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Journal ArticleDOI

Vibrational spectra of acid and alkaline glycine salts

TL;DR: In this article, the infrared and Raman spectra of crystalline acid NH CH COOHP Cl and alkaline Na P NHCH COO 32 2 2 glycine salts were recorded and interpreted.
About: This article is published in Vibrational Spectroscopy.The article was published on 1998-03-01 and is currently open access. It has received 142 citations till now. The article focuses on the topics: Zwitterion & Raman spectroscopy.

Summary (1 min read)

1. Introduction

  • Glycine is the simplest protein structural unit and the smallest amino acid that can act as neuroinhibitor w xin mammalian central nervous systems 1,2 .
  • Interesting vibrational features of the infrared spectra of glycine, w xboth in the zwitterionic 2–9 and neutral forms ) Corresponding author.
  • Glycine salts have not previously received much attention.
  • The calculations were carried out using the basic molecular geometry previously determined by neutron diffraction for an individual molecule in the a-crystalline Ž .

2. Experimental and computational methods

  • A-Glycine p.a. q98% was obtained from Merck.
  • Ž .The solution pH)12 was dried in vacuum until complete solvent evaporation, and the crystals washed with methanol.
  • Molecular geometries were fully optimized by the w xforce gradient method using Berny’s algorithm 17 .
  • ŽThe force constants symmetry internal coordi.nates used in the normal coordinate analysis were obtained from the ab initio Cartesian harmonic force Žconstants using the program TRANSFORMER ver. w xsion 2.0 18 .

3. Results and discussion

  • The optimized molecular geometries for the lowest energy conformation of the various molecules studied are shown in Table 1.
  • ŽIn general, the assignments made for glycine both .neutral and zwitterionic form agree with those prew xviously proposed 2–9 and, together with the results of the calculations, were used as a basis for assignment of the spectra of the two salts.
  • When only one internal mode in the PED have a contribution )10%, its value is ommited.
  • As with the n C5O mode, the calculations also overestimate the frequency of the antisymmetrical COOy stretching mode of the zwitterionic form and of the alkaline salt, while they underestimate the frequencies of the symmetrical COOy stretching Ž .vibration see Tables 2 and 4 .

4. General conclusions

  • In addition, although generally not as accurate as the frequencies, the theoretically predicted intensities Ž .both in infrared and in Raman have proved useful in assignment of the spectra.
  • Finally, a dimeric structure of the acid salt of glycine in the crystalline state was found to give best results in the prediction of the vibrational spectra of this compound.

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Citations
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Journal ArticleDOI
TL;DR: In this paper, the authors investigated the synthesis of the simplest amino acid, glycine, by Galactic cosmic-ray particles in extraterrestrialices and provided detailed reaction mechanisms of how the simple amino acid glycine and its isomer can be synthesized via nonequilibrium chemistry in interstellar and cometary ices.
Abstract: We have investigated the synthesis of the simplest aminoacid, glycine, by Galactic cosmic-ray particles in extraterrestrialices.Laboratoryexperimentscombinedwithelectronicstructurecalculationsshowedthatamethylamine molecule [CH3NH2(X 1 A 0 )] can be dissociated through interaction with energetic electrons in the track of a cosmicray particle to form atomic hydrogen and the radicals CH2NH2(X 2 A 0 )a nd CH3NH(X 2 A 0 ). Hydrogen atoms with sufficient kinetic energy could overcome the entrance barrier to add to a carbon dioxide molecule [CO2(X 1 � þ )], yielding a trans-hydroxycarbonyl radical, HOCO(X 2 A 0 ). Neighboring radicals with the correct geometric orientation then recombine to form glycine, NH2CH2COOH(X 1 A), and also its isomer, CH3NHCOOH(X 1 A). These findings expose for the first time detailed reaction mechanisms of how the simplest amino acid glycine and its isomer can be synthesized via nonequilibrium chemistry in interstellar and cometary ices. Our results offer an important alternative to aqueous and photon-induced formation of amino acids in comets and in molecular clouds. These results also predict the existence of a hitherto undetected isomer of glycine in the interstellar medium, suggest that glycine should be observable on Saturn’s moon Titan, and help to account for the synthesis of more complex amino acids in the Murchison and Orgueil meteorites.

216 citations

Journal ArticleDOI
TL;DR: In this paper, the authors studied the stability of amino acid thin films against ultraviolet (UV) irradiation and used those data to predict the survival time of these compounds on and in the Martian regolith.
Abstract: In the framework of international planetary exploration programs, several space missions are planned to search for organics and bio-signatures on Mars. Previous attempts have not detected any organic compounds in the Martian regolith. It is therefore critical to investigate the processes that may affect organic molecules on and below the planet's surface. Laboratory simulations can provide useful data about the reaction pathways of organic material at Mars' surface. We have studied the stability of amino acid thin films against ultraviolet (UV) irradiation and use those data to predict the survival time of these compounds on and in the Martian regolith. We show that thin films of glycine and D-alanine are expected to have half-lives of 22 ± 5 hr and of 3 ± 1 hr, respectively, when irradiated with Mars-like UV flux levels. Modelling shows that the half-lives of the amino acids are extended to the order of 10 7 years when embedded in regolith. These data suggest that subsurface sampling must be a key component of future missions to Mars dedicated to organic detection.

131 citations


Cites methods from "Vibrational spectra of acid and alk..."

  • ...To confirm the obtained absorption data and perform band assignments, the glycine spectra were compared with spectra of glycine in KBr pellets as measured by Ihs et al. (1990), Uvdal et al. (1990) and Rosado et al. (1998)....

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Journal ArticleDOI
TL;DR: In this paper, a combined theoretical and experimental investigation of the interaction between 2D titanium carbide (MXene), Ti3C2Tx, and glycine was presented, which indicated the functionalization of glycine on the Ti-O2 surface, evidenced by the shared electrons between Ti and N atoms.
Abstract: Restacking of two-dimensional (2D) flakes reduces the accessibility of electrolyte ions and is a problem in energy storage and other applications. Organic molecules can be used to prevent restacking and keep the interlayer space open. Here, we report on a combined theoretical and experimental investigation of the interaction between 2D titanium carbide (MXene), Ti3C2Tx, and glycine. From first principle calculations, we presented the functionalization of glycine on the Ti3C2O2 surface, evidenced by the shared electrons between Ti and N atoms. To experimentally validate our predictions, we synthesized flexible freestanding films of Ti3C2Tx/glycine hybrids. X-ray diffraction and X-ray photoelectron spectroscopy confirmed the increased interlayer spacing and possible Ti–N bonding, respectively, which agree with our theoretical predictions. The Ti3C2Tx/glycine hybrid films exhibited an improved rate and cycling performances compared to pristine Ti3C2Tx, possibly due to better charge percolation within expanded Ti3C2Tx.

88 citations

Journal ArticleDOI
TL;DR: It is shown that adsorption is highly dependent of pH and that it occurs either by forming chelate complexes and/or by electrostatic interaction, and these nanoadsorbents can be used as highly efficient separable and reusable materials for removal of toxic metal ions.

85 citations

Journal ArticleDOI
TL;DR: In this article, the evolution of the interstellar ice analogues affected by both thermal heating and vacuum ultraviolet (VUV) photons, in addition to the nature of the formed molecules and the confrontation of their experimental results with astronomical observations are studied.
Abstract: Context. Analyses of dust cometary grains collected by the Stardust spacecraft have shown the presence of amines and amino acids molecules, and among them glycine (NH2 CH2 COOH). We show how the glycine molecule could be produced in the protostellar environments before its introduction into comets.Aims. We study the evolution of the interstellar ice analogues affected by both thermal heating and vacuum ultraviolet (VUV) photons, in addition to the nature of the formed molecules and the confrontation of our experimental results with astronomical observations.Methods. Infrared spectroscopy and mass spectrometry are used to monitor the evolution of the H2 O:CO2 :CH3 NH2 and CO2 :CH3 NH2 ice mixtures during both warming processes and VUV photolysis.Results. We first show how carbon dioxide (CO2 ) and methylamine (CH3 NH2 ) thermally react in water-dominated ice to form methylammonium methylcarbamate [ CH3 NH] [ CH3 NHCOO- ] noted C. We then determine the reaction rate and activation energy. We show that C thermal formation can occurs in the 50–70 K temperature range of a protostellar environment. Secondly, we report that a VUV photolysis of a pure C sample produces a glycine salt, methylammonium glycinate [ CH3 NH] [ NH2 CH2 COO- ] noted G. We propose a scenario explaining how C and subsequently G can be synthesized in interstellar ices and precometary grains.Conclusions. [ CH3 NH] [ CH3 NHCOO- ] could be readily formed and would act as a glycine salt precursor in protostellar environments dominated by thermal and UV processing. We propose a new pathway leading to a glycine salt, which is consistent with the detection of glycine and methylamine within the returned samples of comet 81P/Wild 2 from the Stardust mission.

75 citations


Additional excerpts

  • ...(1) (Waldron 1953; Cabana & Sandorfy 1962; Castellucci 1974; Bossa et al. 2008a); (2) (Rosado et al. 1998); (3) (Bossa et al. 2008a; Durig et al. 1968); (4) (Bossa et al. 2008a)....

    [...]

  • ...A comparison with the spectra of glycine, in either a neutral (NH2CH2COOH) or a zwitterionic form (NH+3 CH2COO −), is indecisive (Gomez-Zavaglia & Fausto 2003; Rosado et al. 1998)....

    [...]

References
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Journal ArticleDOI
TL;DR: In this article, two extended basis sets (termed 5-31G and 6 -31G) consisting of atomic orbitals expressed as fixed linear combinations of Gaussian functions are presented for the first row atoms carbon to fluorine.
Abstract: Two extended basis sets (termed 5–31G and 6–31G) consisting of atomic orbitals expressed as fixed linear combinations of Gaussian functions are presented for the first row atoms carbon to fluorine. These basis functions are similar to the 4–31G set [J. Chem. Phys. 54, 724 (1971)] in that each valence shell is split into inner and outer parts described by three and one Gaussian function, respectively. Inner shells are represented by a single basis function taken as a sum of five (5–31G) or six (6–31G) Gaussians. Studies with a number of polyatomic molecules indicate a substantial lowering of calculated total energies over the 4–31G set. Calculated relative energies and equilibrium geometries do not appear to be altered significantly.

13,036 citations

Journal ArticleDOI
TL;DR: The effect of these drugs for every type of ganglion cell with complex receptive field properties was to make the receptive field more simple, and the orientation selective cells, large field cells, 'on' direction selective cells and uniformity detectors seem to be centre surround cells with special properties that are abolished by these drugs.
Abstract: 1. The effects of picrotoxin and strychnine were tested on the receptive fields of direction sensitive cells, orientation sensitive cells, local edge detectors, uniformity detectors and large field units in the rabbit retina. 2. Picrotoxin eliminated the direction specificity and size specificity of 'on-off' and 'on' directionally sensitive cells for both black and white objects. Picrotoxin also made 'on' directionally sensitive cells responsive to faster velocities. 3. Picrotoxin eliminated the orientation specificity of orientation sensitive cells, and changed the bar-flank arrangement of the receptive field into a centre surround arrangement. Thus, the orientation specificity is due to inhibitory rather than excitatory mechanisms. 4. Picrotoxin altered the speed sensitivity of large field units so that they responded to slow speeds as well as fast ones, like centre surround Y cells. 5. Strychnine abolished the size specificity of local edge detectors and changed their speed specificity so that they responded to faster speeds. 6. Picrotoxin changed a uniformity detector into a sustained on centre cell. 7. Strychnine did not effect the direction specificity of directionally sensitive cells, the orientation specificity of orientation sensitive cells, or the speed specificity of large field units. Picrotoxin did not affect the size specificity of local edge detectors. 8. Picrotoxin and strychnine usually had opposing effects on the transient responses of these units to spots and annuli. In general picrotoxin prolonged and enhanced these responses at both on and off, and strychnine shortened them. 9. The effect of these drugs for every type of ganglion cell with complex receptive field properties was to make the receptive field more simple. The orientation selective cells, large field cells, 'on' direction selective cells and uniformity detectors seem to be centre surround cells with special properties that are abolished by these drugs. The 'on-off' direction selective cells and local edge detectors still on-off receptive fields, but in each case one of the drugs abolished the feature that was the basis for the cell's name.

290 citations

Journal ArticleDOI
TL;DR: The properties of the zwitterionic form of glycine (NH + 3 CH 2 COO − ) using ab initio molecular orbital theory have been computed in this paper, where a shallow minimum on the ZWitterion potential energy surface may be located with certain basis sets that do not contain p-type polarization functions on hydrogen.

210 citations

Journal ArticleDOI
TL;DR: In this article, the authors investigated the infra-red spectra of a number of dimeric carboxylic acids and their deutero (COOD) analogues in the region of 3700 to 1500 cm−1.

166 citations

Frequently Asked Questions (14)
Q1. What are the contributions in "Vibrational spectra of acid and alkaline glycine salts" ?

In this paper, the vibrational spectra of crystalline glycine zwitterion, NH CH COO and the infrared spectrum of this molecule isolated in an argon 3 2, 4, 5 matrix at low temperature 10 K neutral form, was recorded and interpreted. 

Since vibrational spectroscopy can provide the key to elucidation of both structural and dynamical properties and can be used to establish fundamental correlations between these and the chemical or biochemical behaviour of these substances, considerable effort has been dedicated to such studies on glycine under w xvarious experimental conditions 2–12 . 

In the MI-IR spectrum of neutral glycine, as consequence of the isolated status in the Ar matrix, the OH stretching mode appears as a sharp band at 3560 cmy1. 

ŽThe force constants symmetry internal coordi.nates used in the normal coordinate analysis wereobtained from the ab initio Cartesian harmonic force Žconstants using the program TRANSFORMER ver. w xsion 2.0 18 . 

Assignment of the NH and CH stretching modes in the neutral glycine infrared spectrum is straightforward, since these give rise to bands in a clear spectral region. 

Raman spectra were obtained using a SPEX 1403 Ždouble monochromator spectrometer focal distance .0.85 m, aperture fr7.8 , equipped with holographic y1 Žgratings with 1800 grooves mm Ref. 1800- . 

The ab initio calculated force fields were scaled Ž .down using a single scale factor 0.89 , which isaccepted to be the best for the Hartree–Fock level of w xcalculations 21 . 

Because carboxylic acid group intra-dimer inter-actions in the acid salt of glycine considerably inŽ .crease the double bond character of the C–O Hbond when compared with a pure carboxylic acid moiety, the n C–O vibration in this molecule occurs at a much higher frequency than in the isolated neutral form of glycine. 

sThe carbonyl stretching band is present in both neutral glycine and acid salt spectra and can be assigned to the intense infrared bands at 1780 cmy1 Ž . y1 Ž .glycine and 1745 cm acid salt; B mode and tou the doublet of bands at 1737 and 1717 cmy1 in the( )M .T .R osado et al.r V ibrationalSpectroscopy 16 1998 35 – 54 50( )M .T .R osado et al.r V ibrationalSpectroscopy 16 1998 35 – 54 51Ž . 

The t C–N mode calculated value: 206 y1 .cm was previously assigned to the infrared band y1 Ž y1 .at ca. 520 cm Raman: 509 cm , on the basis of neutron diffraction studies. 

In the zwitterionic glycine, this vibration is predicted to occur at a higher freŽquency than in the acid salt calculated value: 320 y1 .cm and is here assigned to the Raman band at 364 cmy1, whose infrared counterpart occurs at 358 y1 w x Žcm 9 . 

The frequencies of the n NH stretching2 modes in the alkaline salt of glycine and, in particular, the n NH vibrations in both crystalline glycine3 and its acid salt are considerably overestimated by the calculations, since these groups participate in intermolecular hydrogen bonding that is not properly considered in the calculations. 

For zwitterionicglycine, the infrared and Raman spectra of the crysŽ .tal a-modification were obtained, while the neutralform was studied by matrix isolation infrared specŽ .troscopy MI-IR , in Argon, at 10 K.a-Glycine p.a. q98% was obtained from Merck. 

In the alkaline salt, this mode gives rise to the infrared band at 1431 cmy1 and to the Raman doublet at 1439 and 1410 cmy1, while in the acid salt it gives the band at 1421 cmy1 Ž .both in the infrared and Raman spectra .