167793952882\">We now approximate the density and area of the washer to calculate an approximate mass, [latex]{m}_{i}.[\/latex] Note that the area of the washer is given by<\/p>\n<div id=\"fs-id1167793787727\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]\\begin{array}{cc}\\hfill {A}_{i}& =\\pi {({x}_{i})}^{2}-\\pi {({x}_{i-1})}^{2}\\hfill \\\\ & =\\pi \\left[{x}_{i}^{2}-{x}_{i-1}^{2}\\right]\\hfill \\\\ & =\\pi ({x}_{i}+{x}_{i-1})({x}_{i}-{x}_{i-1})\\hfill \\\\ & =\\pi ({x}_{i}+{x}_{i-1})\\text{\u0394}x.\\hfill \\end{array}[\/latex]<\/div>\n<p id=\"fs-id1167794031090\">You may recall that we had an expression similar to this when we were computing volumes by shells. As we did there, we use [latex]{x}_{i}^{*}\\approx ({x}_{i}+{x}_{i-1})\\text{\/}2[\/latex] to approximate the average radius of the washer. We obtain<\/p>\n<div id=\"fs-id1167793266910\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]{A}_{i}=\\pi ({x}_{i}+{x}_{i-1})\\text{\u0394}x\\approx 2\\pi {x}_{i}^{*}\\text{\u0394}x.[\/latex]<\/div>\n<p id=\"fs-id1167793930438\">Using [latex]\\rho ({x}_{i}^{*})[\/latex] to approximate the density of the washer, we approximate the mass of the washer by<\/p>\n<div id=\"fs-id1167793918720\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]{m}_{i}\\approx 2\\pi {x}_{i}^{*}\\rho ({x}_{i}^{*})\\text{\u0394}x.[\/latex]<\/div>\n<p>Adding up the masses of the washers, we see the mass [latex]m[\/latex] of the entire disk is approximated by<\/p>\n<div id=\"fs-id1167793384645\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]m=\\displaystyle\\sum_{i=1}^{n} {m}_{i}\\approx \\displaystyle\\sum_{i=1}^{n} 2\\pi {x}_{i}^{*}\\rho ({x}_{i}^{*})\\text{\u0394}x.[\/latex]<\/div>\n<p id=\"fs-id1167794176147\">We again recognize this as a Riemann sum, and take the limit as [latex]n\\to \\infty .[\/latex] This gives us<\/p>\n<div id=\"fs-id1167793930066\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]m=\\underset{n\\to \\infty }{\\text{lim}} \\displaystyle\\sum_{i=1}^{n} 2\\pi {x}_{i}^{*}\\rho ({x}_{i}^{*})\\text{\u0394}x={\\displaystyle\\int }_{0}^{r}2\\pi x\\rho (x)dx.[\/latex]<\/div>\n<p id=\"fs-id1167793950100\">We summarize these findings in the following theorem.<\/p>\n<section class=\"textbox keyTakeaway\">\n<h3>mass\u2013density formula of a two-dimensional disk<\/h3>\n<p id=\"fs-id1167793625643\">Let [latex]\\rho (x)[\/latex] be an integrable function representing the radial density of a disk of radius [latex]r.[\/latex] Then the mass of the disk is given by<\/p>\n<div id=\"fs-id1167793469833\" class=\"equation\" style=\"text-align: center;\">[latex]m={\\displaystyle\\int }_{0}^{r}2\\pi x\\rho (x)dx[\/latex]<\/div>\n<\/section>\n<section class=\"textbox example\">\n<p>Let [latex]\\rho (x)=\\sqrt{x}[\/latex] represent the radial density of a disk. Calculate the mass of a disk of radius [latex]4[\/latex].<\/p>\n<div class=\"qa-wrapper\" style=\"display: block\"><button class=\"show-answer show-answer-button collapsed\" data-target=\"qfs-id1167793477594\">Show Solution<\/button> <\/p>\n<div id=\"qfs-id1167793477594\" class=\"hidden-answer\" style=\"display: none\">\n<p id=\"fs-id1167793477594\">Applying the formula, we find<\/p>\n<div id=\"fs-id1167793510552\" class=\"equation unnumbered\" style=\"text-align: center;\">[latex]\\begin{array}{cc}\\hfill m& ={\\displaystyle\\int }_{0}^{r}2\\pi x\\rho (x)dx\\hfill \\\\ & ={\\displaystyle\\int }_{0}^{4}2\\pi x\\sqrt{x}dx=2\\pi {\\displaystyle\\int }_{0}^{4}{x}^{3\\text{\/}2}dx\\hfill \\\\ & =2\\pi {\\frac{2}{5}{x}^{5\\text{\/}2}|}_{0}^{4}=\\frac{4\\pi }{5}\\left[32\\right]=\\frac{128\\pi }{5}.\\hfill \\end{array}[\/latex]<\/div>\n<div class=\"equation unnumbered\" style=\"text-align: left;\"><\/div>\n<\/div>\n<\/div>\n<\/section>\n<div>\n<section class=\"textbox tryIt\">\n<iframe loading=\"lazy\" id=\"ohm287495\" class=\"resizable\" src=\"https:\/\/ohm.lumenlearning.com\/multiembedq.php?id=287495&theme=lumen&iframe_resize_id=ohm287495&source=tnh\" width=\"100%\" height=\"150\"><\/iframe><br \/>\n<\/section>\n<\/div>\n","protected":false},"author":6,"menu_order":6,"template":"","meta":{"_candela_citation":"[{\"type\":\"cc\",\"description\":\"Calculus Volume 1\",\"author\":\"Gilbert Strang, Edwin (Jed) Herman\",\"organization\":\"OpenStax\",\"url\":\"https:\/\/openstax.org\/details\/books\/calculus-volume-1\",\"project\":\"\",\"license\":\"cc-by-nc-sa\",\"license_terms\":\"Access for free at https:\/\/openstax.org\/books\/calculus-volume-1\/pages\/1-introduction\"},{\"type\":\"original\",\"description\":\"2.5 Physical Applications\",\"author\":\"Ryan Melton\",\"organization\":\"\",\"url\":\"\",\"project\":\"\",\"license\":\"cc-by\",\"license_terms\":\"\"}]","pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[],"contributor":[],"license":[],"part":450,"module-header":"","content_attributions":[{"type":"cc","description":"Calculus Volume 1","author":"Gilbert Strang, Edwin (Jed) Herman","organization":"OpenStax","url":"https:\/\/openstax.org\/details\/books\/calculus-volume-1","project":"","license":"cc-by-nc-sa","license_terms":"Access for free at https:\/\/openstax.org\/books\/calculus-volume-1\/pages\/1-introduction"},{"type":"original","description":"2.5 Physical Applications","author":"Ryan Melton","organization":"","url":"","project":"","license":"cc-by","license_terms":""}],"internal_book_links":[],"video_content":null,"cc_video_embed_content":{"cc_scripts":"","media_targets":[]},"try_it_collection":null,"_links":{"self":[{"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/pressbooks\/v2\/chapters\/464"}],"collection":[{"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/wp\/v2\/users\/6"}],"version-history":[{"count":0,"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/pressbooks\/v2\/chapters\/464\/revisions"}],"part":[{"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/pressbooks\/v2\/parts\/450"}],"metadata":[{"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/pressbooks\/v2\/chapters\/464\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/wp\/v2\/media?parent=464"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/pressbooks\/v2\/chapter-type?post=464"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/wp\/v2\/contributor?post=464"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/content.one.lumenlearning.com\/calculus2\/wp-json\/wp\/v2\/license?post=464"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}