{"id":686,"date":"2026-07-31T23:00:04","date_gmt":"2026-07-31T23:00:04","guid":{"rendered":"https:\/\/physicsfundamentalsinfo.com\/blog\/?p=686"},"modified":"2026-08-01T00:07:30","modified_gmt":"2026-08-01T00:07:30","slug":"de-broglie-wavelength","status":"publish","type":"post","link":"https:\/\/physicsfundamentalsinfo.com\/blog\/modern-physics\/de-broglie-wavelength\/","title":{"rendered":"De Broglie Wavelength: Formula, Examples and Worked Problems"},"content":{"rendered":"\n<div class=\"pf-citation\"><div class=\"eyebrow\">Definition<\/div><p>\nThe de Broglie wavelength is the wavelength associated with any moving particle, equal to Planck&#8217;s constant divided by the particle&#8217;s momentum (\u03bb = h \/ mv). Every object with mass and velocity has one. It is large enough to measure for electrons and neutrons, but unimaginably small for everyday objects like a cricket ball.\n<\/p><\/div>\n\n<p>Fire a stream of electrons at a thin crystal and they do something no particle should do. Instead of arriving as a scatter of dots, they pile up in bright rings and dark gaps &mdash; the unmistakable signature of a wave passing through a grating.<\/p>\n\n<p>That pattern is not a quirk of electrons. It is a property of everything that moves, and a young French PhD student worked out the rule for it in 1924 with one short equation.<\/p>\n\n<h2>What Is the De Broglie Wavelength?<\/h2>\n\n<p>The de Broglie wavelength is the wavelength a moving particle behaves as if it has, found by dividing Planck&#8217;s constant by the particle&#8217;s momentum. Louis de Broglie proposed it in his 1924 doctoral thesis, and it applies to electrons, neutrons, atoms, molecules and, in principle, you.<\/p>\n\n<p>Physics already accepted that light &mdash; obviously a wave &mdash; sometimes behaves like a stream of particles. De Broglie asked the obvious question in reverse. If waves can act like particles, why shouldn&#8217;t particles act like waves?<\/p>\n\n<p>The idea sounds like a philosophical flourish. It isn&#8217;t. It makes a hard numerical prediction: give a particle a momentum, and its wavelength is fixed. Nothing is left to interpretation.<\/p>\n\n<h2>The De Broglie Wavelength Formula<\/h2>\n\n<p>The de Broglie wavelength formula is Planck&#8217;s constant divided by momentum, written as lambda equals h over mv.<\/p>\n\n<div class=\"pf-formula\">\u03bb = h \/ (m\u00b7v)<\/div>\n\n<p>Because momentum p = m\u00b7v, the same equation is often written more compactly:<\/p>\n\n<div class=\"pf-formula\">\u03bb = h \/ p<\/div>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;min-width:420px;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Symbol<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Quantity<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">SI unit<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>\u03bb<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">De Broglie wavelength<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">metre (m)<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>h<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Planck constant = 6.62607015 &times; 10<sup>-34<\/sup> (exact by definition)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">joule second (J&middot;s)<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>m<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Mass of the particle<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">kilogram (kg)<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>v<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Speed of the particle<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">metre per second (m\/s)<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>p<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Momentum, equal to m&middot;v<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">kilogram metre per second (kg&middot;m\/s)<\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<p>Since 2019 the Planck constant has been fixed by definition rather than measured &mdash; its value is exactly 6.62607015 &times; 10<sup>-34<\/sup> J&middot;s, as published in <a href=\"https:\/\/physics.nist.gov\/cuu\/Constants\/index.html\" target=\"_blank\" rel=\"noopener\">NIST&#8217;s CODATA tables<\/a>. The kilogram is now defined from it.<\/p>\n\n<h3>Two rearrangements worth memorising<\/h3>\n\n<p>Exam questions rarely hand you the speed directly. Far more often you get a kinetic energy or an accelerating voltage, so these two forms save real time:<\/p>\n\n<div class=\"pf-formula\">\u03bb = h \/ sqrt(2\u00b7m\u00b7K)<\/div>\n\n<div class=\"pf-formula\">\u03bb = h \/ sqrt(2\u00b7m\u00b7q\u00b7V)<\/div>\n\n<p>Here K is kinetic energy in joules, q is the particle&#8217;s charge in coulombs, and V is the accelerating potential difference in volts. Both follow from p = sqrt(2mK), which is just <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/mechanics\/kinetic-energy-formula\/\">kinetic energy<\/a> rearranged for momentum.<\/p>\n\n<p>If you only need the number and not the algebra, our <a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/de-broglie-wavelength\">De Broglie Wavelength Calculator<\/a> takes a mass and a speed and returns the wavelength with the working shown, which makes it a fast way to sanity-check your own answers.<\/p>\n\n<h2>How the De Broglie Wavelength Works<\/h2>\n\n<p>De Broglie&#8217;s derivation starts with light and then makes one bold leap. Follow it in three steps.<\/p>\n\n<p><strong>Step 1 &mdash; start with a photon.<\/strong> Einstein and Planck had already established that a light wave of frequency f carries energy in packets of E = hf, the basis of <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/modern-physics\/photon-energy-formula\/\">photon energy<\/a>.<\/p>\n\n<p><strong>Step 2 &mdash; give the photon momentum.<\/strong> Relativity gives a massless particle p = E\/c. Substituting E = hf and c = f&lambda; makes the frequency cancel, leaving p = h\/&lambda;, or &lambda; = h\/p.<\/p>\n\n<p><strong>Step 3 &mdash; drop the assumption of masslessness.<\/strong> De Broglie&#8217;s leap was to claim &lambda; = h\/p is not a fact about light at all. It is a fact about momentum, so it must apply to an electron exactly as it applies to a photon.<\/p>\n\n<p>Nothing in step 3 was justified when he wrote it. It was, in the most literal sense, a hypothesis &mdash; and three years later the electrons settled it.<\/p>\n\n<h3>The experiment that proved it<\/h3>\n\n<p>In 1927, Clinton Davisson and Lester Germer at Bell Labs fired low-energy electrons at a nickel crystal and found scattering peaks exactly where wave <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/waves\/diffraction-physics\/\">diffraction<\/a> predicted them. Their 54 eV electrons behaved like a wave of roughly 0.165 nm.<\/p>\n\n<p>Plug 54 V into the formula and you get 0.167 nm. That agreement, from an experiment that began as an accident after a piece of glassware imploded, is documented in the <a href=\"https:\/\/physics.aps.org\/story\/v17\/st17\" target=\"_blank\" rel=\"noopener\">American Physical Society&#8217;s account of the Davisson&ndash;Germer landmark<\/a>. George Paget Thomson found the same effect in thin films weeks later.<\/p>\n\n<figure style=\"margin:32px auto;max-width:640px;text-align:center;\">\n  <img decoding=\"async\" src=\"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-content\/uploads\/2026\/07\/electron-diffraction-tube-closeup.jpg\"\n       alt=\"Electron diffraction tube used to demonstrate the de Broglie wavelength of electrons\"\n       loading=\"lazy\"\n       style=\"width:100%;height:auto;border-radius:4px;\" width=\"800\" height=\"600\">\n  <figcaption style=\"font-size:13px;color:#1F2E47;font-style:italic;margin-top:8px;\">An electron diffraction tube in operation. Electrons accelerated through a thin film strike the phosphor screen, the standard classroom demonstration of de Broglie&#8217;s prediction that matter diffracts.<\/figcaption>\n<\/figure>\n\n<div class=\"pf-sim-slot\"><div class=\"pf-sim-slot-header\"><span class=\"icon-dot\"><\/span><span class=\"label\">De Broglie Wavelength Lab<\/span><\/div><div class=\"pf-sim-slot-body\"><style>.pf-sim-frame{width:100%;border:none;height:600px}@media(max-width:760px){.pf-sim-frame{height:1000px}}<\/style><iframe src=\"\/labs\/de-broglie-wavelength.html?embed=1\" class=\"pf-sim-frame\" loading=\"lazy\"><\/iframe><\/div><\/div>\n\n<h2>De Broglie Wavelength of an Electron<\/h2>\n\n<p>For an electron accelerated from rest through a potential difference V, the de Broglie wavelength in nanometres is 1.226 divided by the square root of V in volts. It is the single most useful shortcut in this topic.<\/p>\n\n<div class=\"pf-formula\">\u03bb (nm) = 1.226 \/ sqrt(V)<\/div>\n\n<p>The constant 1.226 is not arbitrary. It is h \/ sqrt(2\u00b7m\u00b7e) converted to nanometres, using the electron mass and the elementary charge &mdash; so the shortcut is the full formula with the constants pre-multiplied.<\/p>\n\n<p>Some quick values: 1 V gives 1.23 nm, 100 V gives 0.123 nm, and 10,000 V gives 0.0123 nm. Every hundredfold rise in voltage shrinks the wavelength by a factor of ten.<\/p>\n\n<p>In practice, this is why electron microscopes exist. Visible light stalls at roughly 200 nm of resolving power, but a 100 kV electron carries a wavelength near 3.7 pm &mdash; about 50,000 times shorter.<\/p>\n\n<h2>Real-World Examples of De Broglie Wavelength<\/h2>\n\n<p>The formula is trivial. What surprises people is the spread of results &mdash; twenty-five orders of magnitude between an electron and a walking adult.<\/p>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;min-width:620px;border-collapse:collapse;\">\n<thead>\n<tr style=\"background:#0A1628;color:#FAF6EE;\">\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Object<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Mass (kg)<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Speed (m\/s)<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">De Broglie wavelength<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Comparable to<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Electron through 100 V<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">9.11 &times; 10<sup>-31<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">5.9 &times; 10<sup>6<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.2 &times; 10<sup>-10<\/sup> m (0.12 nm)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Spacing of atoms in a crystal<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Thermal neutron at 300 K<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.67 &times; 10<sup>-27<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">2.7 &times; 10<sup>3<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.5 &times; 10<sup>-10<\/sup> m (0.15 nm)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Spacing of atoms in a crystal<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Helium atom at 300 K<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">6.65 &times; 10<sup>-27<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.4 &times; 10<sup>3<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">7.3 &times; 10<sup>-11<\/sup> m<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Radius of a small atom<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">C60 fullerene molecule<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.2 &times; 10<sup>-24<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">220<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">2.5 &times; 10<sup>-12<\/sup> m (2.5 pm)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Far smaller than the molecule itself<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Speck of dust (1 microgram)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1 &times; 10<sup>-9<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1 &times; 10<sup>-3<\/sup><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">6.6 &times; 10<sup>-22<\/sup> m<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Millions of times smaller than a proton<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Cricket ball (160 g)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">0.16<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">40<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.0 &times; 10<sup>-34<\/sup> m<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">About six Planck lengths<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Adult walking<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">70<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.4<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">6.8 &times; 10<sup>-36<\/sup> m<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">Below the Planck length<\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<svg viewBox=\"0 0 700 330\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" role=\"img\" aria-label=\"Logarithmic chart comparing de Broglie wavelengths from an electron down to a cricket ball\" style=\"width:100%;height:auto;max-width:700px;display:block;margin:24px auto;\">\n<rect x=\"0\" y=\"0\" width=\"700\" height=\"330\" fill=\"#F5F2EA\"\/>\n<text x=\"14\" y=\"26\" font-family=\"Georgia,serif\" font-size=\"17\" fill=\"#0A1628\" font-weight=\"bold\">How small is a de Broglie wavelength?<\/text>\n<text x=\"14\" y=\"46\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#7A1F2B\">Bar length is logarithmic: each labelled step is a million times longer<\/text>\n<text x=\"553\" y=\"46\" font-family=\"Arial,sans-serif\" font-size=\"10\" fill=\"#7A1F2B\">atoms sit about 0.1 nm apart<\/text>\n<line x1=\"549\" y1=\"52\" x2=\"549\" y2=\"248\" stroke=\"#7A1F2B\" stroke-width=\"1.5\" stroke-dasharray=\"5 4\"\/>\n<text x=\"186\" y=\"76\" font-family=\"Arial,sans-serif\" font-size=\"12\" fill=\"#0A1628\" text-anchor=\"end\">Electron, 100 V<\/text>\n<rect x=\"196\" y=\"62\" width=\"354\" height=\"20\" fill=\"#C8932A\"\/>\n<text x=\"556\" y=\"76\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#0A1628\">0.12 nm<\/text>\n<text x=\"186\" y=\"114\" font-family=\"Arial,sans-serif\" font-size=\"12\" fill=\"#0A1628\" text-anchor=\"end\">Neutron, 300 K<\/text>\n<rect x=\"196\" y=\"100\" width=\"355\" height=\"20\" fill=\"#C8932A\"\/>\n<text x=\"557\" y=\"114\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#0A1628\">0.15 nm<\/text>\n<text x=\"186\" y=\"152\" font-family=\"Arial,sans-serif\" font-size=\"12\" fill=\"#0A1628\" text-anchor=\"end\">C60 molecule<\/text>\n<rect x=\"196\" y=\"138\" width=\"331\" height=\"20\" fill=\"#C8932A\"\/>\n<text x=\"533\" y=\"152\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#0A1628\">2.5 pm<\/text>\n<text x=\"186\" y=\"190\" font-family=\"Arial,sans-serif\" font-size=\"12\" fill=\"#0A1628\" text-anchor=\"end\">Speck of dust<\/text>\n<rect x=\"196\" y=\"176\" width=\"201\" height=\"20\" fill=\"#142139\"\/>\n<text x=\"403\" y=\"190\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#0A1628\">6.6 x 10<tspan dy=\"-4\" font-size=\"8\">-22<\/tspan><tspan dy=\"4\" font-size=\"11\"> m<\/tspan><\/text>\n<text x=\"186\" y=\"228\" font-family=\"Arial,sans-serif\" font-size=\"12\" fill=\"#0A1628\" text-anchor=\"end\">Cricket ball<\/text>\n<rect x=\"196\" y=\"214\" width=\"27\" height=\"20\" fill=\"#142139\"\/>\n<text x=\"229\" y=\"228\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#0A1628\">1.0 x 10<tspan dy=\"-4\" font-size=\"8\">-34<\/tspan><tspan dy=\"4\" font-size=\"11\"> m<\/tspan><\/text>\n<line x1=\"196\" y1=\"248\" x2=\"576\" y2=\"248\" stroke=\"#0A1628\" stroke-width=\"1.2\"\/>\n<line x1=\"196\" y1=\"248\" x2=\"196\" y2=\"253\" stroke=\"#0A1628\" stroke-width=\"1.2\"\/>\n<line x1=\"277\" y1=\"248\" x2=\"277\" y2=\"253\" stroke=\"#0A1628\" stroke-width=\"1.2\"\/>\n<line x1=\"359\" y1=\"248\" x2=\"359\" y2=\"253\" stroke=\"#0A1628\" stroke-width=\"1.2\"\/>\n<line x1=\"440\" y1=\"248\" x2=\"440\" y2=\"253\" stroke=\"#0A1628\" stroke-width=\"1.2\"\/>\n<line x1=\"522\" y1=\"248\" x2=\"522\" y2=\"253\" stroke=\"#0A1628\" stroke-width=\"1.2\"\/>\n<text x=\"196\" y=\"266\" font-family=\"Arial,sans-serif\" font-size=\"10\" fill=\"#0A1628\" text-anchor=\"middle\">10<tspan dy=\"-4\" font-size=\"8\">-36<\/tspan><\/text>\n<text x=\"277\" y=\"266\" font-family=\"Arial,sans-serif\" font-size=\"10\" fill=\"#0A1628\" text-anchor=\"middle\">10<tspan dy=\"-4\" font-size=\"8\">-30<\/tspan><\/text>\n<text x=\"359\" y=\"266\" font-family=\"Arial,sans-serif\" font-size=\"10\" fill=\"#0A1628\" text-anchor=\"middle\">10<tspan dy=\"-4\" font-size=\"8\">-24<\/tspan><\/text>\n<text x=\"440\" y=\"266\" font-family=\"Arial,sans-serif\" font-size=\"10\" fill=\"#0A1628\" text-anchor=\"middle\">10<tspan dy=\"-4\" font-size=\"8\">-18<\/tspan><\/text>\n<text x=\"522\" y=\"266\" font-family=\"Arial,sans-serif\" font-size=\"10\" fill=\"#0A1628\" text-anchor=\"middle\">10<tspan dy=\"-4\" font-size=\"8\">-12<\/tspan><\/text>\n<text x=\"386\" y=\"288\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#0A1628\" text-anchor=\"middle\">wavelength in metres<\/text>\n<text x=\"14\" y=\"314\" font-family=\"Arial,sans-serif\" font-size=\"10\" fill=\"#7A1F2B\">Gold bars reach the measurable range; navy bars never will.<\/text>\n<\/svg>\n<p style=\"text-align:center;font-size:13px;font-style:italic;color:#1F2E47;\">De Broglie wavelengths on a log scale. Only particles whose wavelength reaches atomic spacing can be made to diffract.<\/p>\n\n<h3>Where the wave actually shows up<\/h3>\n\n<p>Neutron diffraction is the clearest payoff. Because a room-temperature neutron carries a wavelength close to atomic spacing, firing neutrons at a crystal maps where its atoms sit &mdash; the routine method for locating hydrogen atoms that X-rays largely miss.<\/p>\n\n<p>The most striking demonstration came in 1999, when a Vienna group sent C60 fullerene molecules &mdash; 60 carbon atoms, 720 atomic mass units &mdash; through a nanofabricated grating. Travelling at 220 m\/s, each molecule had a wavelength of 2.5 pm and produced clean interference fringes.<\/p>\n\n<p>That wavelength is hundreds of times smaller than the molecule itself. Experiments since 2019 have pushed this to molecules beyond 25,000 atomic mass units, built from up to 2,000 atoms.<\/p>\n\n<h2>Why You Never See the Wavelength of a Cricket Ball<\/h2>\n\n<p>Everyday objects do have a de Broglie wavelength, but it is far too small to produce any observable effect. Planck&#8217;s constant sits in the numerator at 10<sup>-34<\/sup>, and everyday momentum sits in the denominator at around 1 &mdash; so the answer lands near 10<sup>-34<\/sup> m.<\/p>\n\n<p>Set that against something small. A proton is about 10<sup>-15<\/sup> m across, which makes the cricket ball&#8217;s wavelength roughly nineteen orders of magnitude smaller than a proton.<\/p>\n\n<p>To diffract a wave you need an aperture comparable to its wavelength. There is no aperture that small, and there never will be &mdash; the ball&#8217;s wavelength is only about six times the Planck length.<\/p>\n\n<p>So the classical world isn&#8217;t exempt from quantum mechanics. It just carries too much momentum for anyone to notice.<\/p>\n\n<h2>Common Misconceptions About the De Broglie Wavelength<\/h2>\n\n<h3>&ldquo;Only electrons have a de Broglie wavelength&rdquo;<\/h3>\n\n<p>Every object with momentum has one. Electrons simply have small enough momentum for the wavelength to be measurable. A bowling ball obeys the same equation and gets an unmeasurable answer.<\/p>\n\n<h3>&ldquo;The particle wiggles along a wavy path&rdquo;<\/h3>\n\n<p>Nothing physically oscillates in space. The wave is a probability amplitude &mdash; it tells you where the particle is likely to be found, which is why a single electron sent through a double slit still lands as one dot.<\/p>\n\n<h3>&ldquo;Faster particles have longer wavelengths&rdquo;<\/h3>\n\n<p>The relationship is inverse. Speed sits in the denominator, so doubling a particle&#8217;s speed halves its de Broglie wavelength. This one costs marks in exams more than any other slip in the topic.<\/p>\n\n<h3>&ldquo;The formula applies to photons too&rdquo;<\/h3>\n\n<p>Use &lambda; = h\/p for a photon and you are fine. Use &lambda; = h\/mv and you are dividing by zero, because a photon has no mass. Photon wavelength comes from E = hf instead.<\/p>\n\n<h2>How the De Broglie Wavelength Relates to Other Ideas<\/h2>\n\n<h3>It explains Bohr&#8217;s orbits<\/h3>\n\n<p>Bohr had assumed that angular momentum in a hydrogen atom comes in multiples of h\/2&pi;, with no reason why. De Broglie supplied one: an electron orbit is stable only when a whole number of its wavelengths fits around the circumference.<\/p>\n\n<div class=\"pf-formula\">2\u00b7\u03c0\u00b7r = n\u00b7\u03bb<\/div>\n\n<p>Substitute &lambda; = h\/mv and Bohr&#8217;s rule mvr = nh\/2&pi; drops straight out. An orbit with a non-integer fit would interfere with itself and cancel, which is exactly why the electron cannot spiral into the nucleus.<\/p>\n\n<svg viewBox=\"0 0 660 300\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" role=\"img\" aria-label=\"Diagram showing a matter wave that closes on itself around an allowed electron orbit and one that fails to close on a forbidden orbit\" style=\"width:100%;height:auto;max-width:660px;display:block;margin:24px auto;\">\n<rect x=\"0\" y=\"0\" width=\"660\" height=\"300\" fill=\"#F5F2EA\"\/>\n<text x=\"330\" y=\"26\" font-family=\"Georgia,serif\" font-size=\"16\" fill=\"#0A1628\" font-weight=\"bold\" text-anchor=\"middle\">Why only some orbits are allowed<\/text>\n<circle cx=\"168\" cy=\"146\" r=\"70\" fill=\"none\" stroke=\"#C5D0DC\" stroke-width=\"1\" stroke-dasharray=\"4 4\"\/>\n<path d=\"M238 146L240 150L242 155L244 160L245 165L245 170L245 175L244 180L242 185L240 189L237 193L233 197L229 200L224 202L220 204L215 206L210 206L205 207L200 206L195 206L191 205L186 205L182 204L178 203L175 202L171 202L168 202L165 202L161 202L158 203L154 204L150 205L145 205L141 206L136 206L131 207L126 206L121 206L116 204L112 202L107 200L103 197L99 193L96 189L94 185L92 180L91 175L91 170L91 165L92 160L94 155L96 150L98 146L101 142L103 138L106 135L109 131L112 128L114 126L116 123L118 120L120 117L122 114L123 111L124 107L126 104L127 100L128 95L130 91L132 87L135 83L138 78L141 74L145 71L149 68L153 65L158 64L163 62L168 62L173 62L178 64L183 65L187 68L191 71L195 74L198 78L201 83L204 87L206 91L208 95L209 100L210 104L212 107L213 111L214 114L216 117L218 120L220 123L222 126L224 128L227 131L230 135L233 138L235 142L238 146\" fill=\"none\" stroke=\"#C8932A\" stroke-width=\"2.4\"\/>\n<circle cx=\"168\" cy=\"146\" r=\"7\" fill=\"#7A1F2B\"\/>\n<circle cx=\"238\" cy=\"146\" r=\"4\" fill=\"#0A1628\"\/>\n<text x=\"168\" y=\"252\" font-family=\"Arial,sans-serif\" font-size=\"13\" fill=\"#0A1628\" text-anchor=\"middle\" font-weight=\"bold\">ALLOWED<\/text>\n<text x=\"168\" y=\"270\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#1F2E47\" text-anchor=\"middle\">3 whole wavelengths fit exactly<\/text>\n<text x=\"168\" y=\"286\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#1F2E47\" text-anchor=\"middle\">the wave joins up with itself<\/text>\n<circle cx=\"492\" cy=\"146\" r=\"70\" fill=\"none\" stroke=\"#C5D0DC\" stroke-width=\"1\" stroke-dasharray=\"4 4\"\/>\n<path d=\"M562 146L565 150L567 155L569 160L570 165L570 170L570 176L568 180L566 185L563 189L560 193L556 196L551 198L546 200L541 201L536 202L531 202L526 202L521 201L517 201L513 201L509 201L505 201L502 201L499 202L495 203L492 205L488 206L484 208L480 210L476 212L471 214L466 215L461 216L455 216L450 215L445 214L440 212L436 209L433 205L430 201L428 196L426 191L425 186L425 181L426 176L427 171L428 166L430 161L431 157L433 153L434 149L435 146L436 143L436 139L436 136L436 132L435 128L434 124L434 120L433 115L433 110L432 105L433 100L434 94L436 90L438 85L441 81L444 77L449 74L453 72L458 71L463 70L468 70L474 71L479 73L483 75L488 78L492 80L496 83L499 86L503 88L506 90L509 92L512 94L515 95L519 95L522 96L526 96L531 97L535 97L540 98L545 99L550 101L555 103L559 105L563 108L567 112L570 116L572 121L573 126L574 131L573 136L572 141L570 146\" fill=\"none\" stroke=\"#142139\" stroke-width=\"2.4\"\/>\n<circle cx=\"492\" cy=\"146\" r=\"7\" fill=\"#7A1F2B\"\/>\n<circle cx=\"562\" cy=\"146\" r=\"3.5\" fill=\"#0A1628\"\/>\n<circle cx=\"570\" cy=\"146\" r=\"3.5\" fill=\"#7A1F2B\"\/>\n<line x1=\"582\" y1=\"128\" x2=\"572\" y2=\"142\" stroke=\"#7A1F2B\" stroke-width=\"1.4\"\/>\n<text x=\"584\" y=\"112\" font-family=\"Arial,sans-serif\" font-size=\"10\" fill=\"#7A1F2B\">wave does not<\/text>\n<text x=\"584\" y=\"124\" font-family=\"Arial,sans-serif\" font-size=\"10\" fill=\"#7A1F2B\">close on itself<\/text>\n<text x=\"492\" y=\"252\" font-family=\"Arial,sans-serif\" font-size=\"13\" fill=\"#0A1628\" text-anchor=\"middle\" font-weight=\"bold\">FORBIDDEN<\/text>\n<text x=\"492\" y=\"270\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#1F2E47\" text-anchor=\"middle\">3.4 wavelengths, no whole-number fit<\/text>\n<text x=\"492\" y=\"286\" font-family=\"Arial,sans-serif\" font-size=\"11\" fill=\"#1F2E47\" text-anchor=\"middle\">the wave cancels itself out<\/text>\n<\/svg>\n<p style=\"text-align:center;font-size:13px;font-style:italic;color:#1F2E47;\">A stable Bohr orbit is one where the electron&#8217;s matter wave closes on itself: 2\u03c0r = n\u03bb.<\/p>\n\n<h3>It completes wave&ndash;particle duality<\/h3>\n\n<p>The <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/modern-physics\/photoelectric-effect\/\">photoelectric effect<\/a> showed light behaving as particles. The de Broglie wavelength showed matter behaving as waves. Together they close the loop: the wave and particle descriptions are two views of one thing.<\/p>\n\n<h3>It needs a correction at high speed<\/h3>\n\n<p>Once a particle approaches a noticeable fraction of the speed of light, momentum is no longer simply mv and <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/modern-physics\/special-relativity\/\">special relativity<\/a> takes over. Use p = &gamma;mv, where &gamma; is the Lorentz factor.<\/p>\n\n<p>The error is not academic. A 100 kV electron microscope beam moves fast enough that the non-relativistic answer is wrong by about 5%.<\/p>\n\n<h3>Momentum is doing all the work<\/h3>\n\n<p>Notice that mass and speed never appear separately &mdash; only as their product. Two particles with identical <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/mechanics\/momentum-and-impulse\/\">momentum<\/a> share a wavelength no matter how the mass and speed are divided between them.<\/p>\n\n<h2>Worked Problems<\/h2>\n\n<p>Every step is shown, with units carried through. Work them yourself first, then check.<\/p>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 1<\/div><div class=\"pf-problem-question\">An electron travels at 2.0 \u00d7 10^6 m\/s. Find its de Broglie wavelength. (mass of an electron = 9.11 \u00d7 10^-31 kg)<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n\n<strong>Solution:<\/strong>\n\nStep 1: Use \u03bb = h \/ (m\u00b7v), with h = 6.63 &times; 10<sup>-34<\/sup> J&middot;s.\n\nStep 2: Find the momentum. p = m\u00b7v = (9.11 &times; 10<sup>-31<\/sup> kg)(2.0 &times; 10<sup>6<\/sup> m\/s) = 1.82 &times; 10<sup>-24<\/sup> kg&middot;m\/s.\n\nStep 3: Divide. \u03bb = (6.63 &times; 10<sup>-34<\/sup> J&middot;s) \/ (1.82 &times; 10<sup>-24<\/sup> kg&middot;m\/s) = 3.64 &times; 10<sup>-10<\/sup> m.\n\n<strong>Answer: 3.6 &times; 10<sup>-10<\/sup> m, or 0.36 nm (2 s.f.)<\/strong>\n\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 2<\/div><div class=\"pf-problem-question\">A cricket ball of mass 0.16 kg is bowled at 40 m\/s. Find its de Broglie wavelength.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n\n<strong>Solution:<\/strong>\n\nStep 1: The same equation applies, because mass and speed are all that matter. \u03bb = h \/ (m\u00b7v).\n\nStep 2: p = (0.16 kg)(40 m\/s) = 6.4 kg&middot;m\/s.\n\nStep 3: \u03bb = (6.63 &times; 10<sup>-34<\/sup> J&middot;s) \/ (6.4 kg&middot;m\/s) = 1.04 &times; 10<sup>-34<\/sup> m.\n\nStep 4: Sanity-check the magnitude. A proton is about 10<sup>-15<\/sup> m wide, so this is roughly 10<sup>19<\/sup> times smaller than a proton. No apparatus could ever detect it.\n\n<strong>Answer: 1.0 &times; 10<sup>-34<\/sup> m (2 s.f.)<\/strong>\n\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 3<\/div><div class=\"pf-problem-question\">An electron is accelerated from rest through a potential difference of 100 V. Find its de Broglie wavelength.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n\n<strong>Solution:<\/strong>\n\nStep 1: Work is done on the electron, so its kinetic energy is K = q\u00b7V.\n\nStep 2: K = (1.60 &times; 10<sup>-19<\/sup> C)(100 V) = 1.60 &times; 10<sup>-17<\/sup> J.\n\nStep 3: Convert energy to momentum. p = sqrt(2\u00b7m\u00b7K) = sqrt(2 &times; 9.11 &times; 10<sup>-31<\/sup> &times; 1.60 &times; 10<sup>-17<\/sup>) = 5.40 &times; 10<sup>-24<\/sup> kg&middot;m\/s.\n\nStep 4: \u03bb = (6.63 &times; 10<sup>-34<\/sup>) \/ (5.40 &times; 10<sup>-24<\/sup>) = 1.23 &times; 10<sup>-10<\/sup> m.\n\nStep 5: Check with the shortcut. \u03bb = 1.226 \/ sqrt(100) = 0.1226 nm. The two agree.\n\n<strong>Answer: 1.23 &times; 10<sup>-10<\/sup> m, or 0.123 nm (3 s.f.)<\/strong>\n\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 4<\/div><div class=\"pf-problem-question\">A neutron has kinetic energy 0.025 eV, typical of a thermal neutron in a reactor. Find its de Broglie wavelength. (mass of a neutron = 1.675 \u00d7 10^-27 kg)<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n\n<strong>Solution:<\/strong>\n\nStep 1: Convert the energy to joules. K = (0.025 eV)(1.60 &times; 10<sup>-19<\/sup> J\/eV) = 4.01 &times; 10<sup>-21<\/sup> J.\n\nStep 2: p = sqrt(2\u00b7m\u00b7K) = sqrt(2 &times; 1.675 &times; 10<sup>-27<\/sup> &times; 4.01 &times; 10<sup>-21<\/sup>) = sqrt(1.343 &times; 10<sup>-47<\/sup>) = 3.66 &times; 10<sup>-24<\/sup> kg&middot;m\/s.\n\nStep 3: \u03bb = (6.63 &times; 10<sup>-34<\/sup>) \/ (3.66 &times; 10<sup>-24<\/sup>) = 1.81 &times; 10<sup>-10<\/sup> m.\n\nStep 4: This is comparable to atomic spacing, which is precisely why thermal neutrons are used to probe crystal structure.\n\n<strong>Answer: 1.81 &times; 10<sup>-10<\/sup> m, or 0.181 nm (3 s.f.)<\/strong>\n\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 5<\/div><div class=\"pf-problem-question\">What speed must an electron have for its de Broglie wavelength to be 0.10 nm?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n\n<strong>Solution:<\/strong>\n\nStep 1: Rearrange \u03bb = h \/ (m\u00b7v) to make v the subject: v = h \/ (m\u00b7\u03bb).\n\nStep 2: Convert the wavelength to metres. \u03bb = 0.10 nm = 1.0 &times; 10<sup>-10<\/sup> m.\n\nStep 3: v = (6.63 &times; 10<sup>-34<\/sup>) \/ (9.11 &times; 10<sup>-31<\/sup> &times; 1.0 &times; 10<sup>-10<\/sup>) = (6.63 &times; 10<sup>-34<\/sup>) \/ (9.11 &times; 10<sup>-41<\/sup>) = 7.27 &times; 10<sup>6<\/sup> m\/s.\n\nStep 4: Check whether relativity is needed. 7.27 &times; 10<sup>6<\/sup> divided by 3.00 &times; 10<sup>8<\/sup> is 2.4% of c, so the non-relativistic formula is safe here.\n\n<strong>Answer: 7.3 &times; 10<sup>6<\/sup> m\/s (2 s.f.)<\/strong>\n\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 6<\/div><div class=\"pf-problem-question\">A proton and an electron are each given a kinetic energy of 100 eV. How many times longer is the electron&#039;s de Broglie wavelength? (proton-to-electron mass ratio = 1836)<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n\n<strong>Solution:<\/strong>\n\nStep 1: At fixed kinetic energy, \u03bb = h \/ sqrt(2\u00b7m\u00b7K), so \u03bb is inversely proportional to sqrt(m).\n\nStep 2: Take the ratio. \u03bb<sub>e<\/sub> \/ \u03bb<sub>p<\/sub> = sqrt(m<sub>p<\/sub> \/ m<sub>e<\/sub>) = sqrt(1836).\n\nStep 3: sqrt(1836) = 42.8.\n\nStep 4: Confirm with numbers. \u03bb<sub>e<\/sub> = 0.123 nm from Problem 3, so \u03bb<sub>p<\/sub> = 0.123 \/ 42.8 = 0.00287 nm.\n\n<strong>Answer: About 43 times longer (\u03bb<sub>e<\/sub> = 0.123 nm, \u03bb<sub>p<\/sub> = 2.87 &times; 10<sup>-3<\/sup> nm)<\/strong>\n\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 7<\/div><div class=\"pf-problem-question\">An electron microscope accelerates electrons through 100 kV. Find the de Broglie wavelength with and without the relativistic correction. (electron rest energy = 0.511 MeV)<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n\n<strong>Solution:<\/strong>\n\nStep 1: Non-relativistic first. \u03bb = 1.226 \/ sqrt(100 000) = 1.226 \/ 316.2 = 3.88 &times; 10<sup>-3<\/sup> nm = 3.88 pm.\n\nStep 2: The relativistic form divides by an extra factor: \u03bb = h \/ sqrt(2\u00b7m\u00b7q\u00b7V\u00b7(1 + qV \/ (2\u00b7m\u00b7c\u00b2))).\n\nStep 3: Evaluate the bracket. qV \/ (2mc\u00b2) = 100 keV \/ (2 &times; 511 keV) = 0.0978, so the correction factor is sqrt(1.0978) = 1.048.\n\nStep 4: \u03bb = 3.88 pm \/ 1.048 = 3.70 pm.\n\nStep 5: The error from ignoring relativity is (3.88 &#8211; 3.70) \/ 3.70 = 4.8%.\n\n<strong>Answer: 3.88 pm non-relativistic, 3.70 pm relativistic, a 4.8% error if uncorrected<\/strong>\n\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 8<\/div><div class=\"pf-problem-question\">In hydrogen&#039;s ground state the electron orbits at r = 5.29 \u00d7 10^-11 m with speed 2.19 \u00d7 10^6 m\/s. Show that exactly one de Broglie wavelength fits around the orbit.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n\n<strong>Solution:<\/strong>\n\nStep 1: Find the electron&#8217;s wavelength. \u03bb = h \/ (m\u00b7v) = (6.63 &times; 10<sup>-34<\/sup>) \/ (9.11 &times; 10<sup>-31<\/sup> &times; 2.19 &times; 10<sup>6<\/sup>).\n\nStep 2: The denominator is 1.995 &times; 10<sup>-24<\/sup> kg&middot;m\/s, so \u03bb = 3.32 &times; 10<sup>-10<\/sup> m.\n\nStep 3: Find the circumference. 2\u00b7\u03c0\u00b7r = 2 &times; 3.1416 &times; 5.29 &times; 10<sup>-11<\/sup> = 3.32 &times; 10<sup>-10<\/sup> m.\n\nStep 4: Divide. (2\u00b7\u03c0\u00b7r) \/ \u03bb = 1.00, so n = 1.\n\n<strong>Answer: n = 1, exactly one wavelength fits, confirming 2\u03c0r = n\u03bb<\/strong>\n\n<\/div><\/details><\/div>\n\n<h2>Frequently Asked Questions<\/h2>\n\n<details class=\"pf-faq-item\"><summary>What is the de Broglie wavelength in simple terms?<\/summary><div class=\"pf-faq-item-answer\">\nIt is the wavelength that any moving object behaves as if it has, equal to Planck&#8217;s constant divided by momentum. A heavy or fast object has large momentum and therefore a tiny wavelength. A light, slow particle like an electron has a wavelength big enough to produce measurable diffraction.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>What are the units of the de Broglie wavelength?<\/summary><div class=\"pf-faq-item-answer\">\nThe SI unit is the metre. Because h is in joule seconds and momentum is in kilogram metres per second, the units divide down to metres exactly. In practice, answers are usually quoted in nanometres for electrons and atoms, or picometres for fast electrons and molecules, since raw metre values are awkwardly small.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>Does the de Broglie wavelength depend on charge?<\/summary><div class=\"pf-faq-item-answer\">\nNo. The formula contains only Planck&#8217;s constant, mass and speed, so a neutral neutron and a charged proton of the same momentum have the same wavelength. Charge enters only indirectly, when a particle is accelerated through a voltage, because there the charge determines how much kinetic energy the particle gains.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>What is the de Broglie wavelength of an electron accelerated through 100 V?<\/summary><div class=\"pf-faq-item-answer\">\nIt is 0.123 nm. Use the shortcut: \u03bb in nanometres equals 1.226 divided by the square root of the voltage, so 1.226 divided by sqrt(100) gives 0.1226 nm. That is close to the spacing between atoms in a crystal, which is why electrons at this energy diffract.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>Is the de Broglie wavelength the same as the Compton wavelength?<\/summary><div class=\"pf-faq-item-answer\">\nNo, they are different quantities. The de Broglie wavelength is h divided by momentum and changes with speed. The Compton wavelength is h divided by mass times c, a fixed property of a particle, and equals 2.43 pm for an electron. They become equal once the momentum reaches mass times c, which happens at about 0.71 of the speed of light &mdash; a kinetic energy near 212 keV for an electron. Below that speed the de Broglie wavelength is the longer of the two; above it, the shorter.\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>Who proved de Broglie&#039;s hypothesis experimentally?<\/summary><div class=\"pf-faq-item-answer\">\nClinton Davisson and Lester Germer confirmed it in 1927 by scattering electrons off a nickel crystal and finding diffraction peaks where the formula predicted. George Paget Thomson demonstrated the same effect through thin films independently that year. Davisson and Thomson shared the 1937 Nobel Prize in Physics for the work.\n<\/div><\/details>\n","protected":false},"excerpt":{"rendered":"<p>Every moving particle has a wavelength given by the de Broglie equation. This guide covers the formula, the electron voltage shortcut, six real examples and eight fully worked problems.<\/p>\n","protected":false},"author":1,"featured_media":687,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6],"tags":[],"class_list":["post-686","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-modern-physics"],"_links":{"self":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts\/686","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/comments?post=686"}],"version-history":[{"count":2,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts\/686\/revisions"}],"predecessor-version":[{"id":698,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts\/686\/revisions\/698"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/media\/687"}],"wp:attachment":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/media?parent=686"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/categories?post=686"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/tags?post=686"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}