Mibvunzo yemuenzaniso uye Kukurukurirana kweMutemo waGauss
Mutemo waGauss ndiwo musimboti mukuru wesimba remagetsi. Unopa nzira inoshanda yekuverenga simba remagetsi rinogadzirwa nekugoverwa kwechaji yemagetsi. Muchinyorwa chino, tichakurukura mienzaniso yakati wandei yematambudziko uye tichakurukura mashandisirwo eMutemo waGauss mumamiriro akasiyana-siyana.
Pfungwa huru yeMutemo waGauss
Tisati tatanga nematambudziko emuenzaniso, ngationgororei pfungwa huru yeMutemo waGauss. Mutemo waGauss unoti kuyerera kwemagetsi kose \( \Phi_E \) kunobva panzvimbo yakavharwa kwakaenzana nechaji yose \( q_{in} \) yakavharirwa pamusoro. Pamasvomhu, Mutemo waGauss unoratidzwa se:
\[ \Phi_E = \oint_S \mathbf{E} \cdot d\mathbf{A} = \frac{q_{in}}{\epsilon_0} \]
di mana:
– \( \Phi_E \) ndiyo nzira yemagetsi inoyerera.
– \( \mathbf{E} \) ndiyo nzvimbo yemagetsi.
– \( \mathbf{A} \) ndiyo vhekita yenzvimbo yepamusoro.
– \( q_{in} \) ndiyo chaji iri mukati menzvimbo yakavharwa.
– \( \epsilon_0 \) ndiyo mvumo yekubvisa vacuum (\( \epsilon_0 \approx 8.85 \times 10^{-12} \, \text{C}^2/(\text{N} \cdot \text{m}^2) \)).
Muenzaniso Mubvunzo 1: Munda weMagetsi muDunhu reConductor rine Hollow
Mubvunzo:
Une bhora rekufambisa risina chinhu rine radius yekunze \( R \) uye huwandu hwechaji \( Q \). Sarudza nzvimbo yemagetsi iri mukati me conductor isina chinhu.
Kukurukurirana:
- Kuziva kweGaussian Surface:
Ngatitii tinosarudza nzvimbo yeGaussian yakatenderera ine radius \( r \) mukati me cavity yekufambisa (apo \( r < R \)). - Kuverengera kweFlux neCharge: Sezvo mukati me conductive sphere iri cavity isina chinhu, charge iri mukati me Gaussian surface iri zero (\( q_{in} = 0 \)). - Kushandiswa kweGauss's Law: Maererano neGauss's Law: \[ \oint_S \mathbf{E} \cdot d\mathbf{A} = \frac{q_{in}}{\epsilon_0} \]
Kukurukurirana:
Kune \( r < R \): - Kuziva Nzvimbo yeGaussian: Sarudza nzvimbo yeGaussian yakatenderera yeradius \( r \) mukati mebhora rakasimba. - Kuverenga Kwechaja: Sezvo chaja yakagoverwa zvakaenzana, chaja iri mukati meradius \( r \) ndeiyi: \[ q_{in} = \rho \cdot \frac{4}{3}\pi r^3 \] uko \( \rho = \frac{Q}{\frac{4}{3}\pi R^3} \). \[ q_{in} = \frac{Q}{\frac{4}{3}\pi R^3} \cdot \frac{4}{3}\pi r^3 = Q \left(\frac{r^3}{R^3}\right) \] - Kushandiswa kweMutemo waGauss: \[ \oint_S \mathbf{E} \cdot d\mathbf{A} = \frac{q_{in}}{\epsilon_0} \] Saka: \[ E \cdot 4\pi r^2 = \frac{Q \left(\frac{r^3}{R^3}\right)}{\epsilon_0} \] Nekurerutsa: \[ E = \frac{Q r}{4\pi \epsilon_0 R^3} \] Saka, munda wemagetsi uri mukati mebhora (\( r < R \)) ndewekuti: \[ E = \frac{Q r}{4\pi \epsilon_0 R^3} \] Kune \( r > R \):
- Kuziva kweGaussian Surface:
Sarudza nzvimbo yeGaussian yakatenderera ine radius \( r \) kunze kwebhora rakasimba.
- Kuverenga Mutoro:
Mutengo wose uri pamusoro peGaussian ndiwo mutengo wose webhora \( Q \).
- Kushandiswa kweMutemo waGauss:
\[
\oint_S \mathbf{E} \cdot d\mathbf{A} = \frac{q_{in}}{\epsilon_0}
\]
Kuti:
\[
E \cdot 4\pi r^2 = \frac{Q}{\epsilon_0}
\]
Nekuita kuti zvinhu zvive nyore:
\[
E = \frac{Q}{4\pi \epsilon_0 r^2}
\]
Saka, munda wemagetsi uri kunze kwebhora (\( r > R \)) ndewekuti:
\[
E = \frac{Q}{4\pi \epsilon_0 r^2}
\]
Mhedziso
Mutemo waGauss unopa chishandiso chine simba chekuongorora minda yemagetsi mumamiriro akasiyana-siyana. Nekusarudza nzvimbo yakakodzera yeGaussian uye kushandisa misimboti yayo yekutanga, tinogona kuverenga kugoverwa kweminda yemagetsi zvinobudirira. Kuburikidza nemienzaniso iri pamusoro, takaona kushandiswa kwemutemo waGauss mumamiriro ezvinhu akadai semunda wemagetsi mudenderedzwa rinofambisa magetsi, ndiro yesimbi isingaperi, charge yepoindi, uye denderedzwa rine charge yakaenzana. Kunzwisisa nekuita zvinoenderana kuchaita kuti mutemo waGauss ushandiswe zvakanaka mukushandiswa kwakasiyana-siyana kwemagetsi.